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This PSD is a measure of the relative susceptibility of each design to
microphonics. Note in the 1 to 10 kHz region, the flexible design is less
susceptible to noise, even though it has higher total noise
The “Fan Contact Ratio” is a measure of the susceptibility of each cable to
microphonic noise. It is greater than 1 at frequencies where the cable is
susceptible to microphonic noise
“Fan Contact” shows the noise on each cable with induced vibrations. This
data alone is not very useful until it is compared with the noise on the cable
without induced vibrations
The “No Contact Ratio” is a sanity check to make sure that all cables are
functioning correctly and an indication that the fan running without making
contact with the fridge is comparable to “At Rest” conditions
“No Contact” noise is the noise with the fan running but not making contact
with anything. This is the background noise and takes into account noise
from both background vibrations and electrical signals.
Based on those PSDs, it appears the flexible cables send a noisier signal,
especially in the 1 to 10 kHz region. Unfortunately, this is the range of
frequencies that the signal is sent in the standard CDMS experiment [3].
The coaxial cables used a 20AWG copper wire as the conductor
with copper foil as the shield. The insulator was 1/32 inch
polyolefin heat shrink tubing, and the insulator was copper tape
wrapped around the insulated wire. Before the heat shrink tubing
was fitted to the conductor, 3 coats of M.E. Taylor Engineering
Aquadag E, Conductive Carbon Paint were applied to the conductor
and left to dry over night. The polyolefin tubing and copper foil
were then applied to this painted conductor to complete the coaxial
cable.
And a LABView DAQ took PSDs of the signal with the fan off,
the fan on but making no contact with the fridge, and the fan on
making contact with the fridge (procedure modified from [2].)
The tower was then installed in the
dilution refrigerator
Then the flexible coax was installed
with a vacuum coax on the tower
The Cryogenic Dark Matter Search (CDMS) experiment's detector
run at 50mK that measures the energy of incoming particles. In
order to be able to probe low energies, its setup is low temperature
and low noise. This poses significant challenges for the charge
readout circuit, which depends on a JFET amplifier which runs
optimally at 150K [1]. All cables need to be coaxial, but this makes
the gate of the JFET highly susceptible to microphonic noise. To
avoid this, CDMS uses coaxial cables with vacuum dielectric. This
requires rigid shielding, which necessitates a bulky copper “tower”
with temperature stages to get the signal from the detector to the
JFET. This project aims to design a coaxial cable that is flexible
(eliminating the need of the tower) and impervious to microphonics.
The readout circuit is shown in the circuit diagram below. The noise
of this circuit is predicted [4] by the equation
Where A(f) is the signal shape defined by
Note that the capacitance of the cable is part of the parasitic
capacitance, Cp. While this is not the main source of the noise in
this run, it will be a main issue when replacing the tower.
This cable has capacitance 30±5pF/ft. This needs to be closer to the
capacitance of the tower, 20pF/foot, in order to keep the parasitic
capacitance close to its current value [5].
The cables' susceptibility to microphonic noise can be seen in how much more noise is on a cable when there are vibration induced on the cable. This relationship is quantified by the ratio of a cable's noise in each condition: noise with
induced microphonics (“Fan Contact”) divided by the noise without induced microphonics (“Fan No Contact”). Note the Qi and Qo are two cables of the same design (flexible or vacuum).
First, the cables had to be soldered to the proper interface boards and the
coaxial shields needed to be grounded
Design of ultra-low noise coaxial cable in cryogenic setup
Christopher Phenicie, University of Minnesota Twin Cities; Advisor: Vuk Mandic
A special thanks to Hassan Chagani, Alex Codoreanu, and David Strandberg
Introduction
Motivation
Logistical Physical
Procedure for measuring power spectrum density
Construction
Measurement of susceptibility to microphonic noise
Conclusion
References
Capacitance
e0
2
=| A( f )|
2
{eFET
2
[(CD+C p+C f )
2
(2 π f )
2
+
( 1
R f
+
1
Rb
)
2
]+4kT
( 1
R f
+
1
Rb
)}
A( f )=
R
1+2πiRf C f
[1] V. Mandic, First Results from the Cryogenic Dark Matter Search
Experiment at the Deep Site, Ph.D. Thesis, Department of Physics,
U. C. Berkeley (2004).
[2] D. Strandberg, Analysis of Microphonic Susceptibility of a
Flexible Side Coax for the Cryogenic Dark Matter Search
Experiment, Senior Thesis, Department of Physics and Astronomy,
University of Minnesota Twin Cities (2012).
