Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1029/2018GL077699 |
What Causes Radiation Belt Enhancements: A Survey of the Van Allen Probes Era | |
Boyd, A. J.1; Turner, D. L.2; Reeves, G. D.1,3; Spence, H. E.4; Baker, D. N.5; Blake, J. B.2 | |
2018-06-16 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
![]() |
ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2018 |
卷号 | 45期号:11页码:5253-5259 |
文章类型 | Article |
语种 | 英语 |
国家 | USA |
英文摘要 | We survey radiation belt enhancement events during the Van Allen Probes era to determine what mechanism is the dominant cause of enhancements and where it is most effective. Two primary mechanisms have been proposed: (1) betatron/Fermi acceleration due to the Earthward radial transport of electrons, which produces monotonic gradients in phase space density (PSD), and (2) "local acceleration" due to gyro/Landau resonant interaction with electromagnetic waves, which produces radially localized growing peaks in PSD. To differentiate between these processes, we examine radial profiles of PSD in adiabatic coordinates using data from the Van Allen Probes and Time History of Events and Macroscale Interactions during Substorms satellites for 80 outer belt enhancement events from October 2012 to April 2017 This study shows that local acceleration is the dominant acceleration mechanism for MeV electrons in the outer belt, with 87% of the enhancement events exhibiting growing peaks. The strong correlation of the location of these with geomagnetic activity further supports this conclusion. |
英文关键词 | Radiation Belt Phase Space Density Local Acceleration Van Allen Probes THEMIS |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000436249900003 |
WOS关键词 | HIGHLY RELATIVISTIC ELECTRONS ; PHASE-SPACE DENSITY ; GEOMAGNETIC STORMS ; SEED POPULATION ; ACCELERATION ; WAVES ; MAGNETOSPHERE ; ENERGIZATION ; MECHANISMS ; DIFFUSION |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/27490 |
专题 | 气候变化 |
作者单位 | 1.New Mexico Consortium, Los Alamos, NM 87544 USA; 2.Aerosp Corp, El Segundo, CA 90245 USA; 3.Los Alamos Natl Lab, Los Alamos, NM USA; 4.Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA; 5.Univ Colorado, Lab Atmospher & Space Sci, Boulder, CO 80309 USA |
推荐引用方式 GB/T 7714 | Boyd, A. J.,Turner, D. L.,Reeves, G. D.,et al. What Causes Radiation Belt Enhancements: A Survey of the Van Allen Probes Era[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(11):5253-5259. |
APA | Boyd, A. J.,Turner, D. L.,Reeves, G. D.,Spence, H. E.,Baker, D. N.,&Blake, J. B..(2018).What Causes Radiation Belt Enhancements: A Survey of the Van Allen Probes Era.GEOPHYSICAL RESEARCH LETTERS,45(11),5253-5259. |
MLA | Boyd, A. J.,et al."What Causes Radiation Belt Enhancements: A Survey of the Van Allen Probes Era".GEOPHYSICAL RESEARCH LETTERS 45.11(2018):5253-5259. |
条目包含的文件 | 条目无相关文件。 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论