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<?xml-stylesheet type="text/xsl" media="screen" href="/~d/styles/rss2full.xsl"?><?xml-stylesheet type="text/css" media="screen" href="http://feeds.feedburner.com/~d/styles/itemcontent.css"?><rss xmlns:atom="http://www.w3.org/2005/Atom" xmlns:openSearch="http://a9.com/-/spec/opensearch/1.1/" xmlns:blogger="http://schemas.google.com/blogger/2008" xmlns:georss="http://www.georss.org/georss" xmlns:gd="http://schemas.google.com/g/2005" xmlns:thr="http://purl.org/syndication/thread/1.0" xmlns:feedburner="http://rssnamespace.org/feedburner/ext/1.0" version="2.0"><channel><atom:id>tag:blogger.com,1999:blog-3300702123878659843</atom:id><lastBuildDate>Thu, 16 May 2013 11:30:16 +0000</lastBuildDate><title>University of Ottawa NMR Facility Blog</title><description>A blog for the NMR users at the University of Ottawa and all others interested in NMR spectroscopy.</description><link>http://u-of-o-nmr-facility.blogspot.com/</link><managingEditor>noreply@blogger.com (Glenn Facey)</managingEditor><generator>Blogger</generator><openSearch:totalResults>319</openSearch:totalResults><openSearch:startIndex>1</openSearch:startIndex><openSearch:itemsPerPage>25</openSearch:itemsPerPage><atom10:link xmlns:atom10="http://www.w3.org/2005/Atom" rel="self" type="application/rss+xml" href="http://feeds.feedburner.com/UniversityOfOttawaNmrFacilityBlog" /><feedburner:info uri="universityofottawanmrfacilityblog" /><atom10:link xmlns:atom10="http://www.w3.org/2005/Atom" rel="hub" href="http://pubsubhubbub.appspot.com/" /><feedburner:emailServiceId>UniversityOfOttawaNmrFacilityBlog</feedburner:emailServiceId><feedburner:feedburnerHostname>http://feedburner.google.com</feedburner:feedburnerHostname><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3227947031607601247</guid><pubDate>Fri, 05 Apr 2013 19:39:00 +0000</pubDate><atom:updated>2013-04-05T15:45:51.334-04:00</atom:updated><title>Removing t1 Noise from Homoonuclear 2D NMR Data - Video Tutorial </title><description>The often troublesome stripes of vertical noise in 2D NMR spectra are called t1 noise (i.e. noise originating in the t1 domain). When t1 noise occurs in homoonuclear 2D correlation experiments such as &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/06/cosy-90-vs-cosy-45.html" target="_blank"&gt;COSY&lt;/a&gt;, &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/01/1-h-tocsy.html" target="_blank"&gt;TOCSY&lt;/a&gt;,&amp;nbsp;&lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/01/noesy-small-molecules-vs-large.html" target="_blank"&gt;NOESY&lt;/a&gt; or &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/02/noesy-vs-roesy-for-large-molecules.html" target="_blank"&gt;ROESY&lt;/a&gt;,&amp;nbsp;symmetrization can be used&amp;nbsp;to remove a great deal of the noise and make the data more presentable. The technique was described in a &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/10/eliminating-t1-noise-in-2d-homonuclear.html" target="_blank"&gt;previous post&lt;/a&gt; and is demonstrated in this &lt;a href="http://www.youtube.com/watch?v=XhmzjxkPouo&amp;amp;feature=player_detailpage" target="_blank"&gt;video tutorial &lt;/a&gt;using a magnitude COSY spectrum as an example.&lt;br /&gt;
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&lt;a href="http://www.youtube.com/watch?v=XhmzjxkPouo&amp;amp;feature=player_detailpage" target="_blank"&gt;&lt;img border="0" height="301" mta="true" src="http://4.bp.blogspot.com/-1MfCeC1lBrU/UV8pt6t4_YI/AAAAAAAABIM/tqg9AU1eJZw/s400/homo_t1_noise.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/6tc0jimvUOw" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/6tc0jimvUOw/removing-t1-noise-from-homoonuclear-2d.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-1MfCeC1lBrU/UV8pt6t4_YI/AAAAAAAABIM/tqg9AU1eJZw/s72-c/homo_t1_noise.jpg" height="72" width="72" /><thr:total>1</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/04/removing-t1-noise-from-homoonuclear-2d.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-4091755396563447875</guid><pubDate>Thu, 04 Apr 2013 20:18:00 +0000</pubDate><atom:updated>2013-04-04T16:25:09.253-04:00</atom:updated><title>Cable Length and Probe Tuning</title><description>NMR probes can be &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/04/tuning-and-matching-nmr-probe.html" target="_blank"&gt;tuned and matched&lt;/a&gt; on the bench or while in the magnet&amp;nbsp;using a sweep generator and oscilloscope or a specialized tuning box such as the one available through &lt;a href="http://morrisinstruments.com/" target="_blank"&gt;Morris Instruments&lt;/a&gt;.&amp;nbsp; More typically, probe&amp;nbsp;tuning and matching&amp;nbsp;are monitored&amp;nbsp;using the electronics in the NMR console and preamplifier.&amp;nbsp;&amp;nbsp;In either case,&lt;strong&gt; it is important to realize that any filter&amp;nbsp;or cable between the preamplifier and the probe is part of the rf circuit being tuned and should therefore be present while adjusting the tuning and matching capacitors&amp;nbsp;of the probe.&lt;/strong&gt;&amp;nbsp; This is illustrated in the figure below.&amp;nbsp; An NMR probe was tuned and matched using the &lt;em&gt;wobble&lt;/em&gt; function of a Bruker AVANCE spectrometer. There was a&amp;nbsp;bandpass filter and a short cable between the preamplifier and the probe.&amp;nbsp;&amp;nbsp;The tuning curve is shown in the top of the figure.&amp;nbsp; The 90° pulse was measured at 11.25 μsec. The short cable was then replaced with a long cable and the probe tuning and matching capacitors were left unchanged.&amp;nbsp; The tuning curve is shown in the bottom of the figure below.&amp;nbsp; It is clear that the overall circuit is no longer tuned and matched.&amp;nbsp;&amp;nbsp;The 90° pulse was measured at 13.75 μsec using the long cable.&lt;br /&gt;
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&lt;a href="http://4.bp.blogspot.com/-8cZF1qsQ1Ss/UV3fRDLqovI/AAAAAAAABH0/guyMA9iUyxQ/s1600/cable-tuning.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="307" mta="true" src="http://4.bp.blogspot.com/-8cZF1qsQ1Ss/UV3fRDLqovI/AAAAAAAABH0/guyMA9iUyxQ/s400/cable-tuning.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/pV36M5t6c8w" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/pV36M5t6c8w/cable-length-and-probe-tuning.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-8cZF1qsQ1Ss/UV3fRDLqovI/AAAAAAAABH0/guyMA9iUyxQ/s72-c/cable-tuning.jpg" height="72" width="72" /><thr:total>8</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/04/cable-length-and-probe-tuning.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-1274199013437698828</guid><pubDate>Tue, 26 Mar 2013 18:05:00 +0000</pubDate><atom:updated>2013-03-26T14:05:56.446-04:00</atom:updated><title>Removing t1 Noise from Heteronuclear 2D NMR Data - Video Tutorial</title><description>The often troublesome stripes of vertical noise in 2D NMR spectra are called t1 noise (i.e. noise originating in the t1 domain). When t1 noise occurs in hereronuclear 2D correlation experiments such as HMBC, HSQC, HMQC or HOESY, there is a simple trick to remove a great deal of the noise and make the data more presentable. The technique was described in a &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/12/removing-t1-noise-from-heteronuclear.html" target="_blank"&gt;previous post&lt;/a&gt; and is demonstrated in this &lt;a href="http://www.youtube.com/watch?v=PWux92UrWGY&amp;amp;feature=player_detailpage" target="_blank"&gt;video tutorial&lt;/a&gt; using a 19F - 1H&amp;nbsp;&lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/11/19f-1h-hoesy-experiment.html" target="_blank"&gt;HOESY&lt;/a&gt; spectrum as an example.&lt;br /&gt;
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&lt;a href="http://www.youtube.com/watch?v=PWux92UrWGY&amp;amp;feature=player_detailpage" target="_blank"&gt;&lt;img border="0" height="227" src="http://4.bp.blogspot.com/-s6obnyLqhd4/UVHgPo4rWfI/AAAAAAAABHo/NdfK8LdbSxs/s400/t1_noise_vid.jpg" usa="true" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/oTzbQUEfLno" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/oTzbQUEfLno/removing-t1-noise-from-heteronuclear-2d.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-s6obnyLqhd4/UVHgPo4rWfI/AAAAAAAABHo/NdfK8LdbSxs/s72-c/t1_noise_vid.jpg" height="72" width="72" /><thr:total>2</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/03/removing-t1-noise-from-heteronuclear-2d.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-4331232000149084606</guid><pubDate>Mon, 18 Mar 2013 19:33:00 +0000</pubDate><atom:updated>2013-03-26T13:19:25.494-04:00</atom:updated><title>Exponential Line Broadening - Video Tutorial</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
Exponential line broadening is an important NMR data processing tool.&amp;nbsp; It involves multiplying the time domain signal by a decaying exponential function prior to Fourier transforming the data&amp;nbsp;into the frequency domain.&amp;nbsp; It is used to improve the signal-to-noise ratio and&amp;nbsp;is more fully described in a &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/09/exponential-line-broadening.html" target="_blank"&gt;previous post&lt;/a&gt;.&amp;nbsp; The following short &lt;a href="http://www.youtube.com/watch?feature=player_detailpage&amp;amp;v=gvZx0CUhP7k" target="_blank"&gt;tutorial video&lt;/a&gt; demonstrates its use.&lt;/div&gt;
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&lt;a href="http://www.youtube.com/watch?feature=player_detailpage&amp;amp;v=gvZx0CUhP7k" target="_blank"&gt;&lt;img border="0" height="235" psa="true" src="http://4.bp.blogspot.com/-CozKHXyqcTA/UUdrJzrbyqI/AAAAAAAABG8/0FLtL9-4af0/s400/lb_vid.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/iGAJt5cieYA" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/iGAJt5cieYA/exponential-line-broadening-video.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-CozKHXyqcTA/UUdrJzrbyqI/AAAAAAAABG8/0FLtL9-4af0/s72-c/lb_vid.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/03/exponential-line-broadening-video.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-8860584060850396384</guid><pubDate>Wed, 13 Mar 2013 20:13:00 +0000</pubDate><atom:updated>2013-03-13T16:13:07.456-04:00</atom:updated><title>Phasing a 2D NMR Spectrum - Video Tutorial</title><description>The following &lt;a href="http://www.youtube.com/watch?v=YWP-2ODI0hY" target="_blank"&gt;video&lt;/a&gt; demonstrates how to phase a 2D NMR spectrum in TOPSPIN 3.&lt;br /&gt;