[3] D. S. Akerib, et al. Nuclear Instruments and Methods in Physics
Research Section A. 591, (2008).
[4] T. A. Shutt, A Dark Matter Detector Based on the Simultaneous
Measurement of Phonons and Ionization at 20 mK, PhD thesis, U.C.
Berkeley (1993).
[5] Phipps, The CDMS Ionization Readout Capacitance Budget,
Senior Thesis, Department of Physics, U. C. Berkeley (2008).
Analysis of these PSDs showed that, in terms of susceptibility, this
design is at least comparable to the standard vacuum cables.
However, the flexible cable has more net noise in 1kHz to 10kHz
region, which is alarming because the frequencies used for the
signals fall in this range.
One suggested cause of this noise is the graphite paint chipping and
falling off the conductor. Then, any natural vibrations in the fridge
would be seen on the flexible cable but not in the vacuum cable.
Therefore, the next design will have the graphite painted sealed
with GE varnish. The above consideration of capacitance suggests
a stronger dielectric should be used. Therefore, the next design of
the cable will use a vacuum dielectric with plastic spacers to allow
for flexibility
The tower is bulky, so large
amounts of cooling power are
required to maintain
temperature stages. This limits
the ability of the experiment
to scale, since scaling the size
of the tower increases the
amount of copper that needs
to be heat sunk.
The tower is quite difficult to
install in the fridge, mainly due
to its bulk. Eliminating the tower
would cut out hours of work in
installation and de-installation in
between runs on the fridge.
Furthermore, removing the tower
would decrease the risk of heat
leaks, which is fatal for a run

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compressedFinalSideCoaxPoster

  • 1. This PSD is a measure of the relative susceptibility of each design to microphonics. Note in the 1 to 10 kHz region, the flexible design is less susceptible to noise, even though it has higher total noise The “Fan Contact Ratio” is a measure of the susceptibility of each cable to microphonic noise. It is greater than 1 at frequencies where the cable is susceptible to microphonic noise “Fan Contact” shows the noise on each cable with induced vibrations. This data alone is not very useful until it is compared with the noise on the cable without induced vibrations The “No Contact Ratio” is a sanity check to make sure that all cables are functioning correctly and an indication that the fan running without making contact with the fridge is comparable to “At Rest” conditions “No Contact” noise is the noise with the fan running but not making contact with anything. This is the background noise and takes into account noise from both background vibrations and electrical signals. Based on those PSDs, it appears the flexible cables send a noisier signal, especially in the 1 to 10 kHz region. Unfortunately, this is the range of frequencies that the signal is sent in the standard CDMS experiment [3]. The coaxial cables used a 20AWG copper wire as the conductor with copper foil as the shield. The insulator was 1/32 inch polyolefin heat shrink tubing, and the insulator was copper tape wrapped around the insulated wire. Before the heat shrink tubing was fitted to the conductor, 3 coats of M.E. Taylor Engineering Aquadag E, Conductive Carbon Paint were applied to the conductor and left to dry over night. The polyolefin tubing and copper foil were then applied to this painted conductor to complete the coaxial cable. And a LABView DAQ took PSDs of the signal with the fan off, the fan on but making no contact with the fridge, and the fan on making contact with the fridge (procedure modified from [2].) The tower was then installed in the dilution refrigerator Then the flexible coax was installed with a vacuum coax on the tower The Cryogenic Dark Matter Search (CDMS) experiment's detector run at 50mK that measures the energy of incoming particles. In order to be able to probe low energies, its setup is low temperature and low noise. This poses significant challenges for the charge readout circuit, which depends on a JFET amplifier which