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Observations of Forbush Decreases of Cosmic-Ray Electrons and Positrons with the Dark Matter Particle Explorer

文献类型：期刊论文

作者Alemanno, Francesca15,16; An, Qi17,19; Azzarello, Philipp20; Barbato, Felicia Carla Tiziana15,16; Bernardini, Paolo3,18,22; Bi, XiaoJun4,5; Cai, MingSheng6,7; Casilli, Elisabetta3,18,22; Catanzani, Enrico8; Chang, Jin6,7
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2021-10-01
卷号920期号:2页码:10
关键词Solar coronal mass ejections Forbush effect Cosmic rays
ISSN号2041-8205
DOI10.3847/2041-8213/ac2de6
通讯作者Zang, JingJing(zangjingjing@lyu.edu.cn)
英文摘要The Forbush decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections or high-speed streams from coronal holes. It has been mainly explored with the ground-based neutron monitor network, which indirectly measures the integrated intensities of all species of cosmic rays by counting secondary neutrons produced from interaction between atmospheric atoms and cosmic rays. The space-based experiments can resolve the species of particles but the energy ranges are limited by the relatively small acceptances except for the most abundant particles like protons and helium. Therefore, the FD of cosmic-ray electrons and positrons have just been investigated by the PAMELA experiment in the low-energy range (<5 GeV) with limited statistics. In this paper, we study the FD event that occurred in 2017 September with the electron and positron data recorded by the Dark Matter Particle Explorer. The evolution of the FDs from 2 GeV to 20 GeV with a time resolution of 6 hr are given. We observe two solar energetic particle events in the time profile of the intensity of cosmic rays, the earlier, and weaker, one has not been shown in the neutron monitor data. Furthermore, both the amplitude and recovery time of fluxes of electrons and positrons show clear energy dependence, which is important in probing the disturbances of the interplanetary environment by the coronal mass ejections.
WOS关键词PLASTIC SCINTILLATOR DETECTOR ; SOLAR ; MODULATION ; DRIFT ; ENERGY ; DISTURBANCES ; CALIBRATION ; DEPENDENCE ; INTENSITY ; TRANSPORT
资助项目strategic priority science and technology projects in space science of the Chinese Academy of Sciences ; National Key Research and Development Program of China[2016YFA0400200] ; National Natural Science Foundation of China[11773085] ; National Natural Science Foundation of China[U1738207] ; National Natural Science Foundation of China[11722328] ; National Natural Science Foundation of China[41774185] ; National Natural Science Foundation of China[U1738205] ; National Natural Science Foundation of China[U1738128] ; National Natural Science Foundation of China[11851305] ; National Natural Science Foundation of China[11873021] ; National Natural Science Foundation of China[U1631242] ; strategic priority science and technology projects of the Chinese Academy of Sciences[XDA15051100] ; 100 Talents Program of the Chinese Academy of Sciences ; Young Elite Scientists Sponsorship Program by CAST[YESS20160196] ; Program for Innovative Talents and Entrepreneur in Jiangsu ; Swiss National Science Foundation (SNSF), Switzerland ; National Institute for Nuclear Physics (INFN), Italy
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000709975200001
出版者IOP Publishing Ltd
资助机构strategic priority science and technology projects in space science of the Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Natural Science Foundation of China ; strategic priority science and technology projects of the Chinese Academy of Sciences ; 100 Talents Program of the Chinese Academy of Sciences ; Young Elite Scientists Sponsorship Program by CAST ; Program for Innovative Talents and Entrepreneur in Jiangsu ; Swiss National Science Foundation (SNSF), Switzerland ; National Institute for Nuclear Physics (INFN), Italy
源URL[http://119.78.100.186/handle/113462/136044]  
专题中国科学院近代物理研究所
通讯作者Zang, JingJing
作者单位1.Politecn Bari, Via Amendola 173, I-70126 Bari, Italy
2.Univ Hong Kong, Dept Phys, Pok Fu Lam, Hong Kong, Peoples R China
3.Ist Nazl Fis Nucl INFN, Sez Lecce, I-73100 Lecce, Italy
4.Univ Chinese Acad Sci, Yuquan Rd 19A, Beijing 100049, Peoples R China
5.Chinese Acad Sci, Inst High Energy Phys, Particle Astrophys Div, Beijing 100049, Peoples R China
6.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210023, Peoples R China
7.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
8.Ist Nazl Fis Nucl INFN, Sez Perugia, I-106123 Perugia, Italy
9.Chinese Acad Sci, Natl Space Sci Ctr, Nanertiao 1, Beijing 100190, Peoples R China
10.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
推荐引用方式
GB/T 7714		 Alemanno, Francesca,An, Qi,Azzarello, Philipp,et al. Observations of Forbush Decreases of Cosmic-Ray Electrons and Positrons with the Dark Matter Particle Explorer[J]. ASTROPHYSICAL JOURNAL LETTERS,2021,920(2):10.
APA Alemanno, Francesca.,An, Qi.,Azzarello, Philipp.,Barbato, Felicia Carla Tiziana.,Bernardini, Paolo.,...&Zhu, ChengRui.(2021).Observations of Forbush Decreases of Cosmic-Ray Electrons and Positrons with the Dark Matter Particle Explorer.ASTROPHYSICAL JOURNAL LETTERS,920(2),10.
MLA Alemanno, Francesca,et al."Observations of Forbush Decreases of Cosmic-Ray Electrons and Positrons with the Dark Matter Particle Explorer".ASTROPHYSICAL JOURNAL LETTERS 920.2(2021):10.

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来源：近代物理研究所

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