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&lt;a href="http://www.youtube.com/watch?v=YWP-2ODI0hY" target="_blank"&gt;&lt;img border="0" height="340" psa="true" src="http://1.bp.blogspot.com/-CYsCw5IN6UQ/UUDc5lQptKI/AAAAAAAABGs/iFjKpU5cMoY/s400/2d_phasing_video.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/v9fPQ6e3bQw" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/v9fPQ6e3bQw/phasing-2d-nmr-spectrum-video-tutorial.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-CYsCw5IN6UQ/UUDc5lQptKI/AAAAAAAABGs/iFjKpU5cMoY/s72-c/2d_phasing_video.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/03/phasing-2d-nmr-spectrum-video-tutorial.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-1040150539165529856</guid><pubDate>Thu, 07 Mar 2013 19:33:00 +0000</pubDate><atom:updated>2013-03-07T14:33:55.601-05:00</atom:updated><title>Thermal Noise in NMR Data</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The &lt;a href="http://www.uottawa.ca/welcome.html" target="_blank"&gt;University of Ottawa&lt;/a&gt; has recently been funded for a 600 MHz NMR spectrometer with a cryogenetically cooled probe.&amp;nbsp; Cryoprobes differ from conventional NMR probes in that the &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/04/electronics-for-simple-single-frequency.html" target="_blank"&gt;rf circuits&lt;/a&gt; and preamplifiers are cooled with cold helium gas while the sample is maintained at ambient temperature.&amp;nbsp; The benefit&amp;nbsp;of cryogenically cooled electronics compared to room temperature electronics&amp;nbsp;is that the thermal noise in the&amp;nbsp;system is reduced at cryogenic temperatures while the NMR signal remains constant for the sample at ambient temperature.&amp;nbsp; The&amp;nbsp;signal-to-noise ratio&amp;nbsp;in an NMR spectrum acquired in a cryoprobe is therefore&amp;nbsp;increased dramatically&amp;nbsp;compared to a conventional probe, typically by a factor of 4.&amp;nbsp; This allows&amp;nbsp;for data collection times on the order of 16 times&amp;nbsp;shorter than those using conventional probes&amp;nbsp;as well as&amp;nbsp;lower detection limits.&amp;nbsp; This principle&amp;nbsp;can be crudely demonstrated by replacing the NMR probe with a 50 Ω&amp;nbsp;&amp;nbsp;load and&amp;nbsp;collecting "NMR" data on the load at both high and low temperatures.&amp;nbsp; The "NMR spectra" in the figure below were collected (without using an rf pulse) on a 50&amp;nbsp;Ω load&amp;nbsp;outside of the magnet at room temperature (left panel) and in a dewar of liquid nitrogen at 77 K (right panel).&amp;nbsp; The noise collected in the 77 K spectrum is 35% lower than that&amp;nbsp;in the room temperature spectrum demonstrating the lower thermal noise&amp;nbsp;at lower temperatures.&lt;/div&gt;
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&lt;a href="http://4.bp.blogspot.com/-XXh_XSbzhc8/UTjqAFGrlmI/AAAAAAAABGM/5pzvSWq7HEw/s1600/thermal_noise.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="382" jsa="true" src="http://4.bp.blogspot.com/-XXh_XSbzhc8/UTjqAFGrlmI/AAAAAAAABGM/5pzvSWq7HEw/s400/thermal_noise.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
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This effect is dramatically increased in a crypoprobe which cools the electronics of both the &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/04/electronics-for-simple-single-frequency.html" target="_blank"&gt;rf probe circuits&lt;/a&gt; and preamplifiers to temperatures much lower than 77 K.&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/iRdFAnun5rA" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/iRdFAnun5rA/thermal-noise-in-nmr-data.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-XXh_XSbzhc8/UTjqAFGrlmI/AAAAAAAABGM/5pzvSWq7HEw/s72-c/thermal_noise.jpg" height="72" width="72" /><thr:total>4</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/03/thermal-noise-in-nmr-data.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3260687968676340399</guid><pubDate>Thu, 14 Feb 2013 19:45:00 +0000</pubDate><atom:updated>2013-02-14T14:45:57.038-05:00</atom:updated><title>Receiver Gain and Signal-to-Noise Ratio</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The signal-to-noise ratio in an NMR spectrum can be affected drastically the choice of the receiver gain setting, so care should be taken to set the receiver gain correctly&amp;nbsp;for optimum results.&amp;nbsp; At very low receiver gain settings, both the signal and the noise use only a fraction of the available digitization levels of the analog-to-digital concertor (ADC).&amp;nbsp; As a result, the intensity of each point in the FID is represented with only a few possible values and the FID is "choppy".&amp;nbsp; This is analogous to a black and white photograph being represented with a coarse gray scale of only a few shades of gray.&amp;nbsp; Just like such a poorly represented photograph, the NMR spectrum contains a great deal of digital noise and therefore a low signal-to-noise ratio.&amp;nbsp; As the receiver gain is increased, the&amp;nbsp;FID&amp;nbsp;is digitized with more available digitization levels.&amp;nbsp; Since the&amp;nbsp;thermal noise in the&amp;nbsp;FID at low receiver gain settings is smaller than or comaparable the size of the digitization step of the&amp;nbsp;ADC, the noise&amp;nbsp;(unlike the signal) will not be amplified by increasing the receiver gain until it exceeds the size of the digitization step of the ADC after which it will be amplified in the same way as the signal.&amp;nbsp; As a result, the signal increases more so than the noise as the receiver gain setting is increased therefore, the signal-to-noise ratio in the NMR spectrum increases steadily as the receiver gain setting is increased.&amp;nbsp; As the receiver gain is increased beyond the point where the thermal noise exceeds the size of the digitization step, both the sginal and the noise can be digitized properly and the signal-to-noise ratio increases much less as a function of receiver gain setting increase.&amp;nbsp; If the receiver gain is increased too much, the signal will exceed the limits of the ADC, the FID will be clipped at the beginning and &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/10/consequences-of-setting-receiver-gain.html" target="_blank"&gt;the NMR spectrum will be severely distorted&lt;/a&gt;.&amp;nbsp; The first figure below shows a series of spectra plotted as a function of the receiver gain setting.&amp;nbsp; The spectra were scaled such that the signals were all of the same height.&amp;nbsp; It is clear that the signal-to-noise ratio increases initially and then levels off.&amp;nbsp; The data are plotted in the second figure.&lt;/div&gt;
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&amp;nbsp;&amp;nbsp;&amp;nbsp; &lt;/div&gt;
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&lt;a href="http://3.bp.blogspot.com/-5vNZhcspVnk/UR018-R6ZnI/AAAAAAAABEo/vsrDRPO4eQ8/s1600/receiver_gain_2_1.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" src="http://3.bp.blogspot.com/-5vNZhcspVnk/UR018-R6ZnI/AAAAAAAABEo/vsrDRPO4eQ8/s400/receiver_gain_2_1.jpg" uea="true" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div class="separator" style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none; clear: both; text-align: center;"&gt;
&lt;a href="http://1.bp.blogspot.com/-Xh7XeHaWW2E/UR02Nqzt-AI/AAAAAAAABE8/BuCG2w-dOrA/s1600/receiver_gain_2_2.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" src="http://1.bp.blogspot.com/-Xh7XeHaWW2E/UR02Nqzt-AI/AAAAAAAABE8/BuCG2w-dOrA/s400/receiver_gain_2_2.jpg" uea="true" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/eckvRtrwQ5I" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/eckvRtrwQ5I/receiver-gain-and-signal-to-noise-ratio.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-5vNZhcspVnk/UR018-R6ZnI/AAAAAAAABEo/vsrDRPO4eQ8/s72-c/receiver_gain_2_1.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/02/receiver-gain-and-signal-to-noise-ratio.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-5023120151751908785</guid><pubDate>Wed, 23 Jan 2013 16:12:00 +0000</pubDate><atom:updated>2013-01-23T14:06:59.821-05:00</atom:updated><title>DNP-NMR</title><description>Dynamic nuclear polarization (DNP) is a signal enhancement technique&amp;nbsp;becoming more and more important in NMR studies of biological samples and materials.&amp;nbsp;&amp;nbsp;Enhancement of NMR signals is accomplished by doping samples with stable free radicals.&amp;nbsp; The trapped free radicals in the cooled solid sample are irradiated continuously at the&amp;nbsp;EPR microwave frequency.&amp;nbsp; Microwaves are generated by a gyrotron (which requires iits own superconducting magnet in addition to the superconducting NMR magnet).&amp;nbsp; The microwave radiation is introduced into the NMR probe by way of a wave guide.&amp;nbsp; While&amp;nbsp;the unpaired electrons are irradiated,&amp;nbsp;the population distribution of the Zeeman states of NMR active nuclei are modified&amp;nbsp;providing more polarization and therefore a large NMR sensitivity enhancement.&amp;nbsp;&amp;nbsp;Typically the polarized protons in the sample are used as a &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/12/cross-polarization.html" target="_blank"&gt;cross polarizatuion&lt;/a&gt; source&amp;nbsp;for less abundant nuclides.&amp;nbsp; The data are typically acquired at low temperature with &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/11/magic-angle-spinning.html" target="_blank"&gt;magic angle spinning&lt;/a&gt;.&amp;nbsp; The overall NMR enhancement is typically one or two orders of magnitude when one compares NMR spectra acquired with the microwave source on vs off.&amp;nbsp; &lt;a href="http://www.bruker.com/products/mr/nmr/dnp-nmr/overview.html" target="_blank"&gt;Commercial DNP-NMR&amp;nbsp;instruments&lt;/a&gt; are now available. &lt;br /&gt;
&lt;br /&gt;
&lt;a href="http://www.blogger.com/profile/15272105919342829243" target="_blank"&gt;Thorsten Maly&lt;/a&gt; authors a very informative &lt;a href="http://blog.bridge12.com/" target="_blank"&gt;BLOG&lt;/a&gt; on all things DNP-NMR.&amp;nbsp; I encourage you to take a look at it.&lt;br /&gt;
