Saturn's Weather‐Driven Aurorae Modulate Oscillations in the Magnetic Field and Radio Emissions-Reference-Cited by-同舟云学术

Saturn's Weather‐Driven Aurorae Modulate Oscillations in the Magnetic Field and Radio Emissions

Published:2022-02-07 Issue:3 Volume:49 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Chowdhury M. N.¹^ORCID,Stallard T. S.¹^ORCID,Baines K. H.²³^ORCID,Provan G.¹^ORCID,Melin H.¹^ORCID,Hunt G. J.⁴^ORCID,Moore L.⁵^ORCID,O’Donoghue J.⁶^ORCID,Thomas E. M.¹^ORCID,Wang R.¹^ORCID,Miller S.⁷,Badman S. V.⁸^ORCID

Affiliation:

1. School of Physics and Astronomy University of Leicester Leicester UK

2. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

3. Space Science and Engineering Center University of Wisconsin‐Madison Madison WI USA

4. Blackett Laboratory Imperial College London London UK

5. Center for Space Physics Boston University Boston MA USA

6. Institute for Space and Astronautical Science JAXA Kanagawa Japan

7. Department of Physics and Astronomy University College London London UK

8. Department of Physics Lancaster University Lancaster UK

Funder

Science and Technology Facilities Council

National Aeronautics and Space Administration

NASA Exoplanet Science Institute

Humanities Montana

Office of Legacy Management

Japan Aerospace Exploration Agency

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021GL096492

Reference41 articles.

1. Constraining the Temporal Variability of Neutral Winds in Saturn's Low‐Latitude Ionosphere Using Magnetic Field Measurements

2. Rotational modulation and local time dependence of Saturn’s infrared auroral intensity;Badman S. V.;Journal of Geophysical Research: Space Physics,2012

3. Cassini VIMS observations of latitudinal and hemispheric variations in Saturn’s infrared auroral intensity

4. On the cause of Saturn's plasma periodicity

5. Spin-period effects in magnetospheres with no axial tilt

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