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Local Generation of High-Frequency Plasmaspheric Hiss Observed by Van Allen Probes

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成果类型:
期刊论文
作者:
He, Zhaoguo*;Chen, Lunjin*;Liu, Xu;Zhu, Hui;Liu, Si;...
通讯作者:
He, Zhaoguo;Chen, Lunjin
作者机构:
[He, Zhaoguo] Sun Yat Sen Univ, Sch Atmospher Sci, Zhuhai, Peoples R China.
[He, Zhaoguo] Univ Sci & Technol China, Chinese Acad Sci, Key Lab Geospace Environm, Hefei, Anhui, Peoples R China.
[He, Zhaoguo] CAS Ctr Excellence Comparat Planetol, Hefei, Anhui, Peoples R China.
[He, ZG; Chen, Lunjin; Liu, Xu; Zhu, Hui; Liu, Si; He, Zhaoguo] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Gao, Zhonglei; Liu, Si] Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha, Hunan, Peoples R China.
通讯机构:
[He, Zhaoguo] S
[He, Zhaoguo; He, ZG; Chen, LJ] U
[He, Zhaoguo] C
Sun Yat Sen Univ, Sch Atmospher Sci, Zhuhai, Peoples R China.
Univ Sci & Technol China, Chinese Acad Sci, Key Lab Geospace Environm, Hefei, Anhui, Peoples R China.
语种:
英文
关键词:
plasmaspheric hiss;high frequency;local generation;substorm injection;electron
期刊:
GEOPHYSICAL RESEARCH LETTERS
ISSN:
0094-8276
年:
2019
卷:
46
期:
3
页码:
1141-1148
基金类别:
The HOPE and EMFISIS data are available at the websites (https://cdaweb.gsfc.nasa.gov/istp_public/; http://emfisis.physics.uiowa.edu/Flight/). This work was supported by National Natural Science Foundation of China grant 41704160, Natural Science Foundation of Guangdong Province (2016A030310366) and Shenzhen Technology projects (JCYJ20160226201347750 and ZDSYS201707280904031). Works at UTD are supported by NSF grant 1705079 through the Geospace Environment Modeling Program and the AFOSR grant FA9550-16-1-0344.
机构署名:
本校为其他机构
院系归属:
物理与电子科学学院
摘要:
The generation of a high-frequency plasmaspheric hiss (HFPH) wave observed by Van Allen Probes is studied in this letter for the first time. The wave has a moderate power spectral density (similar to 10(-6) nT(2)/Hz), with a frequency range extended from 2 to 10 kHz. The correlated observations of waves and particles indicate that HFPH is associated with the enhancement of electron flux during the substorm on 6 January 2014. Calculations of the wave linear growth rate driven by the fitted electron phase space density show that the electron distribution after the substorm onset is efficient for...

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