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<head> <meta name=Title content="Baseline Evaluation of XAFS Bending Magnet Beamlines"> <meta name=Keywords content=""> <meta http-equiv=Content-Type content="text/html; charset=macintosh"> <meta name=ProgId content=Word.Document> <meta name=Generator content="Microsoft Word 11"> <meta name=Originator content="Microsoft Word 11"> <link rel=File-List href="20BMBaseline_files/filelist.xml"> <link rel=Edit-Time-Data href="20BMBaseline_files/editdata.mso"> <!--[if !mso]> <style> v\:* {behavior:url(#default#VML);} o\:* {behavior:url(#default#VML);} w\:* {behavior:url(#default#VML);} .shape {behavior:url(#default#VML);} </style> <![endif]--> <title>Baseline Evaluation of XAFS Bending Magnet Beamlines</title> <!--[if gte mso 9]><xml>

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<p class=MsoNormal style='text-align:justify;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Baseline Evaluation of XAFS Bending Magnet Beamlines<o:p></o:p></span></p>

<p class=MsoNormal style='text-align:justify;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Experiments performed under “<i>standard optimized operating conditions</i></span><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>,” as recorded.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Arial;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Rhodium coated harmonic rejection mirror, angle varies. See notes for specific test.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>The SRS-570 current amplifier gain settings are recorded in the data file headers.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>A 10% DC offset on the SRS-570 was automatically corrected by the data acquisition software.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>The monochromator was detuned by 10% on the preslit detector. <o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Feedback stabilization was not used, although it is available. <o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>The beam was unfocused, although vertical focusing is possible with the 20-BM HR Mirror. <o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Dry N<sub>2</sub>

flowing in I0[15 cm] and IT[30 cm] ionization chambers.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Chambers operating at 600 VDC, except where noted.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>7 GeV electron synchrotron operating in top-up mode, 100 mA (nominal).<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-align:justify;text-indent: -.25in;line-height:150%;mso-list:l0 level1 lfo4;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>I0 entrance slits 1.1 mm vertical x 10 mm horizontal.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><i>N.B. Sector 21 is under construction, so this is probably a worst-case-scenario for noise (audible noise—ugh!!).<o:p></o:p></i></span></p>

<span style='font-size:10.0pt;font-family:"Times New Roman";color:black; mso-ansi-language:EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Experiment log<o:p></o:p></span></p>

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<p class=MsoBodyText style='line-height:150%'><span style='color:black'>XANES scans of metal foil reference standards collected over a large energy range without recalibrating the monochromator. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l2 level1 lfo5;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Metal foils from EXAFS Company (Joe Wong). Set provided by M. Newville.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l2 level1 lfo5;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>     

</span></span><![endif]><span style='color:black'>For the low energy range (V, Cr, Cu and Zn ), harmonic rejection mirror set to 5 mrad.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l2 level1 lfo5;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Cutoff ca. 13,400 eV.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l2 level1 lfo5;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>All XANES collected at 0.2 sec/point, unless otherwise noted.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Changed beamline settings to work at the high energy range. Changeover took about 1/2 hour, not including detector gas equilibration time.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l7 level1 lfo3;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>For the high energy range (Mo, Ag), harmonic rejection mirror set to 2.3 mrad.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l7 level1 lfo3;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Cutoff ca. 29,130 eV.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l7 level1 lfo3;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>I0 entrance slits reduced to 0.8 vertical x 10 mm horizontal. <o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l7 level1 lfo3;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Switch to Ar in I0[15 cm] and IT[30 cm] at 600 VDC for Mo and Ag XANES.<o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l7 level1 lfo3;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Detector gases allowed to equilibrate while we all go for lunch, coffee, etc. around 12:45.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>We see a double peak in the 1<sup>st</sup> derivative of agfoil.0001, and assume it is noise. <o:p></o:p></span></p>

<p class=MsoNormal style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l4 level1 lfo6;tab-stops:list .25in'><![if !supportLists]><span style='font-size:10.0pt;font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='font-size:10.0pt;font-family:Chalkboard;color:black'>Increase counting time to 0.5 sec/point.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>†Rev. Sci. Instrum., <b>67</b></span><span style='font-size:10.0pt;font-family:Chalkboard;color:black'> (1996) 686.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>‡Using first peak in first derivative of XANES scan taken at the beamline with LabView DAC.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>§May need to apply a smoothing algorithm to the Ag XANES to get a decent derivative.<o:p></o:p></span></p>

