Variability of Jupiter's IR H 3 + aurorae during Juno approach-Reference-Cited by-同舟云学术

Variability of Jupiter's IR H 3 + aurorae during Juno approach

Published:2017-05-25 Issue:10 Volume:44 Page:4513-4522
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Moore L.¹^ORCID,O'Donoghue J.²^ORCID,Melin H.³^ORCID,Stallard T.³^ORCID,Tao C.⁴^ORCID,Zieger B.¹,Clarke J.¹^ORCID,Vogt M. F.¹^ORCID,Bhakyapaibul T.¹,Opher M.¹,Tóth G.⁵,Connerney J. E. P.²^ORCID,Levin S.⁶^ORCID,Bolton S.⁷^ORCID

Affiliation:

1. Center for Space Physics Boston University Boston Massachusetts USA

2. NASA Goddard Space Flight Center Greenbelt Maryland USA

3. Department of Physics and Astronomy University of Leicester Leicester UK

4. National Institute of Information and Communications Technology Tokyo Japan

5. Center for Space Environment Modeling University of Michigan Ann Arbor Michigan USA

6. Jet Propulsion Laboratory Pasadena California USA

7. Southwest Research Institute San Antonio Texas USA

Funder

National Aeronautics and Space Administration

Science and Technology Facilities Council

National Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017GL073156

Reference49 articles.

1. JIM: A time-dependent, three-dimensional model of Jupiter's thermosphere and ionosphere

2. Weakening of Jupiter's main auroral emission during January 2014

3. Solar Wind Control of Jupiter's H+3Auroras

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