First Fermi-LAT Solar Flare Catalog

被引：40

作者：

Ajello, M. ^{[1
]}

Baldini, L. ^{[2
,3
]}

Bastieri, D. ^{[4
,5
]}

Bellazzini, R. ^{[3
]}

Berretta, A. ^{[6
]}

Bissaldi, E. ^{[7
,8
]}

Blandford, R. D. ^{[9
,10
]}

Bonino, R. ^{[11
,12
]}

Bruel, P. ^{[13
]}

Buson, S. ^{[14
]}

Cameron, R. A. ^{[9
,10
]}

Caputo, R. ^{[15
]}

Cavazzuti, E. ^{[16
]}

Cheung, C. C. ^{[17
]}

Chiaro, G. ^{[18
]}

Costantin, D. ^{[19
]}

Cutini, S. ^{[20
]}

D'Ammando, F. ^{[21
]}

de Palma, F. ^{[11
]}

Desiante, R. ^{[11
]}

Di Lalla, N. ^{[9
,10
]}

Di Venere, L. ^{[7
,8
]}

Dirirsa, F. Fana ^{[22
]}

Fegan, S. J. ^{[13
]}

Fukazawa, Y. ^{[23
]}

Funk, S. ^{[24
]}

Fusco, P. ^{[7
,8
]}

Gargano, F. ^{[8
]}

Gasparrini, D. ^{[25
,26
]}

Giordano, F. ^{[7
,8
]}

Giroletti, M. ^{[21
]}

Green, D. ^{[27
]}

Guiriec, S. ^{[15
,28
]}

Hays, E. ^{[15
]}

Hewitt, J. W. ^{[29
]}

Horan, D. ^{[13
]}

Johannesson, G. ^{[30
,31
,32
]}

Kovac'evic', M. ^{[20
]}

Kuss, M. ^{[3
]}

Larsson, S. ^{[33
,34
,35
]}

Latronico, L. ^{[11
]}

Li, J. ^{[36
]}

Longo, F. ^{[37
,38
]}

Lovellette, M. N. ^{[17
]}

Lubrano, P. ^{[20
]}

Maldera, S. ^{[11
]}

Manfreda, A. ^{[2
,3
]}

Marti-Devesa, G. ^{[39
]}

Mazziotta, M. N. ^{[8
]}

Mereu, I. ^{[6
,20
]}

机构：

[1] Clemson Univ, Kinard Lab Phys, Dept Phys & Astron, Clemson, SC 29634 USA

[2] Univ Pisa, I-56127 Pisa, Italy

[3] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[4] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[5] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy

[6] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy

[7] Univ Politecn Bari, Dipartimento Fis M Merlin, Via Amendola 173, I-70126 Bari, Italy

[8] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[9] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, WW Hansen Expt Phys Lab, Dept Phys, Stanford, CA 94305 USA

[10] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA

[11] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

[12] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy

[13] Ecole Polytech, Lab Leprince Ringuet, CNRS IN2P3, F-91128 Palaiseau, France

[14] Univ Wurzburg, Inst Theoret Phys & Astrophys, Campus Hubland Nord,Emil Fischer Str 31, D-97074 Wurzburg, Germany

[15] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[16] Italian Space Agcy, Via Politecn Snc, I-00133 Rome, Italy

[17] Naval Res Lab, Div Space Sci, Washington, DC 20375 USA

[18] INAF Ist Astrofis Spaziale & Fis Cosmica Milano, Via E Bassini 15, I-20133 Milan, Italy

[19] Univ Padua, Dept Stat Sci, Via 8 Febbraio,2, I-35122 Padua, Italy

[20] Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy

[21] INAF Ist Radioastron, I-40129 Bologna, Italy

[22] Univ Johannesburg, Dept Phys, POB 524, ZA-2006 Auckland Pk, South Africa

[23] Hiroshima Univ, Dept Phys Sci, Higashihiroshima, Hiroshima 7398526, Japan

[24] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany

[25] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy

[26] Agenzia Spaziale Italiana, Space Sci Data Ctr, Via Politecn,Snc, I-00133 Rome, Italy

[27] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[28] George Washington Univ, Dept Phys, 725 21st St NW, Washington, DC 20052 USA

[29] Univ North Florida, Dept Phys, 1 UNF Dr, Jacksonville, FL 32224 USA

[30] Univ Iceland, Inst Sci, IS-107 Reykjavik, Iceland

[31] Royal Inst Technol, NORDITA, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden

[32] Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden

[33] KTH Royal Inst Technol, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden

[34] Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden

[35] Dalarna Univ, Nat Sci, Sch Educ Hlth & Social Studies, SE-79188 Falun, Sweden

[36] Deutsch Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany

[37] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy

[38] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy

[39] Leopold Franzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria

[40] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Higashihiroshima, Hiroshima 7398526, Japan

[41] Ctr Res & Explorat Space Sci & Technol, Greenbelt, MD 20771 USA

[42] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[43] Univ Maryland Baltimore Cty, Dept Phys, Baltimore, MD 21250 USA

[44] Univ Maryland Baltimore Cty, Ctr Space Sci & Technol, Baltimore, MD 21250 USA

[45] Univ Trieste, Trieste, Italy

[46] Ist Nazl Astrofis, Osservatorio Astron Trieste, I-34143 Trieste, Italy

[47] Univ Montpellier, Lab Univers & Particules Montpellier, CNRS IN2P3, F-34095 Montpellier, France

[48] Univ Padua, Dept Phys & Astron, Vicolo Osservatorio 3, I-35122 Padua, Italy

[49] Univ Padua, Ctr Space Studies & Activ G Colombo, Via Venezia 15, I-35131 Padua, Italy

[50] Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 30455, South Korea

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2021年 / 252卷 / 02期

基金：

瑞典研究理事会; 美国国家航空航天局;

关键词：

Solar flares; Solar gamma-ray emission; Gamma-ray sources; Gamma-ray telescopes; Catalogs; HARD X-RAY; GAMMA-RAY; RHESSI OBSERVATIONS; EGRET; ACCELERATION; EMISSION; COMPTON; NEUTRON; TELESCOPE; PARTICLES;

D O I：

10.3847/1538-4365/abd32e

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first Fermi-Large Area Telescope (LAT) solar flare catalog covering the 24th solar cycle. This catalog contains 45 Fermi-LAT solar flares (FLSFs) with emission in the gamma-ray energy band (30 MeV-10 GeV) detected with a significance of >= 5 sigma over the years 2010-2018. A subsample containing 37 of these flares exhibits delayed emission beyond the prompt-impulsive hard X-ray phase, with 21 flares showing delayed emission lasting more than two hours. No prompt-impulsive emission is detected in four of these flares. We also present in this catalog observations of GeV emission from three flares originating from active regions located behind the limb of the visible solar disk. We report the lightcurves, spectra, best proton index, and localization (when possible) for all FLSFs. The gamma-ray spectra are consistent with the decay of pions produced by >300 MeV protons. This work contains the largest sample of high-energy gamma-ray flares ever reported and provides a unique opportunity to perform population studies on the different phases of the flare and thus allowing a new window in solar physics to be opened.

引用

页数：31

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