Bursty Bulk Flow Turbulence as a Source of Energetic Particles to the Outer Radiation Belt-Reference-Cited by-同舟云学术

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Bursty Bulk Flow Turbulence as a Source of Energetic Particles to the Outer Radiation Belt

Published:2022-06-06 Issue:11 Volume:49 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Ergun R. E.¹²^ORCID,Usanova M. E.²^ORCID,Turner D. L.³^ORCID,Stawarz J. E.⁴^ORCID

Affiliation:

1. Department of Astrophysical and Planetary Sciences University of Colorado Boulder CO USA

2. Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA

3. Johns Hopkins University Applied Physics Laboratory Laurel MD USA

4. The Blackett Laboratory Imperial College London London UK

Funder

Science Mission Directorate

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022GL098113

Reference42 articles.

1. Bursty bulk flows in the inner central plasma sheet

2. Statistical characteristics of bursty bulk flow events

3. Average plasma properties in the central plasma sheet

4. Characteristic plasma properties during dispersionless substorm injections at geosynchronous orbit

5. Magnetospheric Multiscale Overview and Science Objectives

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2. Turbulent Magnetic Reconnection as an Acceleration Mechanism in Earth’s Magnetotail;The Astrophysical Journal;2024-04-01

3. Fluctuations of the Electric and Magnetic Fields in the Plasma Sheet of the Earth’s Magnetotail According to MMS Data;Cosmic Research;2024-02

4. Particle Acceleration by Magnetic Reconnection in Geospace;Space Science Reviews;2023-11-07

5. Mesoscale Structure and Properties of the Terrestrial Magnetotail Plasma Sheet From the Magnetospheric Multiscale Mission;Journal of Geophysical Research: Space Physics;2023-09

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