&lt;br /&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://1.bp.blogspot.com/-UNnM4gBPdYo/UQAKz6JBdaI/AAAAAAAABDw/7Yk0rQPPcbE/s1600/DNP.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="281" oea="true" src="http://1.bp.blogspot.com/-UNnM4gBPdYo/UQAKz6JBdaI/AAAAAAAABDw/7Yk0rQPPcbE/s400/DNP.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/8hfYX0v2H28" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/8hfYX0v2H28/dnp-nmr.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-UNnM4gBPdYo/UQAKz6JBdaI/AAAAAAAABDw/7Yk0rQPPcbE/s72-c/DNP.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2013/01/dnp-nmr.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3274984421540638341</guid><pubDate>Fri, 21 Dec 2012 19:03:00 +0000</pubDate><atom:updated>2012-12-21T14:03:29.381-05:00</atom:updated><title>A Useful Winter Emulsion</title><description>The winters in Ottawa are cold (and arguably miserable).&amp;nbsp;&amp;nbsp;The cold can cause&amp;nbsp;many detrimental effects on ones comfort.&amp;nbsp; One particularly uncomfortable condition usually disappears within a day or two&amp;nbsp;on visiting the&amp;nbsp;warm sunny Caribbean.&amp;nbsp; The proton and carbon NMR spectra below were acquired on a very useful emulsion used by many cold Canadians to keep&amp;nbsp;this condition at bay.&amp;nbsp; &amp;nbsp; What is the emulsion?&lt;br /&gt;
&lt;br /&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://4.bp.blogspot.com/-cI34BbyPG70/UNSyDYn0l1I/AAAAAAAABC4/YIsD2OS_TjY/s1600/cream.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" eea="true" height="327" src="http://4.bp.blogspot.com/-cI34BbyPG70/UNSyDYn0l1I/AAAAAAAABC4/YIsD2OS_TjY/s400/cream.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;br /&gt;
Happy Comfortable Holidays !!!!&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/ml0Dm_f1OV0" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/ml0Dm_f1OV0/a-useful-winter-emulsion.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-cI34BbyPG70/UNSyDYn0l1I/AAAAAAAABC4/YIsD2OS_TjY/s72-c/cream.jpg" height="72" width="72" /><thr:total>1</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/12/a-useful-winter-emulsion.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-2099261151783518366</guid><pubDate>Fri, 07 Dec 2012 21:08:00 +0000</pubDate><atom:updated>2012-12-10T09:53:32.778-05:00</atom:updated><title>NMR Tube Thickness and Signal-to-Noise-Ratio</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The amount of NMR signal is expected to be proportional to the&amp;nbsp;amount of sample inside the coil of the NMR probe.&amp;nbsp; As a result, the signal-to-noise ratio for&amp;nbsp;samples run in NMR tubes&amp;nbsp;with thick walls&amp;nbsp;is expected to be lower than that for comparable samples run in&amp;nbsp;NMR tubes with thinner walls due to a reduced filling factor of the NMR probe coil.&amp;nbsp; I was curious to see how much of a difference in signal-to-noise ratio there would&amp;nbsp;be.&amp;nbsp; 0.68 mL of&amp;nbsp; CDCl&lt;sub&gt;3&lt;/sub&gt;&amp;nbsp;(99.8 % D) was put in 5 mm NMR tubes&amp;nbsp;with wall thicknesses&amp;nbsp;of 0.38 mm and 0.80 mm.&amp;nbsp; The NMR tubes were &lt;a href="http://www.newera-spectro.com/" target="_blank"&gt;New Era Entepprises&lt;/a&gt; NE-MP&amp;nbsp;5 (4.20 mm ID) and &lt;a href="http://www.nmrtubes.com/" target="_blank"&gt;Norell&lt;/a&gt; S-300 (3.43&amp;nbsp;mm ID), respectively.&amp;nbsp; The samples are shown here:&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none; clear: both; text-align: center;"&gt;
&lt;a href="http://3.bp.blogspot.com/-Xo7UJjGdAaA/UMJXmLokiGI/AAAAAAAABB8/Q2zZEz5UnN8/s1600/tube_pic.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="640" nea="true" src="http://3.bp.blogspot.com/-Xo7UJjGdAaA/UMJXmLokiGI/AAAAAAAABB8/Q2zZEz5UnN8/s640/tube_pic.jpg" width="392" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The height of the sample column for the thick-walled tube is obviously higher due to the smaller inner diameter of the tube.&amp;nbsp; In this case, much of the sample&amp;nbsp;will be&amp;nbsp;"invisible" to the NMR measurement as it is outside of the active NMR probe coil volume and therefore "wasted".&amp;nbsp; Single scan proton NMR spectra were run for these samples on a 300 MHz instrument.&amp;nbsp; A third sample was prepared by removing some sample from the thick-walled NMR tube such that the column height was equal to the sample in the thin-walled tube.&amp;nbsp; The volume for this sample was 0.45 mL and it was run under identical conditions to the other two.&amp;nbsp; Care was taken to shim the magnet and &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2008/04/tuning-and-matching-nmr-probe.html" target="_blank"&gt;tune and match the NMR probe&lt;/a&gt; reproducibly.&amp;nbsp; The data, processed with 0.5 Hz of line broadening,&amp;nbsp;are plotted side by side&amp;nbsp;in the figure below:&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://4.bp.blogspot.com/-n6k6IElNVjc/UMJV_3hYTgI/AAAAAAAABBs/pGa5C6op1Gw/s1600/tube_SN.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" nea="true" src="http://4.bp.blogspot.com/-n6k6IElNVjc/UMJV_3hYTgI/AAAAAAAABBs/pGa5C6op1Gw/s400/tube_SN.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;
The 0.68&amp;nbsp;mL&amp;nbsp;sample in the thin-walled tube (blue) gave a signal-to-noise-ratio of 566.&amp;nbsp;&amp;nbsp;The 0.68&amp;nbsp;mL&amp;nbsp;sample in the thick-walled tube (red) gave a signal-to-noise-ratio of 339 and the 0.45&amp;nbsp;mL&amp;nbsp;sample in the thick-walled tube (green) gave a signal-to-noise-ratio of 369.&amp;nbsp; The difference in the signal-to-noise-ratios&amp;nbsp;for the two samples in the thick-walled NMR tube may very well be the same within experimental error as the signal-to-noise-ratio is very&amp;nbsp;sensitive to magnet shimming.&amp;nbsp; One would expect them to be similar based on the fact that both samples&amp;nbsp;have volumes exceeding the active volume of the probe coil.&amp;nbsp;&amp;nbsp;From the data, one sees a 35-40% loss in signal&amp;nbsp;on going&amp;nbsp;from a thin-walled to a thick-walled NMR tube.&amp;nbsp; It is instructive to look at the&amp;nbsp;volume corrected&amp;nbsp;signal-to-noise-ratio of the 0.45 mL sample in the thick-walled&amp;nbsp;NMR tube compared to the 0.68 mL sample in the thin-walled NMR tube.&amp;nbsp; If the signal-to-noise ratio for the 0.45 mL sample is&amp;nbsp;multiplied by&amp;nbsp;(0.68 mL/0.45 mL), the corrected&amp;nbsp;value is 557 which is&amp;nbsp;very likely the same as the 566 value measured for the 0.68 mL sample in the thin-walled NMR tube within experimental error.&amp;nbsp;&amp;nbsp;From these observations, one can conclude that the&amp;nbsp;signal-to-noise-ratio&amp;nbsp;loss is entirely due to the reduction in sample volume within the coil.&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/7KHAx1mFE_w" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/7KHAx1mFE_w/nmr-tube-thickness-and-signal-to-noise.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-Xo7UJjGdAaA/UMJXmLokiGI/AAAAAAAABB8/Q2zZEz5UnN8/s72-c/tube_pic.jpg" height="72" width="72" /><thr:total>2</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/12/nmr-tube-thickness-and-signal-to-noise.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3508934456029358680</guid><pubDate>Mon, 19 Nov 2012 21:16:00 +0000</pubDate><atom:updated>2012-11-20T13:05:53.317-05:00</atom:updated><title>EZNMR at the University of Ottawa</title><description>The &lt;a href="http://www.nmr.uottawa.ca/en/welcome.html" target="_blank"&gt;NMR Facility&lt;/a&gt; at the &lt;a href="http://www.uottawa.ca/welcome.html" target="_blank"&gt;University of Ottawa&lt;/a&gt; is equipped with &lt;a href="http://www.nmr.uottawa.ca/?q=en/spectrometers.html" target="_blank"&gt;eight NMR spectrometers&lt;/a&gt; and&amp;nbsp;has on the order of 100&amp;nbsp;hands-on users at the graduate and post-doctoral level.&amp;nbsp; Like any university NMR facility, the users enter at&amp;nbsp;varying knowledge and experience levels: from "What does NMR stand for?" to "How do&amp;nbsp;I do a shearing transform for my 5QMAS data set?".&amp;nbsp; Also, the attitude of the user's supervisors&amp;nbsp;varies considerably.&amp;nbsp; Some&amp;nbsp;supervisors want their students to spend as little time in the NMR lab as possible by&amp;nbsp;collecting all of their data in automation&amp;nbsp;with a sample changer so they can maximize their time&amp;nbsp;at the bench.&amp;nbsp; &amp;nbsp;Others want their students to learn how to collect the best possible data and fully understand the NMR measurements they make.&amp;nbsp; There is no doubt that collecting NMR data under complete automation is&amp;nbsp;incredibly time-efficient however, collecting data in this way&amp;nbsp;teaches the student nothing about NMR measurements.&amp;nbsp; On the other hand,&amp;nbsp;learning to use&amp;nbsp;NMR spectrometers manually, at the most fundamental level,&amp;nbsp;to collect the best possible data, requires a great deal of knowledge (both general and instrument-specific) and although&amp;nbsp;it is the most educationally rewarding, it certainly provides less&amp;nbsp;overall sample throughput.&amp;nbsp;&amp;nbsp;In our facility, almost all students are first given 10 minutes&amp;nbsp;of training,&amp;nbsp;on how to collect NMR data under complete automation using our&amp;nbsp;only fully automated instrument.&amp;nbsp; Running an NMR spectrometer in this way&amp;nbsp;requires absolutely no knowledge of NMR spectroscopy.&amp;nbsp;&amp;nbsp;Most users are also interested in using the other less automated instruments.&amp;nbsp; These students are provided with as much training as they desire.&amp;nbsp;&amp;nbsp;&amp;nbsp;The job of the NMR facility is to educate and satisfy the needs or each user.&amp;nbsp; Doing so, requires finding a "happy medium" between complete automation and complete manual spectrometer operation and using that medium as a minimum training standard.&amp;nbsp; For the last ten years or so, the "happy medium" used by&amp;nbsp;the &lt;a href="http://www.uottawa.ca/welcome.html" target="_blank"&gt;University of Ottawa&lt;/a&gt;&amp;nbsp;to run&amp;nbsp;four of it its Bruker&amp;nbsp;NMR instruments is based on a customized button panel approach.&amp;nbsp; We&amp;nbsp;have&amp;nbsp;written button panels specific to each instrument and call the option &lt;strong&gt;EZNMR.&lt;/strong&gt;&amp;nbsp; We have included &lt;strong&gt;EZNMR&lt;/strong&gt; as an&amp;nbsp;entry on the top TOPSPIN menu bar.&amp;nbsp; Clicking the &lt;strong&gt;EZNMR&lt;/strong&gt; option opens up a button panel like the one shown below, used on our AVANCE 500 spectrometer.&amp;nbsp; &lt;br /&gt;