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<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: V K data (Athena screen shots)<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shapetype

</v:shapetype><v:shape id="_x0000_i1033" type="#_x0000_t75" style='width:225pt;

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image002.png" v:shapes="_x0000_i1033"><![endif]><span style="mso-spacerun: yes">  </span><!--[if gte vml 1]><v:shape id="_x0000_i1034"

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image004.png" v:shapes="_x0000_i1034"><![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Cr K data<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image006.png" v:shapes="_x0000_i1035"><![endif]><span style="mso-spacerun: yes">  </span><!--[if gte vml 1]><v:shape id="_x0000_i1036"

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image008.png" v:shapes="_x0000_i1036"><![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Cu K data<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image010.png" v:shapes="_x0000_i1037"><![endif]><span style="mso-spacerun: yes">  </span><!--[if gte vml 1]><v:shape id="_x0000_i1038"

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image012.png" v:shapes="_x0000_i1038"><![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Zn K data<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image014.png" v:shapes="_x0000_i1046"><![endif]><span style="mso-spacerun: yes">  </span><!--[if gte vml 1]><v:shape id="_x0000_i1047"

</v:shape><![endif]--><![if !vml]><img width=225 height=180 src="20BMBaseline_files/image016.png" v:shapes="_x0000_i1047"><![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Mo K data<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='color:black'><!--[if gte vml 1]><v:shape id="_x0000_i1048" type="#_x0000_t75"

</v:shape><![endif]--><![if !vml]><img width=187 height=181 src="20BMBaseline_files/image019.png" v:shapes="_x0000_i1048"><![endif]></span><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><span style="mso-spacerun: yes">  </span>From Steve Heald<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Ag K data<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=225 height=181 src="20BMBaseline_files/image021.png" v:shapes="_x0000_i1049"><![endif]><span style="mso-spacerun: yes">  </span><!--[if gte vml 1]><v:shape id="_x0000_i1050"

</v:shape><![endif]--><![if !vml]><img width=225 height=181 src="20BMBaseline_files/image023.png" v:shapes="_x0000_i1050"><![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY CALIBRATION: Results<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>†Rev. Sci. Instrum., <b>67</b></span><span style='font-size:10.0pt;font-family:Chalkboard;color:black'> (1996) 686.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>‡Using first peak in first derivative of XANES scan, after application of Athena smoothing algorithm, with the exception of the Mo XANES, which was processed using a spline smoothing algorithm.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>§High energy edges measured with Ar in I0 and IT; detectors gases equilibrated ca. 1 hour, over lunch break.<o:p></o:p></span></p>

<p class=MsoNormal align=center style='text-align:center;line-height:150%'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=344 height=264 src="20BMBaseline_files/image026.png" v:shapes="_x0000_i1051"><![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ENERGY RESOLUTION: Experiment log<o:p></o:p></span></p>

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<p class=MsoBodyText style='line-height:150%'><span style='color:black'>Measure the full width at half maximum of the V<sub>2</sub>O<sub>5</sub> pre-edge feature. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l4 level1 lfo6;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>The sample is powder-on-tape prepared by Matt Newville. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l4 level1 lfo6;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>     

</span></span><![endif]><span style='color:black'>Harmonic Rejection Mirror set to 6 mRad.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l4 level1 lfo6;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>cutoff of ca. 11,179 eV.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l4 level1 lfo6;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Scan details: pre-edge –100 to –20 eV, Post-edge 30 eV to 8k (240 eV) for accurate normalization.<o:p></o:p></span></p>

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<p class=MsoNormal align=center style='text-align:center'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal align=center style='text-align:center'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=227 height=182 src="20BMBaseline_files/image028.png" v:shapes="_x0000_i1052"><![endif]><span style="mso-spacerun: yes">   </span><!--[if gte vml 1]><v:shape id="_x0000_i1053"

