Identification of Controlling Geomagnetic and Solar Wind Factors for Magnetospheric Chorus Intensity Using Feature Selection Techniques-Reference-Cited by-同舟云学术

Identification of Controlling Geomagnetic and Solar Wind Factors for Magnetospheric Chorus Intensity Using Feature Selection Techniques

Published:2021-12-29 Issue:1 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Guo Yingjie¹^ORCID,Ni Binbin¹²^ORCID,Fu Song¹^ORCID,Wang Dedong³^ORCID,Shprits Y. Y.³⁴⁵^ORCID,Zhelavskaya I. S.³⁴^ORCID,Feng Minghang¹,Guo Deyu¹^ORCID

Affiliation:

1. Department of Space Physics School of Electronic Information Wuhan University Wuhan China

2. Chinese Academy of Sciences Center for Excellence in Comparative Planetology Hefei China

3. Section 2.7 Space Physics and Space Weather GFZ German Research Centre for Geosciences Potsdam Germany

4. Institute of Physics and Astronomy University of Potsdam Potsdam Germany

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

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029926

Reference54 articles.

1. Synthetic Empirical Chorus Wave Model From Combined Van Allen Probes and Cluster Statistics

2. Nonlinear interaction of outer zone electrons with VLF waves

3. Multi‐Parameter Chorus and Plasmaspheric Hiss Wave Models

4. Observation of chorus waves by the Van Allen Probes: Dependence on solar wind parameters and scale size

5. CIMI simulations with newly developed multiparameter chorus and plasmaspheric hiss wave models

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