Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation

被引：39

作者：

Catalano, A. ^{[1
]}

Ade, P. ^{[2
]}

Atik, Y. ^{[3
]}

Benoit, A. ^{[4
]}

Breele, E. ^{[5
]}

Bock, J. J. ^{[6
,7
]}

Camus, P. ^{[4
]}

Chabot, M. ^{[8
]}

Charra, M. ^{[3
]}

Crill, B. P. ^{[7
]}

Coron, N. ^{[3
]}

Coulais, A. ^{[9
]}

Desert, F-X ^{[10
]}

Fauvet, L. ^{[11
]}

Giraud-Heraud, Y. ^{[5
]}

Guillaudin, O. ^{[1
]}

Holmes, W. ^{[7
]}

Jones, W. C. ^{[12
]}

Lamarre, J. -M. ^{[9
]}

Macias-Perez, J. ^{[1
]}

Martinez, M. ^{[3
]}

Miniussi, A. ^{[3
]}

Monfardini, A. ^{[4
]}

Pajot, F. ^{[3
]}

Patanchon, G. ^{[5
]}

Pelissier, A. ^{[1
]}

Piat, M. ^{[5
]}

Puget, J. -L. ^{[3
]}

Renault, C. ^{[1
]}

Rosset, C. ^{[5
]}

Santos, D. ^{[1
]}

Sauve, A. ^{[13
]}

Spencer, L. D. ^{[2
]}

Sudiwala, R. ^{[2
]}

机构：

[1] Univ Grenoble 1, Lab Phys Subatom & Cosmol, Inst Natl Polytech Grenoble, CNRS,IN2P3, F-38026 Grenoble, France

[2] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[3] Univ Paris 11, Inst Astrophys Spatiale, CNRS, UMR 8617, F-91405 Orsay, France

[4] Univ Grenoble 1, CNRS, Inst Neel, F-38042 Grenoble, France

[5] Univ Paris 07, CNRS, UMR 7164, F-75205 Paris, France

[6] CALTECH, Pasadena, CA 91125 USA

[7] CALTECH, Jet Prop Lab, Pasadena, CA USA

[8] Univ Paris 11, IPN Inst Phys Nucl, CNRS, IN2P3, F-91406 Orsay, France

[9] Observ Paris, CNRS, LERMA, F-75014 Paris, France

[10] Univ Grenoble 1, IPAG Inst Planetol & Astrophys Grenoble, CNRS, INSU,UMR 5274, F-38041 Grenoble, France

[11] European Space Agcy, Estec, NL-2201 AZ Noordwijk, Netherlands

[12] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[13] CNRS, IRAP, F-31028 Toulouse 4, France

来源：

ASTRONOMY & ASTROPHYSICS | 2014年 / 569卷

关键词：

instrumentation: detectors; space vehicles: instruments; methods: data analysis; cosmic background radiation; cosmic rays; HIGH-FREQUENCY INSTRUMENT; BOLOMETERS; PERFORMANCE; READOUT;

D O I：

10.1051/0004-6361/201423868

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Planck High Frequency Instrument (HFI) surveyed the sky continuously from August 2009 to January 2012. Its noise and sensitivity performance were excellent (from 11 to 40 aW Hz(-1)), but the rate of cosmic-ray impacts on the HFI detectors was unexpectedly higher than in other instruments. Furthermore, collisions of cosmic rays with the focal plane produced transient signals in the data (glitches) with a wide range of characteristics and a rate of about one glitch per second. A study of cosmic-ray impacts on the HFI detector modules has been undertaken to categorize and characterize the glitches, to correct the HFI time-ordered data, and understand the residual effects on Planck maps and data products. This paper evaluates the physical origins of glitches observed by the HFI detectors. To better understand the glitches observed by HFI in flight, several ground-based experiments were conducted with flight-spare HFI bolometer modules. The experiments were conducted between 2010 and 2013 with HFI test bolometers in different configurations using varying particles and impact energies. The bolometer modules were exposed to 23 MeV protons from the Orsay IPN Tandem accelerator, and to Am-241 and Cm-244 alpha-particle and Fe-55 radioactive X-ray sources. The calibration data from the HFI ground-based preflight tests were used to further characterize the glitches and compare glitch rates with statistical expectations under laboratory conditions. Test results provide strong evidence that the dominant family of glitches observed in flight are due to cosmic-ray absorption by the silicon die substrate on which the HFI detectors reside. Glitch energy is propagated to the thermistor by ballistic phonons, while thermal diffusion also contributes. The average ratio between the energy absorbed, per glitch, in the silicon die and that absorbed in the bolometer is equal to 650. We discuss the implications of these results for future satellite missions, especially those in the far-infrared to submillimeter and millimeter regions of the electromagnetic spectrum.

引用

页数：11

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