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40m Log |
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Tue Feb 17 16:44:04 2015, Koji, Update, LSC, Delay line installed again
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Tue Feb 17 19:49:51 2015, Koji, Update, LSC, Delay line un-installed again
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Mon Feb 23 21:57:13 2015, Koji, Update, LSC, Delay line installed again (experiment, round 1)
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Tue Feb 24 01:57:01 2015, Jenne, Update, LSC, Modelled effect of relative modulation phase    
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Thu Feb 26 00:20:54 2015, ericq, Update, LSC, Modelled effect of relative modulation phase  
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Thu Feb 26 01:51:39 2015, ericq, Update, LSC, Sideband HOMs   
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Thu Feb 26 01:53:35 2015, Koji, Update, LSC, Modelled effect of relative modulation phase
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Tue Feb 24 23:39:16 2015, Jenne, Update, LSC, Delay line re-installed again
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Wed Feb 25 04:59:47 2015, Jenne, Update, LSC, Delay line re-installed, measurements round 2
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Wed Feb 25 12:16:27 2015, Koji, Update, LSC, Delay line re-installed, measurements round 2
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Wed Feb 25 14:18:28 2015, rana, Update, LSC, Delay line re-installed, measurements round 2
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Wed Feb 25 14:51:13 2015, Jenne, Update, LSC, Delay line un-installed again
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Wed Feb 25 20:00:39 2015, Jenne, Update, LSC, Delay line un-installed again - sensing matrix comparisons
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Wed Feb 25 23:48:57 2015, rana, Update, LSC, some thoughts
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Thu Feb 26 20:02:46 2015, Jenne, Update, LSC, re: some thoughts
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Message ID: 11067
Entry time: Wed Feb 25 14:18:28 2015
In reply to: 11066
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Author: |
rana |
Type: |
Update |
Category: |
LSC |
Subject: |
Delay line re-installed, measurements round 2 |
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The Schnupp asymmetry is definitely not an important parameter (no need for Koji to explode). It only serves to give us a bigger Q phase signal slope, but is not significant for the I phase signals.
The main anomaly is that the REFL33 optical gain (W/m) seems to have been reduced so much by the phase and amplitude adjustment of the 55 MHz modulation signal. One guess is that the true 3f signal is being made not by the (2*f1 - (-f1)) beat, but by some higher order beat. In addition to the usual RF fields produced by the 2 modulations, we must consider that the sidebands on sidebands produce intermodulation fields just after the EOM and so the fields with which we interrogate the PRMI are more complicated.
Jenne's Optickle calculation today should show us what the sensing matrix contribution is from each pair of fields, so that we can have a sensing matrix signal budget.
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