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| * In the folder 40m_PRFPMI the parameters have been set to mimic the state that the smoo_prfpmi script gets us to. See [[Rana's ilog entry]]. | * In the folder 40m_PRFPMI the parameters have been set to mimic the state that the smoo_prfpmi script gets us to. See [[Rana's ilog entry]]. * The initial conditions are such that the arms are on resonance, the MICH is at 0.8 of a bright fringe, the PRC is at resonance for the carrier (power builds up in the PRC). * Transmission of the signal recycling mirror is set to 1 in the opt40.m parameter file. * Slightly cleaned up version of Kirk's: attachment:powfab.zip . (unzip into the directory where you want your powfab Optickle files) * Added a spob detector to opt40.m. Changed the losses of the optics to be more accurate (from 1ppm). to PR = 60ppm, SR = 60ppm, BS = 100ppm, ITMX = 100ppm, ITMY = 100ppm, ETMX = 100ppm, ETMY = 100ppm. attachment:smoo_PRFPMI.tar.gz = Optickle and Looptickle files for the DRFPMI at the 40m = Get the last version of Optickle and Looptickle http://blue.ligo-wa.caltech.edu:8000/advligo/ISC_Modeling_Software __OPTICKLE__ Configuration files for Optickle: attachment:Optickle40m_DRFPM.zip Run cfg40m to create an "opt" file, then run tickle __LOOPTICKLE__ attachment:Looptickle40m_DRFPM.zip "test40m.m" is the script which produces the noise budget. N.B.: Filters and gains are the ones defined in Stefan's model "demo40m.m", TUNING NEEDS TO BE DONE. = Documentation = * [http://www.ligo.caltech.edu/docs/G/G070728-00/G070728-00.pdf Matt's document, "Optickle"] * [http://www.ligo.caltech.edu/~rward/presentations/QND/Optickle.pdf Rob & Matt's talk, "The Optickle Optical Modeling Tool"] * [http://www.ligo.caltech.edu/docs/P/P030071-00.pdf LIGO-P030071-00-R, Mathematical framework for simulation of quantum fields in complex interferometers. using the two-photon formalism] |
Please Update this page !
Optickle for the PRFPMI at the 40m
attachment:Optickle_prfpmi_40m.zip
In the folder 40m_PRFPMI the parameters have been set to mimic the state that the smoo_prfpmi script gets us to. See Rana's ilog entry.
- The initial conditions are such that the arms are on resonance, the MICH is at 0.8 of a bright fringe, the PRC is at resonance for the carrier (power builds up in the PRC).
- Transmission of the signal recycling mirror is set to 1 in the opt40.m parameter file.
- Slightly cleaned up version of Kirk's: attachment:powfab.zip
- (unzip into the directory where you want your powfab Optickle files)
- Added a spob detector to opt40.m. Changed the losses of the optics to be more accurate (from 1ppm). to PR = 60ppm, SR = 60ppm, BS = 100ppm, ITMX = 100ppm, ITMY = 100ppm, ETMX = 100ppm, ETMY = 100ppm. attachment:smoo_PRFPMI.tar.gz
Optickle and Looptickle files for the DRFPMI at the 40m
Get the last version of Optickle and Looptickle http://blue.ligo-wa.caltech.edu:8000/advligo/ISC_Modeling_Software
OPTICKLE
Configuration files for Optickle: attachment:Optickle40m_DRFPM.zip
Run cfg40m to create an "opt" file, then run tickle
LOOPTICKLE
attachment:Looptickle40m_DRFPM.zip
"test40m.m" is the script which produces the noise budget.
N.B.: Filters and gains are the ones defined in Stefan's model "demo40m.m", TUNING NEEDS TO BE DONE.
Documentation
[http://www.ligo.caltech.edu/docs/G/G070728-00/G070728-00.pdf Matt's document, "Optickle"]
[http://www.ligo.caltech.edu/~rward/presentations/QND/Optickle.pdf Rob & Matt's talk, "The Optickle Optical Modeling Tool"]
[http://www.ligo.caltech.edu/docs/P/P030071-00.pdf LIGO-P030071-00-R, Mathematical framework for simulation of quantum fields in complex interferometers. using the two-photon formalism]