Kelvin–Helmholtz‐Related Turbulent Heating at Saturn's Magnetopause Boundary-Reference-Cited by-同舟云学术

Kelvin–Helmholtz‐Related Turbulent Heating at Saturn's Magnetopause Boundary

Published:2021-02 Issue:2 Volume:126 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Delamere P. A.¹^ORCID,Ng C. S.¹^ORCID,Damiano P. A.¹^ORCID,Neupane B. R.¹^ORCID,Johnson J. R.²^ORCID,Burkholder B.³^ORCID,Ma X.³^ORCID,Nykyri K.³^ORCID

Affiliation:

1. Geophysical Institute University of Alaska Fairbanks Fairbanks AK USA

2. Andrews University Berrien Springs MI USA

3. Department of Physical Sciences and Center for Space and Atmospheric Research Embry‐Riddle Aeronautical University Daytona Beach FL USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028479

Reference55 articles.

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2. Flow of mass and energy in the magnetospheres of Jupiter and Saturn

3. Plasma Physics via Computer Simulation

4. Identifying Active Kelvin–Helmholtz Vortices on Saturn's Magnetopause Boundary

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