Reflection and Refraction of the L‐O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath-Reference-Cited by-同舟云学术

Reflection and Refraction of the L‐O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath

Author:

Wu S. Y.¹^ORCID,Ye S. Y.¹^ORCID,Fischer G.²^ORCID,Jackman C. M.³^ORCID,Wang J.¹^ORCID,Menietti J. D.⁴^ORCID,Cecconi B.⁵^ORCID,Long M. Y.⁶^ORCID

Affiliation:

1. Department of Earth and Space Sciences Southern University of Science and Technology Shenzhen People's Republic of China

2. Space Research Institute Austrian Academy of Sciences Graz Austria

3. School of Cosmic Physics Dublin Institute for Advanced Studies Dublin Ireland

4. Department of Physics and Astronomy University of Iowa Iowa City IA USA

5. LESIA, Observatoire de Paris Université PSL CNRS Sorbonne Université Université de Paris Meudon Paris France

6. Department of Space Physics School of Electronic Information Wuhan University Wuhan People's Republic of China

Funder

Chinese Academy of Sciences

Austrian Science Fund

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

Reference35 articles.

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