The summer project will entail modifying pre-existing automated noise budget code for use on the 40M with an eye for cross-site compatibility. New sensors will be added to the noise budget calculations.
SURF Progress Report #1:
attachment:MaxJonesProgressReport_RoughDraft_3.pdf
SURF Progress Report #2
attachment:MaxJonesSecondProgressReport_RD_1.pdf
SURF Abstract
attachment:SURFAbstract.pdf
Current Status of the 40 m Noise Budget (by source): DARM - Plotting. LSCmodel.m must be revised. MICH - Plotting. PRC - Plotting. Oscillator - Plotting. OpticalLevers - Plotting. WFS - Not yet plotting. OSEM - Not yet plotting. Seismic - Plotting. It may be necessary to obtain new stack and pendulum transfer functions,
- but otherwise accurate. Re-Written.
ETM - Plotting. ITM - Plotting. BS - Plotting. SusTherm - Plotting. IntTherm - Plotting. Shot - Not Yet plotting. Dark - Not Yet plotting. Intensity - Plotting. Frequency - Plotting.
The addition of sources to the 40 m noise budget follows the following steps: 1) Modify the scripts (usually NoiseBudget.m, get(insert noise source).m and get_dtt_dataset.m) to accept
- and plot data from 40 m channels. Often Hanford or Livingston parameters or transfer functions are used