| Subject: Tech Docs Date: Tue, 31 May 2005 11:32:14 -0500 From: Rusyl Wooley Martin, Below is a log entry made by
Rai Weiss with regards to the power supplies. Reference to the
ITM's and ETM's are the test masses located inside the vacuum
system. The comparison to be made is between the ETMX and ETMY
which had the new supplies installed vs. ITMX and ITMY which did
not. In particular, look at the numbers at 60Hz with the inputs
terminated and the bias inputs turned off. I've also included a
link to a series of plots which show the high frequency comb supression
with the toroidal supplies.
User name = reader Password = readonly SURVEY OF THE 60 HZ AND HARMONICS PICKUP AND RF SPECTRA ------------------------------------------------------- R. Amin and R. Weiss We made a survey of the 60 Hz
and harmonics pickup and the RF interference at all four of the test
masses. All measurements were made at the DAQ output of the coil driver
for a variety of conditions. The line frequency and harmonic
measurements were made with a battery operated spectrum analyser to
avoid ground currents. The measurements made in the LVEA would be
invalidated with an instrument having any ground return (the 60 Hz and
harmonic measured amplitudes vary by a factor of 100 depending on
whether the instrument is connected to the line or is operated from
batteries). The measurements at the end stations are much less
dependent on the grounding and could have been made with a instrument
running from the line.
The intent is to establish a baseline before the electronics is moved out of the LVEA. Both end stations have been modified with toroidal balanced mains transformers and the boards have been moved into reduced RFI racks. The interconnections between boards in different racks and long cable runs have been filtered by capacitive RF feedthoughs. The differences between end stations and the LVEA give some indication what can be expected when the move has been completed in the LVEA. The following two log entries are graphical summaries of the measurements. The first shows the low frequency spectra (1 to 400 Hz) at the end stations ETM and then that of the LVEA ITM. The lower of the curves is the case where the bias connections have been removed and the coil driver input has been terminated in 50 ohms. The upper curves are for local damping on, optical lever damping off, the asc and asc inputs off, the system is in run mode, the digital whitening is off, the analog whitening is on, the de whitening is off. ETMY when being damped is experiencing an oscillation at 46.8 Hz and harmonics. This needs to be investigated. The significant difference between the etm and itm are the amplitude of the 60 Hz harmonics which are smaller at the etm. The table below shows the differences. There is, however, another difference in that the broad band noise (1 to 400 Hz) at the ends is higher than in the LVEA. This also needs further investigation. MEASUREMENTS AT THE DAQ OUTPUT OF THE COIL DRIVER (all values averaged over the UL,LL,UR,LR outputs and measured with a battery operated analyser)
Line harmonic amplitude microvolts rms
Mass conditions 60 120 180 240 300 360 ETMY input term., bias off 0.9 <0.02 0.09 <0.02 0.04 <0.02 ETMY damp on, run, dewh off 19 <0.1 1.2 <0.1 0.7 <0.1 lsc and asc off ETMX input term., bias off 0.3 <0.02 0.18 <0.02 0.07 <0.02 ETMX damp on, run, dewh off 3.3 <0.1 5.7 <0.1 1.2 <0.1 lsc and asc off ITMX input term., bias off 13 <0.03 0.14 <0.03 0.18 <0.03 ITMX damp on, run, dewh off 15 0.84 3.8 0.5 2.0 0.24 lsc and asc off ITMY input term., bias off 14 0.2 0.6 0.15 0.14 0.04 ITMY damp on, run, dewh off 16 1.0 4.2 0.6 2.2 0.26 lsc and asc off The second graphics entry are
the RF spectra taken with the HP RF spectrum analyser and a powered FET
probe. The measurements are again taken at the DAQ output of the coil
driver. The figures show the spectra between 100kHz and 70 MHz and then
another concentrating on the band between 100 kHz and 10 MHz. The first
two figures are composites for all the test masses, the following
figures are for individual masses and are easier to follow. The end
masses overall are considerably RF quieter than the LVEA test masses.
However, in the band 100kHz to about 2.3 MHz a significant RF source
has been planted in the end stations. We should try to find this. The
source has an abrupt drop off in the spectrum at 2.3 MHz and is the
same at both X and Y ends. ETMY is better than ETMX at higher
frequencies and this also is worth chasing.
Rusyl Rusyl J. Wooley Sr. Electronics Engineer California Institute of Technology LIGO Livingston Observatory 19100 LIGO Lane P. O. Box 940 Livingston, LA 70754 |