Cassini observations of ionospheric plasma in Saturn's magnetotail lobes-Reference-Cited by-同舟云学术

Cassini observations of ionospheric plasma in Saturn's magnetotail lobes

Published:2016-01 Issue:1 Volume:121 Page:338-357
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Felici M.¹²³,Arridge C. S.³,Coates A. J.¹²,Badman S. V.³,Dougherty M. K.⁴,Jackman C. M.⁵,Kurth W. S.⁶,Melin H.⁷,Mitchell D. G.⁸,Reisenfeld D. B.⁹,Sergis N.¹¹⁰

Affiliation:

1. Mullard Space Science LaboratoryUniversity College London Dorking UK

2. Centre for Planetary Sciences at UCL/Birkbeck London UK

3. Department of PhysicsLancaster University Lancaster UK

4. Space and Atmospheric Physics Group, The Blackett LaboratoryImperial College London London UK

5. Department of Physics and AstronomyUniversity of Southampton Southampton UK

6. Department of Physics and AstronomyUniversity of Iowa Iowa City Iowa USA

7. Department of Physics and AstronomyUniversity of Leicester Leicester UK

8. The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA

9. