Characterization and Physical Explanation of Energetic Particles on Planck HFI Instrument

被引：14

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
]}

Charra, M. ^{[3
]}

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

Coron, N. ^{[3
]}

Coulais, A. ^{[8
]}

Desert, F. -X. ^{[9
]}

Fauvet, L. ^{[10
]}

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

Guillaudin, O. ^{[1
]}

Holmes, W. ^{[7
]}

Jones, W. C. ^{[11
]}

Lamarre, J. -M. ^{[8
]}

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. ^{[12
]}

Spencer, L. ^{[2
]}

Sudiwala, R. ^{[2
]}

机构：

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

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

[3] Univ Paris 11, CNRS, UMR8617, Inst Astrophys Spatiale, F-91405 Orsay, France

[4] Univ Grenoble 1, CNRS, Inst Neel, F-38026 Grenoble, France

[5] Univ Paris 07, CNRS, UMR 7164, Paris, France

[6] CALTECH, Pasadena, CA 91125 USA

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

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

[9] Univ Grenoble 1, IPAG, Grenoble CNRS INSU 1, UMR 5274, F-38041 Grenoble, France

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

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

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

来源：

JOURNAL OF LOW TEMPERATURE PHYSICS | 2014年 / 176卷 / 5-6期

关键词：

Planck satellite; High impedance bolometers; Cosmic rays;

D O I：

10.1007/s10909-014-1116-6

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

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 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 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.

引用

页码：773 / 786

页数：14

共 11 条

[1] Planck early results. II. The thermal performance of Planck [J].

Ade, P. A. R. ;

Aghanim, N. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Baccigalupi, C. ;

Baker, M. ;

Balbi, A. ;

Banday, A. J. ;

Barreiro, R. B. ;

Battaner, E. ;

Benabed, K. ;

Benoit, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bhandari, P. ;

Bhatia, R. ;

Bock, J. J. ;

Bonaldi, A. ;

Bond, J. R. ;

Borders, J. ;

Borrill, J. ;

Bouchet, F. R. ;

Bowman, B. ;

Bradshaw, T. ;

Breelle, E. ;

Bucher, M. ;

Burigana, C. ;

Butler, R. C. ;

Cabella, P. ;

Camus, P. ;

Cantalupo, C. M. ;

Cappellini, B. ;

Cardoso, J. -F. ;

Catalano, A. ;

Cayon, L. ;

Challinor, A. ;

Chamballu, A. ;

Chambelland, J. P. ;

Charra, J. ;

Charra, M. ;

Chiang, L. -Y. ;

Chiang, C. ;

Christensen, P. R. ;

Clements, D. L. ;

Collaudin, B. ;

Colombi, S. ;

Couchot, F. ;

Coulais, A. ;

Crill, B. P. .

ASTRONOMY & ASTROPHYSICS, 2011, 536

[2] Planck 2013 results. I. Overview of products and scientific results [J].

Ade, P. A. R. ;

Aghanim, N. ;

Alves, M. I. R. ;

Armitage-Caplan, C., I ;

Amaud, M. ;

Ashdown, M. ;

Atrio-Barandela, F. ;

Aumont, J. ;

Ausse, H. ;

Baccigalupi, C. ;

Banday, A. J. ;

Barreiro, R. B. ;

Barrenass, R. ;

Bartelmann, M. ;

Bartlett, J. G. ;

Bartolo, N. ;

Basak, S. ;

Battaner, E. ;

Battye, R. ;

Benabed, K. ;

Benoit, A. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bertincourt, B. ;

Bethermin, M. ;

Bielewicz, P. ;

Bikmaev, I. ;

Blanchard, A. ;

Bobin, J. ;

Bock, J. J. ;

Boehringer, H. ;

Bonaldi, A. ;

Bonavera, L. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bourdin, H. ;

Bowyer, J. W. ;

Bridges, M. ;

Brown, M. L. ;

Bucher, M. ;

Burenin, R. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

Cappellini, B. ;

Cardoso, J. -F. ;

Carr, R. .

ASTRONOMY & ASTROPHYSICS, 2014, 571

[3] Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance [J].

