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==Cryogenics==
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__TOC__
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<span style="color:red">(F .Pajot)</span>
 
  
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===Dilution===
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==The dilution cooler==
  
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The HFI 3He-4He dilution cooler produces temperatures of 0.1 K for the bolometers through  
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The HFI dilution cooler cools the bolometers down to 0.1 K through  
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the dilution of 3He into 4He and 1.4 K through JT expansion of the 3He and 4He mixture. The  
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the dilution of <sup>3</sup>He into <sup>4</sup>He and the intermediate optical plate to 1.4 K through Joule-Thomson expansion of the <sup>3</sup>He and <sup>4</sup>He mixture. Two stages of PID regulation are included on the 0.1K stage. The first one (PID1) is at the dilution cold end itself and provides stability on long timescales. When no thermal perturbation is applied to the bolometer plate, the PID1 alone provides the required stability. A passive thermal filter is mounted between the dilution cold end and the bolometer optical plate. It gives a thermal time constant of several hours between these stages. A second regulation system (PID2) is on the bolometer plate, with a similar time constant. The dilution cooler is described in detail in section 2.3.3 of {{PlanckPapers|planck2011-1-3|7}}.
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dilution cooler is described in detail in section 2.3.3 of {{PEarly|2|page=7}}.
 
  
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The dilution was operated with flows set to the minimum available values, and provided a total
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[[Image:HFI_2_4_1_overal_cryo.jpg|thumb|500px|center|Thermal architecture of Planck/HFI]]
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lifetime of 30.5 months, exceeding the nominal lifetime of 16 months by 14.5 months. The
 
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dilution stage was stabilized by a PID control with a regulating power between 20 and 30 nW
 
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providing a temperature close to 101 mK. The bolometer plate was stabilized at 102.8 mK with about 5 nW dissipated
 
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by PID regulation. The cooling power values were in very good agreement with those obtained during the ground tests and calibration.
 
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However, the cosmic particles interactions with the 100 mK stages induced temperature fluctuations and glitches on the thermometers measurements.
 
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The baseline correction of the bolometers signals from the 100 mK bolometer stage temperatures fluctuations is described in the [[TOI processing]] section.
 
  
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[[Image:HFI_2_4_1_100mK_stability.png|thumb|500px|100 mK stages temperatures during the mission]]
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The dilution was operated with flows set to the minimum available values, providing a total
 +
lifetime of 30.5 months exceeding the nominal lifetime of 16 months by 14.5 months. The
 +
dilution stage was stabilized by the PID1 at a temperature close to 101 mK using 20 to 30 nW of power. The bolometer plate was stabilized by the PID2 at 102.8 mK with about 5 nW. The cooling power values were in very good agreement with those obtained during the ground tests and calibration.
  
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At very low frequency, below 1 mHz, the temperature fluctuations are very well correlated with the high energy particles hit rate, as measured by the on-board monitor. At frequencies in the 10 mHz to 1 Hz range, single events inducing a global or partial temperature change of the bolometer plate are observed.
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[[Image:HFI_2_4_1_100mK_stability.png|thumb|500px|center|100mK stages temperatures during the mission]]
  
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[[Image:HFI_2_4_1_1_6K_stability.png|thumb|500px|1.4K stage temperatures during the mission]]
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However, the cosmic particles interactions with the 0.1K stage induced both temperature fluctuations of the 0.1K plates and glitches on the thermometer measurements.
  
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The 1.4K stage is very stable and given the very low coupling coefficients between the 1.4K optical components and the detectors no effect can be measured on the signal.
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At very low frequency, below 1 mHz, the temperature fluctuations are very well correlated with the hit rate of high energy particles, as measured by the on-board Standard Radiation Environment Monitor (SREM). At frequencies in the 10 mHz to 1 Hz range, single events inducing a global or partial temperature change of the bolometer plate are observed. Decorrelation of the bolometer signal from the thermal fluctuations is described in the [[TOI processing#Thermal template for decorrelation|TOI processing]] section.
  
