UMN CDMS Wiki archive
start › cdms › k100 › run_diary › 20161102

2016/11/02 (Wednesday)

Previous Day

Setup: DIB1/3/4 → 3.2 MHz filters → cables 1,2,3 → HV board inputs 1,3,2 → HV board outputs 1,2 → DCRC55(1)/50(3)
0845 Tower/MC/Coldplate = 31.8/34.6/214 mK, Still = 1.19 K / 120 μbar, G1/G2 = 165/150 mbar, 1K Pot = 1.72 K / 36 mbar. MB = 49.7%.
Boiloff rate: closer to slow-mode than fast-mode
0845 Return Cf source to safe.
0855 Fill LN2 cold trap bath.
1100 Begin re-measuring Rp and Rn for DCRC1pA. Bill Page has suggested we not use the calculation method from Monday, in which the assumption was that Rshunt has a parasitic resistance equal to the Rtes parasitic resistance. He says that there are fewer wirebonds on the Rshunt line so you can expect lower parasitic resistance. His suggestion is that, as a rule, you should assume the total resistance of shunt plus its parasitic is 24 mΩ. Bill is going to look over the old schematic tonight to confirm/deny that there are fewer millmax pins on the Rshunt leg. We can compare the two techniques using data taken on Monday:
Assuming equal parasitic
resistance in each branch
Assuming 4 mΩ parasitic
on the shunt branch
Channel Rpar [mΩ] Rn [mΩ] Rpar [mΩ] Rn [mΩ]
HV1pA 11.3 125 8.7 96
HV1pB 10.8 116 8.4 90
HV1pC 15.2 105 10.3 72
HV2pB 17.0 147 11.0 95
HV2pC 11.0 139 8.6 107
HV2pD 21.6 148 12.4 85

It's difficult to say which seems more consistent. We don't expect a correlation between Rparasitic (which is assumed to be at the SQUET) and Rnormal (which is at the detector). There is a slightly stronger correlation in the equal-parasitic-in-each-branch method, suggesting that it is more biased. At any rate we will for now adopt Bill's method and assume that the shunt resistance is 24 mΩ.

1100 Remeasure Rparasitic of HV1pA using baseline-shifts (IbIs) at QET bias = 0 and 20 μA. The equal-parasitic method gives Rpar = 11.1 mΩ, the Rshunt=24 method gives Rpar = 8.6 mΩ. These are quite close to Monday's values.
1105 Use a test signal on the QET bias (18 mVpp, 100 Hz) to measure HV1pA Rpar. QET bias set to 20 μA. Using the Rshunt=24 assumption this gives Rpar = 10.5 mΩ, significantly higher than the IbIs method. That's strange - it may suggest that the assumption that Rbias = 10 kΩ (used to convert test signal voltage to current) is not quite correct.
1110 Measure Rn using a test signal as above but with QET bias set to 400 μA to drive the TES normal. After subtracting Rpar this yields Rn = 103 mΩ.
1125 Measure Rn by heating the fridge. Applied 40 mW to MC heater to heat fridge to 80 mK which is above the transition of HV1pA. Use the test signal as above with QET bias = 0 μA. We get nearly the same Rn, 102 mΩ.
1245 Measure Rn and Rbiased using the IbIs method. Find Rn = 117 mΩ with equal-parasitic assumption, Rn = 90 mΩ with Rshunt=24 assumption. This is about 6% smaller than Monday's values regardless of which assumption is used. It's pretty close to the Rn value we measured today using a test signal. At the new operating QET bias of 185 μA, we find Rbiased = 65/48 mΩ, 56/53 % of Rn, depending on the equal-parasitic/Rshunt=24 assumption.
1420 Send the detector shipping vessel and wood crate to TAMU so they can use it to ship the next HV detector
1530 Build half of the lead/poly shield. The two permanent walls are on the north- and south-sides of the fridge this time as opposed to the previous east- and west-side arrangement.
1537 Start zero-bias data series with QETbiases = 0 (superconducting), Frontend Gain = 5/5, OG = 2/2, all randoms at 20Hz, with no flashing, with all trace lengths set to 20 ms. Intent is to take long-trace randoms only for noise studies. OOPS - did not mean to have OG = 2/2
1544 Start zero-bias data series with QETbiases = 0 (superconducting), Frontend Gain = 5/5, OG = 8/8, all randoms at 20Hz, with no flashing, with all trace lengths set to 20 ms. Intent is to take long-trace randoms only for noise studies.
1552 Stop data
1556 07161102_1556 - Take another superconducting data set with 52.4288ms (65526 bin) traces. Notes: DCRC 1, channel C looks anomalously noisy
1610 Apply 50 mW to the MC heater to heat the TESs to their normal state. Should target 105 mK to insure we're above all the Tcs.
1615 Tower = 85 mK and rising slowly. Bump the MC power to 60 mW.
1622 07161102_1621 - Normal-state data set with 52.4288ms (65526 bin) traces, with Tbase = 102mK. Notes: DCRC 1, channel C again looks anomalously noisy
1631 Normal-state data set with 20ms traces, to make Matt happy
1636 set MC heater back to 0mW now that normal data is acquired
1720 MB = 36.7%
1725 Begin LHe transfer @ 35.8%
1752 Finish LHe transfer @ MB = 91.3%
1755 Fill LN2 cold trap bath
1800 Place Cf source near cryostat at detector height for activation.
1807 Release pressure from main bath
1853 Release pressure from the main bath
2000 looked at SC and normal data above. Unfortunately channel DCRC1chC, as predicted above, was inhibitively noisy. A fair amount of SQUID zapping and DCRC power cycling was required to get DCRCs in reasonable order. DCRC3, in fact, became noisy on all channels before power cycling/SQUID zapping bought it's channels down to the level of DCRC1 (and still channel B on DCRC3 was the worste of all 6 channels)
2105 started SC series but had wrong trace length (only 50ms)
2108 started SC series with correct 52.4288ms traces … this is crap too because ch B railed at some point.
2118 07161102_2117 finally started hopefully good SC series with 52.4288ms traces … DCRC3chB has a peak at 100Hz that we'll have to live with
2138 the DCRC1 test signal has been malfunctioning. turning it on automatically sends a signal down channel B, with no ability to turn it off. This is not a GUI bug because the ODB reflects the changes made from the GUI. Either this is a driver bug or a DCRC firmware bug. Also have a new series with normal data: 07161102_2332

Next Day