Ade, P. A. R. ;

Aghanim, N. ;

Ansari, R. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Banday, A. J. ;

Bartelmann, M. ;

Bartlett, J. G. ;

Battaner, E. ;

Benabed, K. ;

Benoit, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bhatia, R. ;

Bock, J. J. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bradshaw, T. ;

Breelle, E. ;

Bucher, M. ;

Camus, P. ;

Cardoso, J. -F. ;

Catalano, A. ;

Challinor, A. ;

Chamballu, A. ;

Charra, J. ;

Charra, M. ;

Chary, R. -R. ;

Chiang, C. ;

Church, S. ;

Clements, D. L. ;

Colombi, S. ;

Couchot, F. ;

Coulais, A. ;

Cressiot, C. ;

Crill, B. P. ;

Crook, M. ;

de Bernardis, P. ;

Delabrouille, J. ;

Delouis, J. -M. ;

Desert, F. -X. ;

Dolag, K. ;

Dole, H. ;

Dore, O. ;

Douspis, M. ;

Efstathiou, G. ;

Eng, P. .

ASTRONOMY & ASTROPHYSICS, 2011, 536

[4] PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra [J].

Adriani, O. ;

Barbarino, G. C. ;

Bazilevskaya, G. A. ;

Bellotti, R. ;

Boezio, M. ;

Bogomolov, E. A. ;

Bonechi, L. ;

Bongi, M. ;

Bonvicini, V. ;

Borisov, S. ;

Bottai, S. ;

Bruno, A. ;

Cafagna, F. ;

Campana, D. ;

Carbone, R. ;

Carlson, P. ;

Casolino, M. ;

Castellini, G. ;

Consiglio, L. ;

De Pascale, M. P. ;

De Santis, C. ;

De Simone, N. ;

Di Felice, V. ;

Galper, A. M. ;

Gillard, W. ;

Grishantseva, L. ;

Jerse, G. ;

Karelin, A. V. ;

Koldashov, S. V. ;

Krutkov, S. Y. ;

Kvashnin, A. N. ;

Leonov, A. ;

Malakhov, V. ;

Malvezzi, V. ;

Marcelli, L. ;

Mayorov, A. G. ;

Menn, W. ;

Mikhailov, V. V. ;

Mocchiutti, E. ;

Monaco, A. ;

Mori, N. ;

Nikonov, N. ;

Osteria, G. ;

Palma, F. ;

Papini, P. ;

Pearce, M. ;

Picozza, P. ;

Pizzolotto, C. ;

Ricci, M. ;

Ricciarini, S. B. .

SCIENCE, 2011, 332 (6025) :69-72

[5] RADIATION HARDNESS OF A COMPOSITE BOLOMETER COOLED AT HE-3 TEMPERATURE [J].

CASERTA, A ;

DEBERNARDIS, P ;

MASI, S ;

MATTIOLI, M .

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1990, 294 (1-2) :328-334

[6] Initial test results on bolometers for the Planck high frequency instrument [J].

Holmes, Warren A. ;

Bock, James J. ;

Crill, Brendan P. ;

Koch, Timothy C. ;

Jones, William C. ;

Lange, Andrew E. ;

Paine, Christopher G. .

APPLIED OPTICS, 2008, 47 (32) :5996-6008

[7] Anomalous and Galactic Cosmic Rays at 1 AU During the Cycle 23/24 Solar Minimum [J].

Leske, R. A. ;

Cummings, A. C. ;

Mewaldt, R. A. ;

Stone, E. C. .

SPACE SCIENCE REVIEWS, 2013, 176 (1-4) :253-263

[8] On the effect of cosmic rays in bolometric cosmic microwave background measurements from the stratosphere [J].

Masi, S. ;

Battistelli, E. ;

de Bernardis, P. ;

Lamagna, L. ;

Nati, F. ;

Nati, L. ;

Natoli, P. ;

Polenta, G. ;

Schillaci, A. .

ASTRONOMY & ASTROPHYSICS, 2010, 519

[9] RECORD-SETTING COSMIC-RAY INTENSITIES IN 2009 AND 2010 [J].

Mewaldt, R. A. ;

Davis, A. J. ;

Lave, K. A. ;

Leske, R. A. ;

Stone, E. C. ;

Wiedenbeck, M. E. ;

Binns, W. R. ;

Christian, E. R. ;

Cummings, A. C. ;

de Nolfo, G. A. ;

Israel, M. H. ;

Labrador, A. W. ;

von Rosenvinge, T. T. .

ASTROPHYSICAL JOURNAL LETTERS, 2010, 723 (01) :L1-L6

[10] The ESA standard radiation environment monitor program first results from PROBA-I and INTEGRAL [J].

Mohammadzadeh, A ;

Evans, H ;

Nieminen, P ;

Daly, E ;

Vuilleumier, P ;

Bühler, P ;

Eggel, C ;

Hajdas, W ;

Schlumpf, N ;

Zehnder, A ;

Schneider, J ;

Fear, R .

IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 2003, 50 (06) :2272-2277

← 1 2 →