&lt;br /&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://1.bp.blogspot.com/-5dy-nsYSljs/UKqcpordSrI/AAAAAAAABAo/HcRDggdV12w/s1600/panel_1D.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="640" rea="true" src="http://1.bp.blogspot.com/-5dy-nsYSljs/UKqcpordSrI/AAAAAAAABAo/HcRDggdV12w/s640/panel_1D.jpg" width="238" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
Each button either issues a command, runs a macro or runs an "au program".&amp;nbsp; Some of our students use exclusively this panel to collect their data.&amp;nbsp; The advantage to using such a system is that the student must at least learn all of the steps involved with collecting the data.&amp;nbsp; A typical &lt;strong&gt;EZNMR&lt;/strong&gt; session involves simply following the button panel from top to bottom.&amp;nbsp; If the probe contains a sample, it is ejected with the &lt;strong&gt;EJECT&lt;/strong&gt; button.&amp;nbsp; A new sample is lowered into the probe with the &lt;strong&gt;INSERT&lt;/strong&gt; button.&amp;nbsp; The deuterium lock is established by pressing the &lt;strong&gt;LOCK&lt;/strong&gt; button which prompts the user for the solvent and then establishes the lock.&amp;nbsp;&amp;nbsp; The &lt;strong&gt;SHIM&lt;/strong&gt; button first calls up a standard set of shims and then initiates a gradient shimming routine.&amp;nbsp;&amp;nbsp;After the magnet is&amp;nbsp;shimmed, the user presses any one of the green buttons&amp;nbsp;depending on which NMR measurement they intend to carry out.&amp;nbsp; Pressing&amp;nbsp;one of these buttons prompts the user to define a data set and then calls up a&amp;nbsp;reasonable set of parameters into that data set.&amp;nbsp;&amp;nbsp;If desired,&amp;nbsp;the user&amp;nbsp;can change the number of scans or some of the parameters by pressing the &lt;strong&gt;SCANS&lt;/strong&gt; or &lt;strong&gt;PARAMETERS&lt;/strong&gt; buttons.&amp;nbsp; The probe is then tuned using the &lt;strong&gt;TUNE&lt;/strong&gt; button.&amp;nbsp; The &lt;strong&gt;START&lt;/strong&gt; button optimizes the receiver gain and begins collecting the data.&amp;nbsp; Once started, the data can be processed at any time using the &lt;strong&gt;Proc 1D&lt;/strong&gt; button or halted using the &lt;strong&gt;HALT&lt;/strong&gt; button.&amp;nbsp; We use a similar button panel for the commonly used 2D NMR experiments which can be called up from the 1D panel.&amp;nbsp; It is shown here:&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://1.bp.blogspot.com/-9i4aXClPr5k/UKqc9315FII/AAAAAAAABAw/L4fzu79mNA8/s1600/panel_2D.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="320" rea="true" src="http://1.bp.blogspot.com/-9i4aXClPr5k/UKqc9315FII/AAAAAAAABAw/L4fzu79mNA8/s320/panel_2D.jpg" width="224" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The advantages to using this system&amp;nbsp;are:&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; It is highly customizable for the hardware of each instrument as it is based on macros and "au programs".&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
- &amp;nbsp;It&amp;nbsp;can be added to as demands change.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; All NMR spectrometers using &lt;strong&gt;EZNMR&lt;/strong&gt; look pretty much the same&amp;nbsp;so&amp;nbsp;instrument specific training&amp;nbsp;is less of an issue.&amp;nbsp;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; Students can begin running NMR experiments very quickly.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; Students are more likely to ask questions about each step and can learn at their own pace while maintaining high sample throughput.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; Its use is entirely optional.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
-&amp;nbsp; It is much more time-efficient than complete manual operation.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;br /&gt;&lt;/div&gt;
Students are of course encouraged to learn more about spectrometer operation than is available through the &lt;strong&gt;EZNMR&lt;/strong&gt; buton panels.&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=HNnS4ZMxX-o:8K0Q44kiiik:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/HNnS4ZMxX-o" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/HNnS4ZMxX-o/eznmr-at-university-of-ottawa.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-5dy-nsYSljs/UKqcpordSrI/AAAAAAAABAo/HcRDggdV12w/s72-c/panel_1D.jpg" height="72" width="72" /><thr:total>2</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/11/eznmr-at-university-of-ottawa.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-8034502918433215134</guid><pubDate>Thu, 15 Nov 2012 20:32:00 +0000</pubDate><atom:updated>2012-11-15T15:48:59.739-05:00</atom:updated><title>19F NOESY</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
Two-dimensional &lt;sup&gt;1&lt;/sup&gt;H &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2007/11/what-mixing-time-should-i-use-for-my-2d.html" target="_blank"&gt;NOESY&lt;/a&gt; data are routinely used to&amp;nbsp;assign specific stereo-isomers based on&amp;nbsp;the proton&amp;nbsp;nuclear Overhauser effects (NOE's)&amp;nbsp;which are strongly correlated to inter-proton&amp;nbsp;distances through space.&amp;nbsp; For example, NOE's may be observed for&amp;nbsp;&lt;em&gt;cis-&lt;/em&gt; protons across a double bond but not observed for &lt;em&gt;trans-&lt;/em&gt; protons.&amp;nbsp; The same technique can be used with &lt;sup&gt;19&lt;/sup&gt;F in fluorinated compounds to gauge the inter-fluorine distance and assign stereochemistry.&amp;nbsp; The figure below shows the &lt;sup&gt;19&lt;/sup&gt;F NOESY spectrum of a fluorine containing cobalt complex.&lt;/div&gt;
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&lt;br /&gt;&lt;/div&gt;
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&lt;a href="http://2.bp.blogspot.com/-9U0_yr29qlU/UKVPofiVVHI/AAAAAAAAA_w/u0OF6dTTWu4/s1600/19F_NOESY.jpg" imageanchor="1" style="clear: left; cssfloat: left; float: left; margin-bottom: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" rea="true" src="http://2.bp.blogspot.com/-9U0_yr29qlU/UKVPofiVVHI/AAAAAAAAA_w/u0OF6dTTWu4/s400/19F_NOESY.jpg" width="400" /&gt;&lt;/a&gt;From the 1D-&lt;sup&gt;19&lt;/sup&gt;F NMR spectrum, it is not clear which fluorine atoms are on the same or opposite sides of the four membered cobalt containing ring.&amp;nbsp; The 2D-&lt;sup&gt;19&lt;/sup&gt;F NOESY spectrum, on the other hand, shows strong NOE cross peaks between fluorine&amp;nbsp;C and&amp;nbsp;both&amp;nbsp;A and E indicating that&amp;nbsp;C, A and E&amp;nbsp;are on the same side of the ring.&amp;nbsp; There are also strong cross peaks between fluorine D,&amp;nbsp;and both B&amp;nbsp;and F indicating that&amp;nbsp;D,&amp;nbsp;B anf F&amp;nbsp;are on the same side of the ring.&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
&lt;strong&gt;&lt;em&gt;Thank you&amp;nbsp;to Graham Lee (of &lt;/em&gt;&lt;/strong&gt;&lt;a href="http://www.catalysis.uottawa.ca/baker-group/" target="_blank"&gt;&lt;strong&gt;&lt;em&gt;Dr. R.T. Baker's research group&lt;/em&gt;&lt;/strong&gt;&lt;/a&gt;&lt;strong&gt;&lt;em&gt;&amp;nbsp;at the &lt;/em&gt;&lt;/strong&gt;&lt;a href="http://www.uottawa.ca/welcome.html" target="_blank"&gt;&lt;strong&gt;&lt;em&gt;University of Ottawa&lt;/em&gt;&lt;/strong&gt;&lt;/a&gt;&lt;strong&gt;&lt;em&gt;) for kindly providing the&amp;nbsp;sample and sharing his data.&amp;nbsp;&lt;/em&gt;&lt;/strong&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=5et6YTv0z3U:xsOPxB4RlOM:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/5et6YTv0z3U" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/5et6YTv0z3U/19-f-noesy.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://2.bp.blogspot.com/-9U0_yr29qlU/UKVPofiVVHI/AAAAAAAAA_w/u0OF6dTTWu4/s72-c/19F_NOESY.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/11/19-f-noesy.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-652417139463820460</guid><pubDate>Mon, 22 Oct 2012 20:30:00 +0000</pubDate><atom:updated>2012-10-23T10:10:56.114-04:00</atom:updated><title>Isotope Effects and the 19F - 13C HMQC Spectrum of Trifluoroacetic Acid</title><description>&lt;div class="separator" style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none; clear: both; text-align: center;"&gt;
&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2010/06/19-f-13-c-hmqc.html" target="_blank"&gt;&lt;sup&gt;19&lt;/sup&gt;F - &lt;sup&gt;13&lt;/sup&gt;C HMQC&lt;/a&gt; spectrum of trifluoroacetic acid is shown in the figure below.&lt;/div&gt;
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&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none; clear: both; text-align: center;"&gt;
&lt;a href="http://4.bp.blogspot.com/-roN1Zav9lO8/UIWplTlt8WI/AAAAAAAAA-o/G0N2j7vkqns/s1600/tfa1.jpg" imageanchor="1" style="clear: right; cssfloat: right; float: right; margin-bottom: 1em; margin-left: 1em;"&gt;&lt;img border="0" height="283" oea="true" src="http://4.bp.blogspot.com/-roN1Zav9lO8/UIWplTlt8WI/AAAAAAAAA-o/G0N2j7vkqns/s400/tfa1.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The data were collected with a delay appropriate for a &lt;sup&gt;19&lt;/sup&gt;F - &lt;sup&gt;13&lt;/sup&gt;C J&amp;nbsp; coupling constant between the &lt;sup&gt;1&lt;/sup&gt;J&lt;sub&gt;F-C&lt;/sub&gt; coupling constant of 284&amp;nbsp;Hz and the &lt;sup&gt;2&lt;/sup&gt;J&lt;sub&gt;F-C&lt;/sub&gt; coupling constant of&amp;nbsp;44 Hz.&amp;nbsp; The top and side traces are the one-pulse &lt;sup&gt;19&lt;/sup&gt;F and &lt;sup&gt;13&lt;/sup&gt;C spectra, respectively.&amp;nbsp; Why are the HMQC responses not at the same &lt;sup&gt;19&lt;/sup&gt;F chemical shift and why aren't they correlated to the peak in the &lt;sup&gt;19&lt;/sup&gt;F spectrum?&amp;nbsp; In order to answer these questions one must take into consideration the &lt;sup&gt;19&lt;/sup&gt;F - &lt;sup&gt;12, 13&lt;/sup&gt;C isotope effects.&amp;nbsp; The chemical shift of the fluorine depends on whether&amp;nbsp;it is bound to a&amp;nbsp;&lt;sup&gt;12&lt;/sup&gt;C or a &lt;sup&gt;13&lt;/sup&gt;C.&amp;nbsp; The effect is largest&amp;nbsp;across one bond and gets smaller&amp;nbsp;over multiple bonds.&amp;nbsp; The &lt;sup&gt;19&lt;/sup&gt;F NMR spectrum for trifluoroacetic acid is shown in the figure below with and without &lt;sup&gt;13&lt;/sup&gt;C broadband decoupling in the upper and lower traces, respectively.&lt;/div&gt;
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&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://4.bp.blogspot.com/-uKTSsQ5RzNU/UIWqyfH2QKI/AAAAAAAAA-w/MzjNcUujjiY/s1600/tfa2.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="278" oea="true" src="http://4.bp.blogspot.com/-uKTSsQ5RzNU/UIWqyfH2QKI/AAAAAAAAA-w/MzjNcUujjiY/s400/tfa2.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