runs optimally at 150K [1]. All cables need to be coaxial, but this makes the gate of the JFET highly susceptible to microphonic noise. To avoid this, CDMS uses coaxial cables with vacuum dielectric. This requires rigid shielding, which necessitates a bulky copper “tower” with temperature stages to get the signal from the detector to the JFET. This project aims to design a coaxial cable that is flexible (eliminating the need of the tower) and impervious to microphonics. The readout circuit is shown in the circuit diagram below. The noise of this circuit is predicted [4] by the equation Where A(f) is the signal shape defined by Note that the capacitance of the cable is part of the parasitic capacitance, Cp. While this is not the main source of the noise in this run, it will be a main issue when replacing the tower. This cable has capacitance 30±5pF/ft. This needs to be closer to the capacitance of the tower, 20pF/foot, in order to keep the parasitic capacitance close to its current value [5]. The cables' susceptibility to microphonic noise can be seen in how much more noise is on a cable when there are vibration induced on the cable. This relationship is quantified by the ratio of a cable's noise in each condition: noise with induced microphonics (“Fan Contact”) divided by the noise without induced microphonics (“Fan No Contact”). Note the Qi and Qo are two cables of the same design (flexible or vacuum). First, the cables had to be soldered to the proper interface boards and the coaxial shields needed to be grounded Design of ultra-low noise coaxial cable in cryogenic setup Christopher Phenicie, University of Minnesota Twin Cities; Advisor: Vuk Mandic A special thanks to Hassan Chagani, Alex Codoreanu, and David Strandberg Introduction Motivation Logistical Physical Procedure for measuring power spectrum density Construction Measurement of susceptibility to microphonic noise Conclusion References Capacitance e0 2 =| A( f )| 2 {eFET 2 [(CD+C p+C f ) 2 (2 π f ) 2 + ( 1 R f + 1 Rb ) 2 ]+4kT ( 1 R f + 1 Rb )} A( f )= R 1+2πiRf C f [1] V. Mandic, First Results from the Cryogenic Dark Matter Search Experiment at the Deep Site, Ph.D. Thesis, Department of Physics, U. C. Berkeley (2004). [2] D. Strandberg, Analysis of Microphonic Susceptibility of a Flexible Side Coax for the Cryogenic Dark Matter Search Experiment, Senior Thesis, Department of Physics and Astronomy, University of Minnesota Twin Cities (2012). [3] D. S. Akerib, et al. Nuclear Instruments and Methods in Physics Research Section A. 591, (2008). [4] T. A. Shutt, A Dark Matter Detector Based on the Simultaneous Measurement of Phonons and Ionization at 20 mK, PhD thesis, U.C. Berkeley (1993). [5] Phipps, The CDMS Ionization Readout Capacitance Budget, Senior Thesis, Department of Physics, U. C. Berkeley (2008). Analysis of these PSDs showed that, in terms of susceptibility, this design is at least comparable to the standard vacuum cables. However, the flexible cable has more net noise in 1kHz to 10kHz region, which is alarming because the frequencies used for the signals fall in this range. One suggested cause of this noise is the graphite paint chipping and falling off the conductor. Then, any natural vibrations in the fridge would be seen on the flexible cable but not in the vacuum cable. Therefore, the next design will have the graphite painted sealed with GE varnish. The above consideration of capacitance suggests a stronger dielectric should be used. Therefore, the next design of the cable will use a vacuum dielectric with plastic spacers to allow for flexibility The tower is bulky, so large amounts of cooling power are required to maintain temperature stages. This limits the ability of the experiment to scale, since scaling the size of the tower increases the amount of copper that needs to be heat sunk. The tower is quite difficult to install in the fridge, mainly due to its bulk. Eliminating the tower would cut out hours of work in installation and de-installation in between runs on the fridge. Furthermore, removing the tower would decrease the risk of heat leaks, which is fatal for a run