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Detailed thermal analysis of the in-flight stability of the  
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[[Image:HFI_2_4_1_100mK_srem.png|thumb|500px|center|Correlation between the TC1 hits count of the SREM (protons of energy larger than 20 MeV) and the 100 mK bolometer plate temperature]]
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The 1.4K stage is very stable and given the very low coupling coefficients between the 1.4K optical components and the detectors no effect can be measured on the signal. Detailed thermal analysis of the in-flight stability of the  
 
dilution cooler can be found in section  
 
dilution cooler can be found in section  
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5.4 of {{PEarly|2|page=23}}.
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5.4 of {{PlanckPapers|planck2011-1-3|23}}.
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[[Image:HFI_2_4_1_1_6K_stability.png|thumb|500px|center|1.4K stage temperatures during the mission]]
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<div style="clear: both"></div>
 
<div style="clear: both"></div>
  
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=== 4K J-T cooler ===
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==The 4K J-T cooler ==
  
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The HFI 4K J-T cooler produces a temperature of  
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The HFI 4K Joule-Thomson (J-T) cooler produces a temperature of  
 
4K for the HFI 4K stage and optics and the  
 
4K for the HFI 4K stage and optics and the  
 
precooling of the dilution gases. Full  
 
precooling of the dilution gases. Full  
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description of the 4K cooler can be found in
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description of the 4K cooler can be found  
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in section 2.3.2 of {{PEarly|2|page=7}}.
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in section 2.3.2 of {{PlanckPapers|planck2011-1-3|7}}.
  
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The 4K cooler was operated without interruption  
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The two mechanical compressors produce micro-vibrations and also induce electromagnetic interference affecting the science signals of bolometers. The risks associated with these effects were taken into account early in the design of the HFI by phase-locking the sample frequency of the data to a harmonic of the compressor frequency. The removal of these interferences is addressed in the [[TOI processing#Thermal template for decorrelation|4K cooler lines variability]] section.
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Operation of the 4K J-T cooler was flawless during the whole mission, but for an unexpected shutdown during the CPV on August 6th 2009, caused by an SEU on the precharge regulator. It never occured again, and the 4K J-T cooler was then operated without interruption  
 
during all the survey phase of the mission. It is  
 
during all the survey phase of the mission. It is  
 
still in operation as it also provides the  
 
still in operation as it also provides the  
 
cooling of the optical reference loads of the  
 
cooling of the optical reference loads of the  
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LFI. The 4K PID stabilizing the temperature of
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LFI.
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the HFI optics is regulated at 4.81 K using a
 
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power around 1.8 mW.
 
  
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[[Image:HFI_2_4_1_4K_stability.png|thumb|500px|4K stage temperatures during the mission]]
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The 4K J-T cooler compressor amplitude was set to 3450 micrometers during the CPV, and was maintained to this value during all the mission. Its cooling power is very stable and gives enough margin to cancel out the fluctuations and drifts induced by the sorption cooler fluctuations and adjustments. The PID stabilizing the temperature of  
−
 
+
the HFI optics is regulated at 4.81K using a power around 1.8mW.
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The 4K J-T cooler compressors amplitude was set to 3450 micrometers during the CPV, and was maintained to this value during all the mission. Its cooling power is very stable and gives enough margin to cancel out the fluctuations induced by the sorption cooler fluctuations and adjustments. Following the unexpected shutdown of the compressors during CPV, their operation was nominal during all the rest of the mission.
 
  
 
Details on the in-flight performance of the  
 
Details on the in-flight performance of the  
 
4K J-T cooler can be found in in section  
 
4K J-T cooler can be found in in section  
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5.3 of {{PEarly|2|page=21}}.
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5.3 of {{PlanckPapers|planck2011-1-3|21}}.
 +
 
 +
[[Image:HFI_2_4_1_4K_stability.png|thumb|500px|center|4K stage temperatures during the mission]]
 +
 
  
 
<div style="clear: both"></div>
 
<div style="clear: both"></div>
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== References ==
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<References />
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[[Category:HFI design, qualification and performance|001]]

Latest revision as of 15:36, 22 July 2014

The dilution cooler[edit]

The HFI dilution cooler cools the bolometers down to 0.1 K through the dilution of 3He into 4He and the intermediate optical plate to 1.4 K through Joule-Thomson expansion of the 3He and 4He mixture. Two stages of PID regulation are included on the 0.1K stage. The first one (PID1) is at the dilution cold end itself and provides stability on long timescales. When no thermal perturbation is applied to the bolometer plate, the PID1 alone provides the required stability. A passive thermal filter is mounted between the dilution cold end and the bolometer optical plate. It gives a thermal time constant of several hours between these stages. A second regulation system (PID2) is on the bolometer plate, with a similar time constant. The dilution cooler is described in detail in section 2.3.3 of Planck-Early-II[1].