Approximately 98% of the trifluoroacetic acid is the&amp;nbsp;&lt;sup&gt;12&lt;/sup&gt;CF&lt;sub&gt;3&lt;/sub&gt;-&lt;sup&gt;12&lt;/sup&gt;COOH isotopomer, giving rise to a large singlet plotted off-scale in the figure.&amp;nbsp;Approximately 1% of the signal is from the &lt;sup&gt;13&lt;/sup&gt;CF&lt;sub&gt;3&lt;/sub&gt;-&lt;sup&gt;12&lt;/sup&gt;COOH isotoponer giving rise to a doublet with &lt;sup&gt;1&lt;/sup&gt;J&lt;sub&gt;F-C&lt;/sub&gt; =&amp;nbsp;284 Hz and approximately 1% of the signal is from the &lt;sup&gt;12&lt;/sup&gt;CF&lt;sub&gt;3&lt;/sub&gt;-&lt;sup&gt;13&lt;/sup&gt;COOH isotoponer giving rise to a doublet with &lt;sup&gt;2&lt;/sup&gt;J&lt;sub&gt;F-C&lt;/sub&gt; =&amp;nbsp;44 Hz.&amp;nbsp; All of these signals are clearly present in the lower trace of the figure.&amp;nbsp; When &lt;sup&gt;13&lt;/sup&gt;C broadband decoupling is applied, the doublets collapse into singlets.&amp;nbsp; The singlets from each of the isotopomers are resolved in the top trace.&amp;nbsp; The one-bond &lt;sup&gt;19&lt;/sup&gt;F - &lt;sup&gt;12, 13&lt;/sup&gt;C isotope effect is 0.13 ppm and the two-bond effect is 0.02 ppm.&amp;nbsp; The figure below shows the same HMQC data with the spectrum from the top trace used as a projection.&lt;/div&gt;
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&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://2.bp.blogspot.com/-pMrnND8VmXk/UIWrSfZAmEI/AAAAAAAAA-4/ON5PrpP4KQ8/s1600/tfa3.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="298" oea="true" src="http://2.bp.blogspot.com/-pMrnND8VmXk/UIWrSfZAmEI/AAAAAAAAA-4/ON5PrpP4KQ8/s400/tfa3.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
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One can see that the HMQC responses are correlated to their respective isotopomers.&amp;nbsp; These effects are also present in &lt;sup&gt;1&lt;/sup&gt;H - &lt;sup&gt;13&lt;/sup&gt;C HMQC spectra, but the &lt;sup&gt;1&lt;/sup&gt;H - &lt;sup&gt;12, 13&lt;/sup&gt;C isotope effect is much smaller than the &lt;sup&gt;19&lt;/sup&gt;F - &lt;sup&gt;12, 13&lt;/sup&gt;C isotope effect.&amp;nbsp;&amp;nbsp;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/VUTNF1qRH6I" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/VUTNF1qRH6I/isotope-effects-and-19-f-13-c-hmqc.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-roN1Zav9lO8/UIWplTlt8WI/AAAAAAAAA-o/G0N2j7vkqns/s72-c/tfa1.jpg" height="72" width="72" /><thr:total>1</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/10/isotope-effects-and-19-f-13-c-hmqc.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-8167170081516109627</guid><pubDate>Fri, 17 Aug 2012 18:46:00 +0000</pubDate><atom:updated>2012-08-17T14:47:18.525-04:00</atom:updated><title>Measurement of Long Range C H Coupling Constants</title><description>The stereochemistry of compounds is assigned very often with proton - proton NOE's by applying the 2D NOESY technique or the &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2009/05/selective-1d-gradient-noesy.html" target="_blank"&gt;1D selective gradient NOESY&lt;/a&gt; technique.&amp;nbsp; These methods fail, however when the distance between protons is too large to measure an NOE.&amp;nbsp; When faced with this situation, it may be possible to measure long range proton - carbon coupling constants which are able to provide the necessary information.&amp;nbsp;&amp;nbsp;Three-bond carbon -&amp;nbsp;proton couplings follow a Karplus relationship where the magnitude of the coupling constant&amp;nbsp;is related to the dihedral angle between the carbon and the proton.&amp;nbsp; In some cases, these dihedral angles&amp;nbsp;may be used to assign the stereochemistry.&amp;nbsp; Coupling constants are largest for dihedral angles of 0° and 180° and smallest for dihedral angles of 90°. The simplest way to measure the&amp;nbsp;long range coupling constants is to collect a &lt;sup&gt;13&lt;/sup&gt;C NMR spectrum without &lt;sup&gt;1&lt;/sup&gt;H decoupling.&amp;nbsp; These spectra can be very complicated as can be seen from the figure below&amp;nbsp;showing the C2 and C3 aromatic carbons of toluene.&lt;br /&gt;
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&lt;a href="http://1.bp.blogspot.com/-GAK0eeIlyyg/UC6PMzM7LnI/AAAAAAAAA9o/ug_eQneqHOk/s1600/jres1.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" mda="true" src="http://1.bp.blogspot.com/-GAK0eeIlyyg/UC6PMzM7LnI/AAAAAAAAA9o/ug_eQneqHOk/s400/jres1.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: left;"&gt;
Extracting specific long range carbon - proton coupling constants is quite&amp;nbsp;tedious.&amp;nbsp; One way to simplify matters and obtain specific carbon - proton coupling constants&amp;nbsp;is to apply the selective 2D heteronuclear J-resolved technique first introduced by Bax and Freeman&amp;nbsp;in 1982 (JACS 104, 1099).&amp;nbsp; This method employs a &lt;sup&gt;13&lt;/sup&gt;C spin echo&amp;nbsp;with a selective &lt;sup&gt;1&lt;/sup&gt;H 180° pulse applied&amp;nbsp;simultaneously with the &lt;sup&gt;13&lt;/sup&gt;C nonselective 180° pulse.&amp;nbsp;A version of this sequence is shown in the figure below with a shaped&amp;nbsp;adiabatic &lt;sup&gt;13&lt;/sup&gt;C 180° pulse.&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: left;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://1.bp.blogspot.com/-g9N4DitTEEw/UC6P4tJNCEI/AAAAAAAAA9w/f_3DfqG2AoA/s1600/jres2.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="268" mda="true" src="http://1.bp.blogspot.com/-g9N4DitTEEw/UC6P4tJNCEI/AAAAAAAAA9w/f_3DfqG2AoA/s400/jres2.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: left;"&gt;
In this sequence one obtains a 2D spectrum with&amp;nbsp;&lt;sup&gt;13&lt;/sup&gt;C in the F2 domain and the long range couplings to the selectively inverted proton in the F1 domain.&amp;nbsp; An example is shown in the figure below for toluene where the methyl protons were selectively inverted with a 20 msec Gaussian pulse.&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: left;"&gt;
&lt;br /&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: center;"&gt;
&lt;a href="http://2.bp.blogspot.com/-zfPJht6fBAc/UC6QFqgLIdI/AAAAAAAAA94/t6KKLzan6vg/s1600/jres3.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="300" mda="true" src="http://2.bp.blogspot.com/-zfPJht6fBAc/UC6QFqgLIdI/AAAAAAAAA94/t6KKLzan6vg/s400/jres3.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
&lt;div class="separator" style="clear: both; text-align: left;"&gt;
All of the carbons coupled to the methyl protons are split into quartets in the F1 domain and the long range coupling constants which were very difficult to obtain from the&amp;nbsp;coupled&amp;nbsp;&lt;sup&gt;13&lt;/sup&gt;C spectrum can simply be read directly&amp;nbsp;from the 2D spectrum.&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/b40voG_dVwA" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/b40voG_dVwA/measurement-long-range-c-h-coupling.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-GAK0eeIlyyg/UC6PMzM7LnI/AAAAAAAAA9o/ug_eQneqHOk/s72-c/jres1.jpg" height="72" width="72" /><thr:total>14</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/08/measurement-long-range-c-h-coupling.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-2170008243597752767</guid><pubDate>Mon, 25 Jun 2012 18:33:00 +0000</pubDate><atom:updated>2012-06-25T15:16:21.066-04:00</atom:updated><title>Exact Simulaion of Quadrupolar Lineshapes in Solids</title><description>The NMR spectra for quadrupolar nuclei in solids contain a great deal of structural information.&amp;nbsp; The evaluation of quadrupolar coupling constants, asymmetry parameters, isotropic chemical shifts, chemical shift spans, chemical shift skews&amp;nbsp;and the angles relating the electric field gradient tensor to the chemical shift tensor is typically done by simulating the NMR spectrum with suitable software and fitting the simulated spectrum to the experimental data.&amp;nbsp; Almost always, the spectra of quadrupolar nuclei in solids have been simulated using perturbation theory where the quadrupolar interaction is treated as a perturbation on the much larger Zeeman interaction.&amp;nbsp; With the recent developments&amp;nbsp;in the collection of ultra-wide line NMR spectra, quadrupolar nuclei with larger and larger quadrupolar coupling constants are being studied by NMR and the&amp;nbsp;perturbation approach may not be valid.&amp;nbsp; Errors between&amp;nbsp;simulated and experimental spectra&amp;nbsp;appear when&amp;nbsp;the Larmor frequency is not significantly larger than the quadrupolar coupling constant.&lt;br /&gt;
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&lt;a href="http://4.bp.blogspot.com/-2_GtowPpsNQ/T-itLUAMpdI/AAAAAAAAA80/ELt4sYzrnss/s1600/quest_logo.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="306" rca="true" src="http://4.bp.blogspot.com/-2_GtowPpsNQ/T-itLUAMpdI/AAAAAAAAA80/ELt4sYzrnss/s400/quest_logo.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;
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Recently, a new program called QUEST (&lt;strong&gt;QU&lt;/strong&gt;adrupolar &lt;strong&gt;E&lt;/strong&gt;xact &lt;strong&gt;S&lt;/strong&gt;of&lt;strong&gt;T&lt;/strong&gt;ware) has been written by Frédéric Parras from the &lt;a href="http://mysite.science.uottawa.ca/dbryce/" target="_blank"&gt;research group&lt;/a&gt; of &lt;a href="http://www.science.uottawa.ca/fac/professor_details.html?en/36" target="_blank"&gt;David Bryce&lt;/a&gt; at the &lt;a href="http://www.uottawa.ca/welcome.html" target="_blank"&gt;University of Ottawa&lt;/a&gt;.&amp;nbsp; As the name implies, this program is capable of simulating exactly the spectra of quadrupolar nuclei in solids without resorting to the assumptions of perturbation theory.&amp;nbsp;QUEST is able to quickly calculate accurate lineshapes regardless of the ratio between the Larmor frequency and the quadrupolar coupling constant.&amp;nbsp; It even works in cases where the Larmor frequency is much less than the quadrupolar coupling constant (i.e. NQR).&amp;nbsp;The figure below shows a series of spectra calculated for a spin &lt;em&gt;I=3/2&lt;/em&gt; nucleus as a function of the ratio of the Larmor frequency, ν&lt;sub&gt;&lt;em&gt;L&lt;/em&gt;&lt;/sub&gt;&amp;nbsp;, to the quadrupolar coupling constant, &lt;em&gt;C&lt;sub&gt;Q&lt;/sub&gt;&lt;/em&gt;. The spectra&amp;nbsp;near the top are NMR-like and those near the bottom are NQR-like.&amp;nbsp; QUEST is a fast, graphical, easy-to-use program&amp;nbsp;able to handle multiple sites, export data in Bruker format, import experimental spectra&amp;nbsp;for comparison to the simulations and simulate spectra as a function of the angle of the detection coil with respect to the magnetic field.&amp;nbsp;The package also includes a very helpful well written pdf manual.&amp;nbsp; The program is reported and described fully &lt;a href="http://www.sciencedirect.com/science/article/pii/S0926204012000586" target="_blank"&gt;here&lt;/a&gt;.&amp;nbsp; To take a look at the program in action,&amp;nbsp;watch these &lt;a href="http://www.youtube.com/user/QUESTtutorialvideos" target="_blank"&gt;tutorial videos&lt;/a&gt; prepared by the author.&amp;nbsp; The complete program is available for free &lt;a href="http://mysite.science.uottawa.ca/dbryce/" target="_blank"&gt;download here&lt;/a&gt;.&amp;nbsp; I highly recommend it!&lt;/div&gt;
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&lt;a href="http://4.bp.blogspot.com/-zGalBXq1Y3k/T-iupkuZX4I/AAAAAAAAA88/UDuLQTKcW9E/s1600/quest.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"&gt;&lt;img border="0" height="400" rca="true" src="http://4.bp.blogspot.com/-zGalBXq1Y3k/T-iupkuZX4I/AAAAAAAAA88/UDuLQTKcW9E/s400/quest.jpg" width="302" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/ydVpTUWzl8I" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/ydVpTUWzl8I/exact-simulaion-of-quadrupolar.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-2_GtowPpsNQ/T-itLUAMpdI/AAAAAAAAA80/ELt4sYzrnss/s72-c/quest_logo.jpg" height="72" width="72" /><thr:total>6</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/06/exact-simulaion-of-quadrupolar.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-6336762570957210938</guid><pubDate>Wed, 02 May 2012 20:04:00 +0000</pubDate><atom:updated>2012-05-02T16:12:21.054-04:00</atom:updated><title>60 MHz NMR on the Bench Top</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
The&amp;nbsp;development of bench top NMR spectrometers&amp;nbsp;has certainly been exciting recently!&amp;nbsp; &lt;a href="http://www.nanalysis.com/index.htm#"&gt;Nanalysis&lt;/a&gt; (a Canadian company) has recently introduced a 60 MHz bench top NMR spectrometer.&amp;nbsp; The &lt;a href="http://www.nanalysis.com/index.htm#"&gt;NMReady&lt;sup&gt;TM&lt;/sup&gt;60P&lt;/a&gt; is capable of running both &lt;sup&gt;1&lt;/sup&gt;H and &lt;sup&gt;19&lt;/sup&gt;F NMR spectra.&amp;nbsp; Like the &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/2010/11/new-bench-top-1-h-nmr.html"&gt;PicoSpin&lt;/a&gt; spectrometer, this instrument should have a high impact&amp;nbsp;on the NMR scene.&lt;/div&gt;
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&lt;a href="http://www.nanalysis.com/index.htm#"&gt;&lt;img border="0" height="130" mea="true" src="http://1.bp.blogspot.com/-ERqiDm5qD7Q/T6GSQELTv8I/AAAAAAAAA8o/M-xvkVqw7xw/s400/nanalysis.jpg" width="400" /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/T7B_9ELoWNw" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/T7B_9ELoWNw/60-mhz-nmr-on-bench-top.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-ERqiDm5qD7Q/T6GSQELTv8I/AAAAAAAAA8o/M-xvkVqw7xw/s72-c/nanalysis.jpg" height="72" width="72" /><thr:total>5</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/05/60-mhz-nmr-on-bench-top.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3257990631950577102</guid><pubDate>Fri, 20 Apr 2012 17:26:00 +0000</pubDate><atom:updated>2012-04-20T13:29:12.150-04:00</atom:updated><title>Weak Lock Signals and Distorted NMR Spectra</title><description>&lt;div style="border-bottom: medium none; border-left: medium none; border-right: medium none; border-top: medium none;"&gt;
A good &lt;sup&gt;2&lt;/sup&gt;H lock signal with a high signal-to-noise ratio is a real advantage for maintaining a stable magnetic field for long data acquisitions and also&amp;nbsp;for shimming the magnet using the lock signal.&amp;nbsp; Sometimes, however it is desirable to run NMR&amp;nbsp;spectra&amp;nbsp;for samples with only a only a very small quantity of deuterated solvent and therefore a very weak lock signal.&amp;nbsp; Such may be the case when one is monitoring a&amp;nbsp;chemical reaction&amp;nbsp;by removing aliquots and adding a drop or two of a deuterated solvent to help with magnet shimming&amp;nbsp;using the &lt;sup&gt;2&lt;/sup&gt;H lock signal.&amp;nbsp; Although one may be able to shim a magnet&amp;nbsp;using a very weak lock signal (with difficulty), running the spectrum locked may not be a good idea.&amp;nbsp; Running a spectrum while locked on a very weak lock signal can lead to distortions in the spectrum.&amp;nbsp; It is often better to use the weak lock signal to shim the magnet as best you can and then run the spectrum unlocked.&amp;nbsp; This is demonstrated in the figure below.&lt;img alt="" border="0" height="300" qda="true" src="http://3.bp.blogspot.com/-bnhE9GlO_IQ/T5Gap1OEVBI/AAAAAAAAA8g/AHX8ysC1yaI/s400/weak_lock.jpg" title="" width="400" /&gt;&amp;nbsp; &lt;br /&gt;
The figure shows two single scan&amp;nbsp;&lt;sup&gt;1&lt;/sup&gt;H NMR spectra of a sample of acetone (one drop)&amp;nbsp;in CCl&lt;sub&gt;4&lt;/sub&gt; with a drop of CDCl&lt;sub&gt;3&lt;/sub&gt;.&amp;nbsp; The spectrum on the left was acquired using the &lt;sup&gt;2&lt;/sup&gt;H lock and the one on the right was acquired unlocked.&amp;nbsp; One can clearly see the distortion in the &lt;sup&gt;1&lt;/sup&gt;H spectrum caused by locking on a very weak &lt;sup&gt;2&lt;/sup&gt;H&amp;nbsp;signal. &lt;/div&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/jsHZ3uIK3DY" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/jsHZ3uIK3DY/weak-lock-signals-and-distorted-nmr.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-bnhE9GlO_IQ/T5Gap1OEVBI/AAAAAAAAA8g/AHX8ysC1yaI/s72-c/weak_lock.jpg" height="72" width="72" /><thr:total>4</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/04/weak-lock-signals-and-distorted-nmr.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-5799205892874314549</guid><pubDate>Fri, 30 Mar 2012 17:27:00 +0000</pubDate><atom:updated>2012-04-02T08:43:39.730-04:00</atom:updated><title>The Extremely Complicated 1H NMR Spectrum of Ethane</title><description>It is often incorrectly assumed that simple compounds yield simple NMR spectra. The &lt;sup&gt;1&lt;/sup&gt;H NMR spectrum of ethane is such an example. The complexity arises when one takes into account the inequivalence between methyl groups in the mono &lt;sup&gt;13&lt;/sup&gt;C isotopomer which accounts for 1% of the naturally occurring ethane. In this isotopomer, one methyl group experiences a one-bond &lt;sup&gt;1&lt;/sup&gt;H - &lt;sup&gt;13&lt;/sup&gt;C coupling (&lt;sup&gt;1&lt;/sup&gt;J&lt;sub&gt;H-C&lt;/sub&gt;) while the other methyl group experiences a two-bond &lt;sup&gt;1&lt;/sup&gt;H - &lt;sup&gt;13&lt;/sup&gt;C coupling (&lt;sup&gt;2&lt;/sup&gt;J&lt;sub&gt;H-C&lt;/sub&gt;). Also, the effects of the three-bond &lt;sup&gt;1&lt;/sup&gt;H - &lt;sup&gt;1&lt;/sup&gt;H coupling (&lt;sup&gt;3&lt;/sup&gt;J&lt;sub&gt;H-H&lt;/sub&gt;) are exhibited in the spectrum due to the inequivalence. These couplings have a dramatic effect on the spectrum. Furthermore, there is a very small &lt;a href="http://u-of-o-nmr-facility.blogspot.ca/search?q=isotope+shift"&gt;isotope effect &lt;/a&gt;on the &lt;sup&gt;1&lt;/sup&gt;H chemical shifts of each methyl group due to the presence of &lt;sup&gt;13&lt;/sup&gt;C vs &lt;sup&gt;12&lt;/sup&gt;C. This effect however, is very small (~0.002 ppm) and has very little effect on the spectrum. The left panel of the figure below shows a simulation of the &lt;sup&gt;1&lt;/sup&gt;H NMR spectrum of the &lt;sup&gt;12&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt;-&lt;sup&gt;12&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt; which accounts for 98% of naturally occurring ethane. As expected, the spectrum is a singlet as both methyl groups are equivalent to one another. The middle panel of the figure shows a simulation of the &lt;sup&gt;1&lt;/sup&gt;H NMR spectrum of the &lt;sup&gt;13&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt;-&lt;sup&gt;12&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt; isotopomer which accounts for 2% of naturally occurring ethane. In this case the spectrum is extremely complex due to the &lt;sup&gt;1&lt;/sup&gt;J&lt;sub&gt;H-C &lt;/sub&gt;, &lt;sup&gt;2&lt;/sup&gt;J&lt;sub&gt;H-C&lt;/sub&gt; and &lt;sup&gt;3&lt;/sup&gt;J&lt;sub&gt;H-H&lt;/sub&gt; coupling. The panel on the right shows a simulation of a scaled up representation of what one would expect for naturally occurring ethane.&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 300px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5726782985646546706" border="0" alt="" src="http://2.bp.blogspot.com/-bg2rPcXQzlQ/T3meyJ02nxI/AAAAAAAAA8Y/ZSA5LRbbwHQ/s400/ethane_sim.jpg" /&gt;&lt;br /&gt;The parameters for the simulations are as follows: Δδ&lt;sub&gt;H&lt;/sub&gt; between -&lt;sup&gt;12&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt; and -&lt;sup&gt;13&lt;/sup&gt;CH&lt;sub&gt;3&lt;/sub&gt;= 0.002 ppm, &lt;sup&gt;1&lt;/sup&gt;J&lt;sub&gt;H-C &lt;/sub&gt;= 125 Hz, &lt;sup&gt;2&lt;/sup&gt;J&lt;sub&gt;H-C &lt;/sub&gt;= -4.67 Hz, &lt;sup&gt;3&lt;/sup&gt;J&lt;sub&gt;H-H &lt;/sub&gt;= 8 Hz and LB = 0.5 Hz.&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/uIt6TAJcteg" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/uIt6TAJcteg/extremely-complicated-1-h-nmr-spectrum.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://2.bp.blogspot.com/-bg2rPcXQzlQ/T3meyJ02nxI/AAAAAAAAA8Y/ZSA5LRbbwHQ/s72-c/ethane_sim.jpg" height="72" width="72" /><thr:total>4</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/03/extremely-complicated-1-h-nmr-spectrum.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-4330521660836923699</guid><pubDate>Thu, 29 Mar 2012 13:49:00 +0000</pubDate><atom:updated>2012-03-29T10:06:16.488-04:00</atom:updated><title>The Major Constituents of Natural Gas</title><description>The major constituent of natural gas is methane however, other gaseous hydrocarbons are also present. One way to identify other components is to dissolve some natural gas in a solvent and examine the &lt;sup&gt;1&lt;/sup&gt;H NMR spectrum. The spectrum in the figure below was acquired on a sample prepared by bubbling natural gas through benzene&lt;em&gt;-d&lt;sub&gt;6&lt;/sub&gt;&lt;/em&gt; for several minutes. The spectrum clearly shows the presence of methane, ethane, propane and water.