The 2‐D Structure of Foreshock‐Driven Field Line Resonances Observed by THEMIS Satellite and Ground‐Based Imager Conjunctions-Reference-Cited by-同舟云学术

The 2‐D Structure of Foreshock‐Driven Field Line Resonances Observed by THEMIS Satellite and Ground‐Based Imager Conjunctions

Published:2019-08 Issue:8 Volume:124 Page:6792-6811
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Wang Boyi¹^ORCID,Nishimura Yukitoshi²^ORCID,Zhang Hui³^ORCID,Shen Xiao‐Chen¹,Lyons Larry⁴^ORCID,Angelopoulos Vassilis⁵,Ebihara Yusuke⁶^ORCID,Weatherwax Allan⁷,Gerrard Andrew J.⁸^ORCID,Frey Harald U.⁹^ORCID

Affiliation:

1. Department of Astronomy and Center for Space Sciences Boston University Boston MA USA

2. Department of Electrical and Computer Engineering and Center for Space Sciences Boston University Boston MA USA

3. Geophysical Institute University of Alaska Fairbanks Fairbanks AK USA

4. Department of Atmospheric and Oceanic Sciences University of California Los Angeles CA USA

5. Department of Earth, Planetary and Space Sciences University of California Los Angeles CA USA

6. Research Institute for Sustainable Humanosphere Kyoto University Kyoto Japan

7. School of Science and Engineering Merrimack College North Andover MA USA

8. Department of Physics Center for Solar‐Terrestrial Research New Jersey Institute of Technology Newark NJ USA

9. Space Sciences Laboratory University of California Berkeley CA USA

Funder

Air Force Office of Scientific Research

National Aeronautics and Space Administration

National Science Foundation

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA026668

Reference97 articles.

1. Spatial and temporal structure of a high-latitude transient ULF pulsation

2. The THEMIS Mission

3. The Space Physics Environment Data Analysis System (SPEDAS)

4. Foreshock cavitons for different interplanetary magnetic field geometries: Simulations and observations

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