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Comment: Schematic
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== Schematic ==

 * [http://www.ligo.caltech.edu/~fnocera/files/ISS%20rev%20D%20nov04.pdf Schematic of 40m ISS servo] - Beware that there are various "Revision D" ISS's floating around; this link is to the 40m version. There is a paper version of this at the 40m that is marked up with further modifications to the 40m ISS.
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|| C1:PSL-ISS_INSENSPD_F || ||
|| C1:PSL-ISS_INSENSPD_FW || ||
|| C1:PSL-ISS_INMONPD_F || ||
|| C1:PSL-ISS_INSE
NPD_FW || ||
|| C1:PSL-ISS_CSDRIVE_F || ||
|| C1:PSL-ISS_CSDRIVE_FW || ||
|| C1:PSL-ISS_INSENSPD_F  || In-loop photodiode ||
|| C1:PSL-ISS_INSENSPD_FW ||  In-loop photodiode, whitened ||
|| C1:PSL-ISS_INMONPD_F   || Out-of-loop photodiode ||
|| C1:PSL-ISS_INMO
NPD_FW  || Out-of-loop photodiode, whitened ||
|| C1:PSL-ISS_CSDRIVE_F   || ||
|| C1:PSL-ISS_CSDRIVE_FW  || ||

The ISS measures the power fluctuations on a photodiode placed after the Mach Zender, but before the Mode Cleaner, and tries to servo that signal to zero.

The ISS is AC-coupled, so its purpose is not to control long-term drift. In its nominal configuration, it has gain from 1-100,000 Hz. This is to suppress the intensity noise in our measurement band.

The ISS servo sits on the PSL table; its a beige box with black front and back panels. All of the hooks for doing fast loop measurements are on that box.

The ISS actuator is the Current Shunt in the MOPA box.

Schematic

DAQ channels

C1:PSL-ISS_INSENSPD_F

In-loop photodiode

C1:PSL-ISS_INSENSPD_FW

In-loop photodiode, whitened

C1:PSL-ISS_INMONPD_F

Out-of-loop photodiode

C1:PSL-ISS_INMONPD_FW

Out-of-loop photodiode, whitened

C1:PSL-ISS_CSDRIVE_F

C1:PSL-ISS_CSDRIVE_FW

PSL/Intensity_Stabilization_Servo (last edited 2020-08-06 22:55:40 by GautamvenugopalanATligoDOTorg)