&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 347px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5725319007148266818" border="0" alt="" src="http://1.bp.blogspot.com/-q-r6TSTHCdk/T3RrTY7dVUI/AAAAAAAAA8A/lYTb4acZIQU/s400/natural_gas.jpg" /&gt; The spectrum also indicated other impurities at much lower levels (not shown in the figure).&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/Wt37CXkfuNk" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/Wt37CXkfuNk/major-constituents-of-natural-gas.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-q-r6TSTHCdk/T3RrTY7dVUI/AAAAAAAAA8A/lYTb4acZIQU/s72-c/natural_gas.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/03/major-constituents-of-natural-gas.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-8191009218195381040</guid><pubDate>Fri, 16 Mar 2012 19:17:00 +0000</pubDate><atom:updated>2012-03-16T15:55:03.721-04:00</atom:updated><title>Protic Samples in Aprotic Solvents</title><description>The appearance of the &lt;sup&gt;1&lt;/sup&gt;H NMR signals of protic samples in aprotic solvents depends critically on the concentration of the sample. The -OH, -NH&lt;sub&gt;2&lt;/sub&gt; or -COOH signals can have chemical shift values and line widths over a wide range due to varying extents of hydrogen bonding and chemical exchange. The concentration can also determine whether or not one is able to observe J coupling between and -OH proton and other protons in the sample. An example of this is illustrated below. The figure shows the spectrum of methanol in deuterated acetone. The spectrum on the top is that of concentrated methanol and it consists of two singlets. In this case the methanol molecules are hydrogen bonded to one another and the -OH protons are undergoing fast exhange with one another. The spectrum on the bottom is that of very dilute methanol. It is a &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2008/07/second-order-1-nmr-spectra-of-isopropyl.html"&gt;second order &lt;/a&gt;spectrum with two signals approximating a doublet and a quartet due the J coupling between the methyl protons and -OH proton, respectively. Note that the chemical shift of the -OH proton is much lower for the dilute methanol compared to the concentrated methanol. In this case the methanol molecules are not hydrogen bonded to one another and there is no (or very slow) exchange among the -OH protons between molecules allowing for the observation of the J coupling.&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 317px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5720585046777090722" border="0" alt="" src="http://3.bp.blogspot.com/-tga1NR9HuTM/T2OZyoSPUqI/AAAAAAAAA70/MEdQHkbM9ww/s400/protic_samples.jpg" /&gt;&lt;div class="feedflare"&gt;
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&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/obgDS9tbEU4" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/obgDS9tbEU4/protic-samples-in-aprotic-solvents.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-tga1NR9HuTM/T2OZyoSPUqI/AAAAAAAAA70/MEdQHkbM9ww/s72-c/protic_samples.jpg" height="72" width="72" /><thr:total>5</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/03/protic-samples-in-aprotic-solvents.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-5074409642513700156</guid><pubDate>Thu, 15 Mar 2012 18:31:00 +0000</pubDate><atom:updated>2012-03-15T15:11:12.105-04:00</atom:updated><title>Double Presaturation</title><description>&lt;a href="http://u-of-o-nmr-facility.blogspot.com/2010/02/presaturation.html"&gt;Presaturation &lt;/a&gt;is a common method of reducing the water signal in the &lt;sup&gt;1&lt;/sup&gt;H NMR spectra of aqueous samples. Sometimes, a sample may contain more than one undesirable resonance which a user may want to presaturate. In such a case, one must presaturate at multiple frequencies simultaneously. On a two-channel Bruker spectrometer, two signals can be presaturated. This is accomplished by using both Signal Generation Units (SGUs). One of the undesirable signals is put on-resonance and is presaturated with the signal from SGU1 after which the hard pulse is given (also through SGU1). The second undesirable resonance is presaturated using SGU2. The configuration is as follows:&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 300px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5720200700494368338" border="0" alt="" src="http://3.bp.blogspot.com/-6dnBCpoVGV4/T2I8OuzoTlI/AAAAAAAAA7o/-eKKyJG6ZbE/s400/double_presaturation_1.jpg" /&gt;If one has a three-channel system, one can presaturate three resonances using three SGUs. The figure below shows an example of double presaturation on a two-channel system. &lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 300px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5720200118535475762" border="0" alt="" src="http://4.bp.blogspot.com/-z7u18iTz9lc/T2I7s210UjI/AAAAAAAAA7c/6pyAR8UJdAI/s400/double_presaturation_2.jpg" /&gt;The sample consisted of phenylalanine dissolved in D&lt;sub&gt;2&lt;/sub&gt;O contaminated with methanol. The one-pulse spectrum in the bottom left panel shows the intense HDO and methanol signals. The double presaturation spectrum in the top left panel is on the same vertical scale as the one on the bottom left. One can see that both solvent signals have been almost completely eliminated. The spectra on the right-hand side are the same data as on the left except the vertical scale has been increased by a factor of 100. You can try this on your Bruker spectrometer using the pulse program "lc1prf2".&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=V1POFh7N8M4:gu_ONo1-xPc:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/V1POFh7N8M4" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/V1POFh7N8M4/double-presaturation.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-6dnBCpoVGV4/T2I8OuzoTlI/AAAAAAAAA7o/-eKKyJG6ZbE/s72-c/double_presaturation_1.jpg" height="72" width="72" /><thr:total>10</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/03/double-presaturation.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3934075473271453324</guid><pubDate>Thu, 19 Jan 2012 16:42:00 +0000</pubDate><atom:updated>2012-01-20T09:44:49.187-05:00</atom:updated><title>Sorting Out NOE's for Exchanging Rotamers</title><description>&lt;a href="http://u-of-o-nmr-facility.blogspot.com/2008/01/noesy-small-molecules-vs-large.html"&gt;2D NOESY &lt;/a&gt;spectra contain cross peaks from both NOE interactions and peaks due to rotamers in slow exchange with one another on the &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2008/08/nmr-time-scale.html"&gt;NMR tine scale&lt;/a&gt;. For small molecules, the cross peaks resulting from slowly exchanging rotamers are of the same sign as the diagonal peaks. The NOE cross peaks, on the other hand, are of opposite sign compared to the diagonal peaks. When both types of correlations are present there may be more NOE correlations than expected. What follows is an example of this. The figure below shows a color coded chemical structure of a ruthenium complex with a color coded partial &lt;sup&gt;1&lt;/sup&gt;H NMR spectrum.&lt;img id="BLOGGER_PHOTO_ID_5699388424917185586" style="DISPLAY: block; MARGIN: 0px auto 10px; WIDTH: 400px; CURSOR: hand; HEIGHT: 300px; TEXT-ALIGN: center" alt="" src="http://3.bp.blogspot.com/-JwukDwi8jVg/TxhLk2gpdDI/AAAAAAAAA6s/ggcOJjYiTe4/s400/justin_noesy_1.jpg" border="0" /&gt;It is obvious from the NMR spectrum that all of the signals from the color coded protons are doubled in the spectrum. One possible explanation for this is that there is a slow rotation about the ruthenium carbon bond indicated with the red curly arrow allowing for two possible nonequivalent rotamers. This is confirmed with the 2D &lt;sup&gt;1&lt;/sup&gt;H NOESY spectrum shown in the figure below with a 0.9 second mixing time. The spectrum clearly shows exchange peaks between corresponding pairs of &lt;sup&gt;1&lt;/sup&gt;H signals from each rotamer.&lt;img id="BLOGGER_PHOTO_ID_5699388756336354866" style="DISPLAY: block; MARGIN: 0px auto 10px; WIDTH: 400px; CURSOR: hand; HEIGHT: 345px; TEXT-ALIGN: center" alt="" src="http://3.bp.blogspot.com/-oJQ6eJEIm_c/TxhL4JJIpjI/AAAAAAAAA64/WEqd6d02qy8/s400/justin_noesy_2.jpg" border="0" /&gt;The interesting thing to note from the NOESY spectrum is that each aromatic proton (pink) from a single rotamer shows NOE correlations to the methyl groups (blue and yellow) of both rotamers - not just those from a single rotamer. With this data, it is not possible to assign the subspectrum of a single rotamer. Presumably, the assignment could be made by collecting a 2D NOESY spectrum at low temperature where the rotation was completely frozen out or by collecting a 2D NOESY spectrum with a very short mixing time where the rotation would be limited. The problem with the former approach is that the solvent may freeze at a temperature too high to stop the bond rotation. The problem with the latter approach is that the NOE's would be much reduced due to the short mixing time and collecting a 2D data set with sufficient signal to noise ratio would take a great deal of time. Another approach is to collect &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2009/05/selective-1d-gradient-noesy.html"&gt;selective 1D gradient NOESY spectra &lt;/a&gt;with selective excitation of the aromatic proton from each rotamer individually. These data are shown in the figure below for two different mixing times.&lt;img id="BLOGGER_PHOTO_ID_5699389094445046354" style="DISPLAY: block; MARGIN: 0px auto 10px; WIDTH: 400px; CURSOR: hand; HEIGHT: 259px; TEXT-ALIGN: center" alt="" src="http://3.bp.blogspot.com/-EDe38yF37jU/TxhML0sh2lI/AAAAAAAAA7E/WG2ZPknywPA/s400/justin_noesy_3.jpg" border="0" /&gt;Each spectrum is displayed in two parts. The left-hand panel is the aromatic region with the selectively excited resonance colored red and the right-hand panel is the aliphatic region showing the NOE correlations to the methyl groups. From the spectra collected with a 2 second mixing time, one can see that the selective excitation is no longer selective due to bond rotation during the long mixing time. One can see inverted peaks for the aromatic protons of both rotamers despite the fact that the &lt;sup&gt;1&lt;/sup&gt;H signal of only one rotamer was selectively excited. Furthermore, NOEs to the methyl signals from both rotamers are present. The spectra collected with only a 0.2 second mixing time, on the other hand, show very selective excitation. The time scale of the bond rotation is obviously longer than the 0.2 second mixing time. The spectra show only the NOEs between the selectively excited aromatic proton and the methyl groups from a single rotamer. The NOEs build up fast enough to be observed during the 0.2 second mixing time before rotation occurs. These data allow for the assignment of signals from each of the rotamers.