Reports until 20:27, Wednesday 10 December 2014
H1 ISC
alexan.staley@LIGO.ORG - posted 20:27, Wednesday 10 December 2014 - last comment - 10:18, Friday 19 December 2014(15548)
Ringdown

Evan, Alexa

Following the preparation described in alog 15524, we made a ringdown measurement of both the x- and y-arm. For each arm, we locked the IR beam and ran the wfs to ensure maximum build up. We then turned the wfs off, and switched the input polarity of the MC common mode board to unlock the MC quickly (based on LLO's alog 11727 the MC has about a 15usec ringdown time). We used the relfected signal at the AS port to capture the ringdown. We repeated this measurement 10 times to have ample data for our uncertainities. We also measured the "off-resonance" ringdown, by unlocking the arm and misaligning the respective ETM. All the data can be found in /ligo/home/alexan.staley/Public/Ringdown/EX(Y)data (these folders are then split into locked and unlocked times).  From this data we calculated the total loss:

X arm: 14310(100) ppm

Y arm: 15000(100) ppm

Based on the galaxy ITMY transmissivity (1.42%) this amounts to 800ppm of loss in the y-arm. Meanwhile, for the x-arm, the ITMX transmissivity is 1.39 % corresponding to a 410ppm loss in the arm. We are in the process of calculating the transmissivity of the ITMs based on our ringdown fit. Our code can be found in /ligo/home/alexan.staley/Public/Ringdown/proccess.py. The y-arm losses seems consitent with our scan measurements; however the x arm does not. These numbers are very sensitive to the transmissivity we use; so before we make an conclusion with this we should inprove our confidence in the transmissivity values.

Comments related to this report
evan.hall@LIGO.ORG - 11:14, Thursday 11 December 2014 (15551)

I’ve attached the code, the data, and the plots in a zip file.

Also attached are a few representative plots with the arms locked and unlocked.

Also, Dave wants me to note that the inferred loss of 410 ppm in the X arm is probably wrong; we’ve just pulled the ITMX transmissivity from the galaxy website instead of extracting it from our data. This is in progress.

The time constant of the ringdown is half of the cavity storage time, and the cavity storage time is related to the arm reflectivities by an equation in Isogai (sec 4.3):

	au_{
m{s}} = frac{-1}{f_{
m{fsr}} ln(r_{
m{I}} r_{
m{E}})}

We've assumed that we know RE = 1 − 5×10−6.

Non-image files attached to this comment
evan.hall@LIGO.ORG - 11:06, Thursday 18 December 2014 (15683)

Here are the values for the ITM transmissivities, as inferred from the ringdown data.

In summary, to within experimental error there is no anomalous loss in the X arm. In the Y arm, the anomalous loss is 1330(370) ppm.

An updated version of the code is attached, along with a document giving the expression for TITM in terms of the measured quantities.

Here I've assumed RETM = 1, as was done in the paper by Isogai et al.

[Edit: Alexa has pointed out that we need to use m1 = RITM(P0+P1), rather than the original Isogai formula m1 = P0+P1, since we are using a PD in reflection. I've updated the table and the attachments accordingly. The ITM transmissivities change slightly and the extra losses go up a bit, but the conclusions remain the same.]

  X arm Y arm
m1 201(5) mV 153(5) mV
m2 70(13) mV 467(30) mV
m3 203(16) mV 114(12) mV
m4 1.863(13) ms 1.778(12) ms
ITM transmission, TITM 1.419(35) % 1.366(36) %
Total loss, L 14 310(100) ppm 14 990(100) ppm
L − TITM 120(360) ppm 1330(370) ppm
ITM transmission, TITM 1.425(35) % 1.37(4) %
Total loss, L 14 310(100) ppm 14 990(100) ppm
L − TITM 60(360) ppm 1290(410) ppm

For posterity, the old, incorrect values for the ITM transmissions were 1.425(35) % for X and 1.37(4) % for Y. The incorrect values for the extra losses were 60(360) ppm for X and 1290(410) ppm for Y.

Non-image files attached to this comment
garilynn.billingsley@LIGO.ORG - 10:18, Friday 19 December 2014 (15741)
Check the assumption on ETM transmission?  Our measurement is 3.6 ppm with a tolerance of 0.2 ppm for both LHO ETMs.  https://dcc.ligo.org/LIGO-E1300313