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Journal articles
Characterization and physical explanation of energetic particles on Planck HFI instrument
A. Catalano
1
P. Ade
Y. Atik
A. Benoit
2
E. Bréelle
3
J.J. Bock
P. Camus
4
M. Charra
B.P. Crill
N. Coron
A. Coulais
5
F.X. Dèsert
L. Fauvet
Y. Giraud-Héraud
6, 3
O. Guillaudin
1
W. Holmes
W.C. Jones
J.M. Lamarre
5
J. Macias-Perez
1
M. Martinez
A. Miniussi
3
Alessandro Monfardini
2
F. Pajot
G. Patanchon
3
A. Pelissier
1
M. Piat
3
J.L. Puget
C. Renault
1
C. Rosset
3
D. Santos
1
A. Sauvé
L. Spencer
R. Sudiwala
A. Miniussi 3
Author
Alessandro Monfardini 2
Author
F. Pajot
Author IdHAL : francois-pajot
G. Patanchon 3
Author
R. Sudiwala
Author
1
LPSC - Laboratoire de Physique Subatomique et de Cosmologie (53 avenue des Martyrs - 38026 Grenoble Cedex - France)
- UJF - Université Joseph Fourier - Grenoble 1 (BP 53 - 38041 Grenoble Cedex 9 - France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- Institut Polytechnique de Grenoble - Grenoble Institute of Technology (France)
- CNRS - Centre National de la Recherche Scientifique : UMR5821 (France)
2
HELFA - Hélium : du fondamental aux applications (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- NEEL - Institut Néel (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- UJF - Université Joseph Fourier - Grenoble 1 (BP 53 - 38041 Grenoble Cedex 9 - France)
- CNRS - Centre National de la Recherche Scientifique : UPR2940 (France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
3
APC (UMR_7164) - AstroParticule et Cosmologie (APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7164 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7164 (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
4
Cryo - Cryogénie (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- NEEL - Institut Néel (Institut NEEL, 25 rue des Martyrs, BP 166,
38042 Grenoble cedex 9 - France)
- Grenoble INP - Institut polytechnique de Grenoble - Grenoble Institute of Technology (46 avenue Félix Viallet 38031 Grenoble Cedex 1 - France)
- CNRS - Centre National de la Recherche Scientifique : UPR2940 (France)
- UGA [2016-2019] - Université Grenoble Alpes [2016-2019] (38058 Grenoble cedex - France)
5
LERMA - Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (61, avenue de l'Observatoire - 75014 PARIS - France)
- ENS Paris - École normale supérieure - Paris (45, Rue d'Ulm - 75230 Paris cedex 05 - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- UCP - Université de Cergy Pontoise : UMR8112 (33 Boulevard du Port, 95011 Cergy-Pontoise Cedex - France)
- Université Paris-Seine (3 avenue Bernard Hirsch, CS 50105, 95021 Cergy-Pontoise - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8112 (France)
6
APC - Cosmologie (France)
- APC (UMR_7164) - AstroParticule et Cosmologie (APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7164 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7164 (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
Abstract : The Planck High Frequency Instrument (HFI) has been surveying the sky continuously from the second Lagrangian point (L2) between August 2009 and January 2012. It operates with 52 high impedance bolometers cooled at 100 mK in a range of frequency between 100 GHz and 1 THz with unprecedented sensitivity, but strong coupling with cosmic radiation. At L2, the particle flux is about 5 hbox {cm}^{-2} hbox {s}^{-1} and is dominated by protons incident on the spacecraft. Protons with an energy above 40 MeV can penetrate the focal plane unit box causing two different effects: glitches in the raw data from direct interaction of cosmic rays with detectors (producing a data loss of about 15 % at the end of the mission) and thermal drifts in the bolometer plate at 100 mK adding non-Gaussian noise at frequencies below 0.1 Hz. The HFI consortium has made strong efforts in order to correct for this effect on the time ordered data and final Planck maps. This work intends to give a view of the physical explanation of the glitches observed in the HFI instrument in-flight. To reach this goal, we performed several ground-based experiments using protons and α particles to test the impact of particles on the HFI spare bolometers with a better control of the environmental conditions with respect to the in-flight data. We have shown that the dominant part of glitches observed in the data comes from the impact of cosmic rays in the silicon die frame supporting the micro-machined bolometric detectors propagating energy mainly by ballistic phonons and by thermal diffusion. The implications of these results for future satellite missions will be discussed.
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Journal articles
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http://hal.in2p3.fr/in2p3-00847209
Contributor : Emmanuelle Vernay <>
Submitted on : Tuesday, March 25, 2014 - 8:41:40 AM
Last modification on : Thursday, July 1, 2021 - 5:32:20 PM
Contributor : Emmanuelle Vernay <>
Submitted on : Tuesday, March 25, 2014 - 8:41:40 AM
Last modification on : Thursday, July 1, 2021 - 5:32:20 PM
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- HAL Id : in2p3-00847209, version 1
- ARXIV : 1403.5639
- BIBCODE : 2014JLTP..176..773C
- DOI : 10.1007/s10909-014-1116-6
Collections
APC | LPSC | CNRS | IN2P3 | CEA | UNIV-PARIS7 | OBSPM | NEEL | USPC | IRFU-APC | DSM-IRFU | CEA-DRF | UNIV-PARIS | GEPI | UP-SCIENCES | LERMA | ENS-PARIS | SORBONNE-UNIVERSITE | SU-SCIENCES | UPMC | UNIV-CERGY | INSU | PSL | UGA | SU-TI
Citation
A. Catalano, P. Ade, Y. Atik, A. Benoit, E. Bréelle, et al.. Characterization and physical explanation of energetic particles on Planck HFI instrument. Journal of Low Temperature Physics, Springer Verlag (Germany), 2014, 176 (5-6), pp.773-786. ⟨10.1007/s10909-014-1116-6⟩. ⟨in2p3-00847209⟩
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