&lt;br /&gt;&lt;br /&gt;Thank you to Justin Lummiss of &lt;a href="http://mysite.science.uottawa.ca/dfogg/default.htm"&gt;Dr. Fogg's &lt;/a&gt;research group for aharing this interesting system.&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=fHDevYVV0cg:hp-GQwbA9oA:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/fHDevYVV0cg" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/fHDevYVV0cg/sorting-out-noes-for-exchanging.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-JwukDwi8jVg/TxhLk2gpdDI/AAAAAAAAA6s/ggcOJjYiTe4/s72-c/justin_noesy_1.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2012/01/sorting-out-noes-for-exchanging.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-6409608386756141650</guid><pubDate>Thu, 22 Dec 2011 15:46:00 +0000</pubDate><atom:updated>2011-12-22T11:55:30.171-05:00</atom:updated><title>13C NMR of a Delicious Christmas Treat</title><description>As my Santa Claus-like belly may indicate, I love holiday treats. The solid-state &lt;sup&gt;13&lt;/sup&gt;C NMR spectra below were collected from a special sample of a holiday treat prepared by my wife, Patty from her Great Grandma Jennings lab book. The sample was prepared from only four ingredients as follows:&lt;br /&gt;&lt;br /&gt;To 227 g of softened butter, 65 g of fructose was added while stirring with a spatula. Slowly, 199 g of flour and 1.26 g of sodium chloride were stirred into the mixture until it became difficult to mix with a spatula. The mixture was kneaded gently until cracks in the surface began to appear after which it was rolled to a thickness of 38 mm and cut into round samples of approximately 51 mm in size. The samples were heated in an oven at 436 K - 450 K for approximately 600 seconds until gold in color.&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;&lt;div&gt;&lt;/div&gt;&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 373px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5688983781992801650" border="0" alt="" src="http://4.bp.blogspot.com/-Lp_eeBvoTtc/TvNUm7KjpXI/AAAAAAAAA6g/SoWa1lfBRMA/s400/shortbread.jpg" /&gt;The bottom trace is a &lt;sup&gt;13&lt;/sup&gt;C &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2007/12/cross-polarization.html"&gt;CPMAS&lt;/a&gt; spectrum and the top trace is a &lt;sup&gt;13&lt;/sup&gt;C MAS spectrum. Both spectra were acquired with high power &lt;sup&gt;1&lt;/sup&gt;H decoupling. This pair of spectra serves to illustrate the different types of information available from each of these techniques. The sample is a mixture of rigid and mobile components. The &lt;sup&gt;13&lt;/sup&gt;C CPMAS technique detects mainly the more rigid components as it relies on the dipolar coupling between protons and &lt;sup&gt;13&lt;/sup&gt;C for the cross polarization. The dipolar coupling is averaged to nearly zero for the mobile constituents and therefore they do not appear in the spectrum. The &lt;sup&gt;13&lt;/sup&gt;C CPMAS spectrum therefore, shows primarily all of the rigid constituents (mainly flour and sugar). The &lt;sup&gt;13&lt;/sup&gt;C MAS spectrum with high power &lt;sup&gt;1&lt;/sup&gt;H decoupling shows both rigid and mobile constituents. The resonances from the mobile constituents (mainly butter) have sharp lines while the broader lines from the rigid constituents show up at very low intensity as the sensitivity is not enhanced by cross polarization.&lt;br /&gt;&lt;br /&gt;Now, you too have enjoyed Patty's delicious shortbread.&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=xH19E-vRKSk:fsLs1YVmZ4o:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/xH19E-vRKSk" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/xH19E-vRKSk/13-c-nmr-of-delicious-christmas-treat.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://4.bp.blogspot.com/-Lp_eeBvoTtc/TvNUm7KjpXI/AAAAAAAAA6g/SoWa1lfBRMA/s72-c/shortbread.jpg" height="72" width="72" /><thr:total>3</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2011/12/13-c-nmr-of-delicious-christmas-treat.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3537109039761513262</guid><pubDate>Wed, 07 Dec 2011 19:32:00 +0000</pubDate><atom:updated>2011-12-07T14:59:44.969-05:00</atom:updated><title>Enlightening NMR Videos on YouTube</title><description>&lt;a href="http://www.journals.elsevier.com/journal-of-magnetic-resonance/"&gt;The Journal of Magnetic Resonance &lt;/a&gt;(JMR) has been publishing important contributions from NMR spectroscopists since 1969. Some of these contributions have become "classic papers" and have been sited thousands of times. A &lt;a href="http://www.youtube.com/playlist?list=PL1D790E241B661706"&gt;play list of videos &lt;/a&gt;has been assembled on YouTube highlighting some of the most significant contributions in NMR spectroscopy over the last few decades. The research is described anecdotally (and in some cases very humbly) by the original authors in the videos. I think you will enjoy putting faces to the names of the authors of these highly cited papers.&lt;a href="http://www.youtube.com/playlist?list=PL1D790E241B661706"&gt;&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 193px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5683477936007804530" border="0" alt="" src="http://3.bp.blogspot.com/-7FU52GO0EvY/Tt_FEgiD9nI/AAAAAAAAA6U/tgIDsQwn3_4/s400/youtube_jmr.jpg" /&gt;&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;&lt;div&gt;&lt;/div&gt;&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=NK7e-bl5_x4:bBJAbDVqc2Q:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/NK7e-bl5_x4" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/NK7e-bl5_x4/enlightening-nmr-videos-on-youtube.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://3.bp.blogspot.com/-7FU52GO0EvY/Tt_FEgiD9nI/AAAAAAAAA6U/tgIDsQwn3_4/s72-c/youtube_jmr.jpg" height="72" width="72" /><thr:total>0</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2011/12/enlightening-nmr-videos-on-youtube.html</feedburner:origLink></item><item><guid isPermaLink="false">tag:blogger.com,1999:blog-3300702123878659843.post-3046827444648845837</guid><pubDate>Fri, 28 Oct 2011 14:40:00 +0000</pubDate><atom:updated>2011-10-28T13:53:43.965-04:00</atom:updated><title>The Effect of Viscosity on 1H NOESY Spectra</title><description>For small molecules, &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2008/01/noesy-small-molecules-vs-large.html"&gt;&lt;sup&gt;1&lt;/sup&gt;H 2D NOESY spectra &lt;/a&gt;exhibit positive NOE's between protons close to one another in space and the off-diagonal correlations are opposite in phase to those of the diagonals. As molecules become larger and larger the motional correlation times become longer and longer. As the correlation times become longer and longer, the NOE's become less positive, cross zero and then become negative. For large molecules, like proteins, the NOE's are negative and the off-diagonal correlations between close protons are of the same phase as the diagonal peaks. When the correlation times are extremely long, for example in rigid macromolecules or solids, the dipolar coupling among all of the protons is inefficiently averaged by molecular motions and spin diffusion becomes efficient. Spin diffusion allows all of the protons in a dipolar coupled network to exhibit correlations with one another. The sign of the correlations is similar to that observed for &lt;a href="http://u-of-o-nmr-facility.blogspot.com/2008/07/2d-exsy.html"&gt;chemical exchange &lt;/a&gt;or negative NOE's. This phenomenon is demonstrated in the figure below. In the figure, positive contours are represented in black and negative contours are represented in red. The NOESY spectrum on the left is that of a solution of menthol in CDCl&lt;sub&gt;3&lt;/sub&gt;. The off-diagonal correlations between proximate protons is opposite in phase compared to the diagonal responses, typical of small molecules with short correlation times. The NOESY spectrum on the right is that of the same solution of menthol dissolved in a very viscous fluorinated oil. The extreme viscosity of the sample is sufficient to make the correlation time for the molecules very long such that the menthol behaves like a very large macromolecule where spin diffusion is efficient. As a result, off-diagonal responses are of the same phase as those of the diagonal and are observed between &lt;strong&gt;all&lt;/strong&gt; protons in the molecule.&lt;img style="TEXT-ALIGN: center; MARGIN: 0px auto 10px; WIDTH: 400px; DISPLAY: block; HEIGHT: 290px; CURSOR: hand" id="BLOGGER_PHOTO_ID_5668599159872888258" border="0" alt="" src="http://1.bp.blogspot.com/-cnR_O9cPpj0/Tqro5wJNHcI/AAAAAAAAA6I/vT6cTnlfnqw/s400/noesy_oil.jpg" /&gt;This technique has been cleverly applied* to mixtures of molecules immersed in viscous oils where intra-molecular correlations are observed whereas inter-molecular correlations are not observed. The data allow for the observation of the constituent components of complex mixtures.&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;&lt;div&gt;* Andre J. Simpson, Gwen Woods, and Omid Mehrzad, &lt;em&gt;Anal. Chem&lt;/em&gt;, &lt;strong&gt;80&lt;/strong&gt;, 186-194 (2008).&lt;/div&gt;&lt;div class="feedflare"&gt;
&lt;a href="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?a=v2GviDqdOCI:clqdZvVOOQE:yIl2AUoC8zA"&gt;&lt;img src="http://feeds.feedburner.com/~ff/UniversityOfOttawaNmrFacilityBlog?d=yIl2AUoC8zA" border="0"&gt;&lt;/img&gt;&lt;/a&gt;
&lt;/div&gt;&lt;img src="http://feeds.feedburner.com/~r/UniversityOfOttawaNmrFacilityBlog/~4/v2GviDqdOCI" height="1" width="1"/&gt;</description><link>http://feedproxy.google.com/~r/UniversityOfOttawaNmrFacilityBlog/~3/v2GviDqdOCI/effect-of-viscosity-on-1-h-noesy.html</link><author>noreply@blogger.com (Glenn Facey)</author><media:thumbnail xmlns:media="http://search.yahoo.com/mrss/" url="http://1.bp.blogspot.com/-cnR_O9cPpj0/Tqro5wJNHcI/AAAAAAAAA6I/vT6cTnlfnqw/s72-c/noesy_oil.jpg" height="72" width="72" /><thr:total>4</thr:total><feedburner:origLink>http://u-of-o-nmr-facility.blogspot.com/2011/10/effect-of-viscosity-on-1-h-noesy.html</feedburner:origLink></item></channel></rss>
