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<p class="MsoNormal">Hi again Sean, <o:p></o:p></p>
<p class="MsoNormal">I also thing that like Andrew suggested, ultimately, changing the latency for these two layers 1 & 3 to center the APV25 peak for the hits in the central area of the detector will address the concern (tracking efficiency)<o:p></o:p></p>
<p class="MsoNormal">Best regards <o:p></o:p></p>
<p class="MsoNormal">Kondo<o:p></o:p></p>
<p class="MsoNormal"><o:p> </o:p></p>
<p class="MsoNormal"><b>From:</b> Sbs_gems <sbs_gems-bounces@jlab.org> <b>On Behalf Of
</b>Sean Jeffas<br>
<b>Sent:</b> Saturday, January 15, 2022 11:02 AM<br>
<b>To:</b> Sbs_gems@jlab.org<br>
<b>Subject:</b> Re: [Sbs_gems] [EXTERNAL] UV Latency Analysis Results<o:p></o:p></p>
<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">Hi All,<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">We have finished analyzing a cosmic test after turning the gas flow down on layers 1 and 3 from 525 cc/min to 375. The data is attached below. For reference:<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal"><b>Run 13240: </b>Taken January 11th with all four UV layers and 2 uA on LH2 at the <span class="gmail-il">SBS</span>-14 kinematic. Gas flow at 525 cc/min<o:p></o:p></p>
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<p class="MsoNormal"><b>Run 12423:</b> Taken January 14th with cosmic data. UV layers 1 and 3 gas flowing at 375 cc/min<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">These runs are a bit difficult to compare since one is with beam and the other is comsic, but it's all that we have. Overall you can see that the timing distribution is a bit better for layer 1 and 3, but still not great. Also the efficiencies
and gains are not significantly reduced by the lower gas flow. So I think we can run with this setting. <o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">Kondo/Nilanga/Xinzhan: Will this reduced gas flow have a greater effect with the beam on? I suppose we will find out in two hours anyway.<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">Also I would be interested in turning up the voltage on layer 1 and module 1 in the XY layer by 25 V. Are there any objections?<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">Best,<br>
Sean<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">On Thu, Jan 13, 2022 at 3:49 PM Sean Jeffas <<a href="mailto:sj9ry@virginia.edu">sj9ry@virginia.edu</a>> wrote:<o:p></o:p></p>
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<p class="MsoNormal">Hi Andrew,<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">I am not sure if you meant to only reply to only me, but here are the plots you asked for. I actually already had them but decided it was kind of overkill.<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">Best,<o:p></o:p></p>
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<p class="MsoNormal">Sean<o:p></o:p></p>
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<p class="MsoNormal"><o:p> </o:p></p>
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<p class="MsoNormal">On Thu, Jan 13, 2022 at 3:21 PM Andrew Puckett <<a href="mailto:puckett@jlab.org" target="_blank">puckett@jlab.org</a>> wrote:<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Hi Sean,
<o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Interesting results. Another interesting way to visualize these results would be in terms of the strip mean times, which might (or might not) have somewhat better resolution than
the time sample peaking distribution. I would also be curious to see a couple of alternative ways of visualizing the data. For example:
<o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<li class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto;mso-list:l0 level1 lfo1">
A more “binary” approach: 1D and 2D distributions vs. x and/or y for hits peaking in sample 5 and for hits NOT peaking in sample 5<o:p></o:p></li><li class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto;mso-list:l0 level1 lfo1">
Same as 1, but perhaps broken out by hits peaking in samples 1, 2, 3, 4, 5, etc.<o:p></o:p></li></ol>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Cheers,<o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Andrew<o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;margin-bottom:12.0pt"><b><span style="font-size:12.0pt;color:black">From:
</span></b><span style="font-size:12.0pt;color:black">Sbs_gems <<a href="mailto:sbs_gems-bounces@jlab.org" target="_blank">sbs_gems-bounces@jlab.org</a>> on behalf of Sean Jeffas <<a href="mailto:sj9ry@virginia.edu" target="_blank">sj9ry@virginia.edu</a>><br>
<b>Date: </b>Thursday, January 13, 2022 at 3:03 PM<br>
<b>To: </b><a href="mailto:Sbs_gems@jlab.org" target="_blank">Sbs_gems@jlab.org</a> <<a href="mailto:sbs_gems@jlab.org" target="_blank">sbs_gems@jlab.org</a>><br>
<b>Subject: </b>[Sbs_gems] [EXTERNAL] UV Latency Analysis Results</span><o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Hi All,<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">I have finished analyzing the spatial distribution of the peak time samples. I have attached the results below for two runs.<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"><b>Run 13240:
</b>Taken January 11th with all four UV layers and 2 uA on LH2 at the SBS-14 kinematic.<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"><b>Run 12423:</b> Taken December 1st with J0 still in the layer 1 position but the UV layer was in layer 3 position. This was 2 uA on LD2 at SBS-11.<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">In the recent run (13240) you can clearly see the peak time sample is uniform over the hit map for every layer except for layer 1 and layer 3. Similarly if you look at the December
run (12423) the same issue was present in layer 3, but we never noticed it because we were always the first and last bin out of the analysis. John and I measured the resistors on the GEMs today and did not find a resistance that would suggest that the gas
window has collapsed onto the cathode. Unfortunately the shielding blocks us from seeing the gas window, otherwise it would be very easy to tell. <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Therefore our current conclusion is that since the GEM layers 1 and 3 both have a non uniform gas flow, this is probably causing some bend in the readout board, which causes this
issue. To fix this we can turn down the gas flow rate and see how everything is affected. Since the experiment is down for a few days it would be good to turn it down today and take some cosmic data, if possible.<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto"> <o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Best,<o:p></o:p></p>
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<p class="MsoNormal" style="mso-margin-top-alt:auto;mso-margin-bottom-alt:auto">Sean<o:p></o:p></p>
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