Thermal architecture of Planck/HFI

The dilution was operated with flows set to the minimum available values, providing a total lifetime of 30.5 months exceeding the nominal lifetime of 16 months by 14.5 months. The dilution stage was stabilized by the PID1 at a temperature close to 101 mK using 20 to 30 nW of power. The bolometer plate was stabilized by the PID2 at 102.8 mK with about 5 nW. The cooling power values were in very good agreement with those obtained during the ground tests and calibration.

100mK stages temperatures during the mission

However, the cosmic particles interactions with the 0.1K stage induced both temperature fluctuations of the 0.1K plates and glitches on the thermometer measurements.

At very low frequency, below 1 mHz, the temperature fluctuations are very well correlated with the hit rate of high energy particles, as measured by the on-board Standard Radiation Environment Monitor (SREM). At frequencies in the 10 mHz to 1 Hz range, single events inducing a global or partial temperature change of the bolometer plate are observed. Decorrelation of the bolometer signal from the thermal fluctuations is described in the TOI processing section.

Correlation between the TC1 hits count of the SREM (protons of energy larger than 20 MeV) and the 100 mK bolometer plate temperature

The 1.4K stage is very stable and given the very low coupling coefficients between the 1.4K optical components and the detectors no effect can be measured on the signal. Detailed thermal analysis of the in-flight stability of the dilution cooler can be found in section 5.4 of Planck-Early-II[1].

1.4K stage temperatures during the mission


The 4K J-T cooler[edit]

The HFI 4K Joule-Thomson (J-T) cooler produces a temperature of 4K for the HFI 4K stage and optics and the precooling of the dilution gases. Full description of the 4K cooler can be found in section 2.3.2 of Planck-Early-II[1].

The two mechanical compressors produce micro-vibrations and also induce electromagnetic interference affecting the science signals of bolometers. The risks associated with these effects were taken into account early in the design of the HFI by phase-locking the sample frequency of the data to a harmonic of the compressor frequency. The removal of these interferences is addressed in the 4K cooler lines variability section.

Operation of the 4K J-T cooler was flawless during the whole mission, but for an unexpected shutdown during the CPV on August 6th 2009, caused by an SEU on the precharge regulator. It never occured again, and the 4K J-T cooler was then operated without interruption during all the survey phase of the mission. It is still in operation as it also provides the cooling of the optical reference loads of the LFI.

The 4K J-T cooler compressor amplitude was set to 3450 micrometers during the CPV, and was maintained to this value during all the mission. Its cooling power is very stable and gives enough margin to cancel out the fluctuations and drifts induced by the sorption cooler fluctuations and adjustments. The PID stabilizing the temperature of the HFI optics is regulated at 4.81K using a power around 1.8mW.

Details on the in-flight performance of the 4K J-T cooler can be found in in section 5.3 of Planck-Early-II[1].

4K stage temperatures during the mission


References[edit]

  1. ↑ 1.01.11.21.3 Planck early results. II. The thermal performance of Planck, Planck Collaboration II, A&A, 536, A2, (2011). Cite error: Invalid <ref> tag; name "planck2011-1-3" defined multiple times with different content Cite error: Invalid <ref> tag; name "planck2011-1-3" defined multiple times with different content Cite error: Invalid <ref> tag; name "planck2011-1-3" defined multiple times with different content

(Planck) High Frequency Instrument

[LFI meaning]: absolute calibration refers to the 0th order calibration for each channel, 1 single number, while the relative calibration refers to the component of the calibration that varies pointing period by pointing period.

Space Radiation Environment Monitor

Calibration and Performance Verification

(Planck) Low Frequency Instrument

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