</v:shape><![endif]--><![if !vml]><img width=227 height=182 src="20BMBaseline_files/image030.png" v:shapes="_x0000_i1053"><![endif]><o:p></o:p></span></p>

<p class=MsoNormal align=center style='text-align:center'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><!--[if gte vml 1]><v:shape

</v:shape><![endif]--><![if !vml]><img width=284 height=217 src="20BMBaseline_files/image032.jpg" v:shapes="_x0000_i1054"><![endif]>From Matt Newville<o:p></o:p></span></p>

<p class=MsoNormal align=center style='text-align:center'><span style='font-size:10.0pt;font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal><span style='font-size:10.0pt;font-family:Chalkboard; color:black'>HARMONIC CONTENT: Experiment log<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Scan the energy around 6.66 keV through a Mo foil to look for emergent Mo XANES from the third harmonic.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Nominal edge position for Mo is 20,000 eV. Run a XANES scan with E0 = 6,6667. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Harmonic rejection mirror set to 8.5 mRad.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>nominal cutoff ca. 7880 eV.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Limiting factor in HR cutoff is tilting the BM table. N<sub>2</sub> in both chambers. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>I0 is 15 cm, IT is 30 cm gas ionization at 600 VDC.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l1 level1 lfo7;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>25 µm thick Mo foil from the PNC set of foil standards.<o:p></o:p></span></p>

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<p class=MsoBodyText style='line-height:150%'><span style='color:black'>†Crude estimate at beamline is 2-3 x 10^4 harmonic photons/sec.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>‡Crude estimate at beamline is 10^3 harmonic photons/sec.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>BASE NOISE LEVEL: Experiment Log<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Record at 10 keV for 3 minutes. Record with beam off for 3 minutes.<span style="mso-spacerun: yes">  </span>Record data with knife edge 1/2 way through beam, Horizontal and Vertical, for 3 minutes.<o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l3 level1 lfo8;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Harmonic rejection mirror set to 5 mRad. on the HR mirror. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.25in;text-indent:-.25in;line-height: 150%;mso-list:l3 level1 lfo8;tab-stops:list .25in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Return to standard optimized settings: <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.75in;text-indent:-.25in;line-height: 150%;mso-list:l3 level2 lfo8;tab-stops:list .75in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Monochromator detuned by 10% on pre-slit detector. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.75in;text-indent:-.25in;line-height: 150%;mso-list:l3 level2 lfo8;tab-stops:list .75in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>      </span></span><![endif]><span style='color:black'>Re-centered I0 slits. <o:p></o:p></span></p>

<p class=MsoBodyText style='margin-left:.75in;text-indent:-.25in;line-height: 150%;mso-list:l3 level2 lfo8;tab-stops:list .75in'><![if !supportLists]><span style='font-family:"Courier New";color:black'>o<span style='font:7.0pt "Times New Roman"'>     

</span></span><![endif]><span style='color:black'>Slit size H x R = 6 mm x 1.1 mm (est.) <o:p></o:p></span></p>

<p class=MsoBodyText style='line-height:150%'><span style='color:black'>Dummy scan for 3 minutes at 1 sec/pt (180 points). Estimated run time for scan is 3 min. 18 seconds. Measure offsets. Gains are I0 20 nA/V; IT 10 nA/V.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>We took the harmonic rejection mirror back to zero angle to double check the angle calibration. The mirror not have been correctly aligned for the previous measurements, and we may want to repeat HARMONIC CONTENT evaluation.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>BREAK FOR LUNCH 12:43.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Construction noise seemed to settle down around 3pm. At least most of the grinding, drilling, and hammering has stopped.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><br clear=ALL style='page-break-before:always'> </span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>DATA QUALITY: Experiment log<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Transmission EXAFS of solutions with 0.1 edge step in ca. 2 absorption lengths of water. Cover a range of energies (Cl, Zn, Cd).<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Solutions and transmission cells prepared by Matt Newville using dilution calculations by Bruce Ravel.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>zinc nitrate <o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>445 mg Zn(NO<sub>3</sub>)2•6H<sub>2</sub>O (Alfa #22403)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>was dissolved into ≈40 ml H<sub>2</sub>O (Fischer W2-4 DIVF water) and stirred for 5 minutes.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>The solution was then brought to 50 ml.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>cadmium nitrate<sub><o:p></o:p></sub></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>626 mg Cd(NO<sub>3</sub>)2•6H<sub>2</sub>O (Alfa #21853)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>was dissolved in ≈25 ml H<sub>2</sub>O (Fischer W2-4 DIVF water) and stirred for 5 minutes.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>The solution was then brought to 30 ml.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Beamline 10% detuned on pre-slit; HR mirror at 5 mRad; N2 in I0 (15 cm) and IT (30 cm) at 600 VDC.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Beamline Ar in I0 (15 cm) and IT (30 cm) at 600 VDC; HR mirror to 2.3 mRad; close slits to 800 µm x 10,000 µm; beam height changed with large energy change (from 10 keV to 20 keV); The flux seems too low, so SH takes the HR mirror back to zero angle and adjusts height to center in beam. It was off by 800 µm, which is the same as the entrance slit height, so this error had a huge effect on the flux. Nominal Cd edge position is 26,713 eV.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><span style="mso-spacerun: yes"> </span>EXAFS scan parameters saved as JPEG.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Cd and Zn have comparable flux, noise, and reproducibiliby.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>(6) FLUX at 10 keV: Measure on all beamlines with a common detector/amplifier combination.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>ADC 10 cm detector, 1000 VDC, N2 stp, slit size is 1 x 10 mm, 4.1% absorption<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>†calculated using PNC web programs<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><u><![if !supportEmptyParas]> <![endif]><o:p></o:p></u></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>DETECTOR LINEARITY: Experiment Log<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Move a knife edge or aperture across the incident beam and monitor the I0/IT ratio. <o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Apparently there are several different types of linearity tests one could perform. We debate the merits and applicability, and decide to perform a slit scan: scan a narrow slit across the beam horizontally, to see how uniform the detector is from side to side.<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Monochromator detuned 10% on pre-slit; HR mirror at 5 mRad; N2 in I0[15 cm] and IT[30 cm]<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<span style='font-size:10.0pt;font-family:Chalkboard;color:black;mso-ansi-language: EN-US;mso-fareast-language:EN-US'><u><br clear=ALL style='page-break-before: always'> </u></span>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>BEAMLINE OPERATIONS<o:p></o:p></span></p>

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<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Practical limits on energy range for EXAFS (highest and lowest measured spectra)<o:p></o:p></span></p>

<p class=MsoBodyText style='line-height:150%'><span style='color:black'>Chlorine, but requires major modifications to “standard” configuration to reduce attenuation.<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Ease of changing energy<o:p></o:p></span></p>

<p class=MsoBodyText style='line-height:150%'><span style='color:black'>Large energy changes, such as from 10 keV (Zn) to 25 keV (Cd) required some manual adjustment of the optics, including the HR mirror zero, HR mirror tilt (normal, since cutoff energy is different), detuning, slit size (to match HR mirror acceptance), gains, detector gases. <o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Availability of detectors<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Availability of special sample environments (high/low temp., vacuum, pressure, etc.)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Ease of integrating APS Pool Detectors and Equipment<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Data collection software<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>On-line data processing and analysis<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>Sources of systematic errors (random electronic noise, known monochromator glitches, etc.)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><comment><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoBodyText style='line-height:150%'><span style='color:black'>SOFTWARE CAPABILITIES (need to make a table for this)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>maximum number of regions for energy scans<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>k-space scanning<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>k-weighted integration time<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>automatic offset correction<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>macro capabilities<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>plotting capabilities<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>on-line analysis capabilities<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>example of data file header (what information is automatically recorded)<o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'><![if !supportEmptyParas]> <![endif]><o:p></o:p></span></p>

<p class=MsoNormal style='line-height:150%'><span style='font-size:10.0pt; font-family:Chalkboard;color:black'>9.1 % absorption at Cd, 15 cm Ar. estimated flux is 8x10^9 above the edge.<o:p></o:p></span></p>

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APSXAFS/APS_XOR_Eval/20BMNotes/20BMNotes (last edited 2009-10-09 19:51:19 by localhost)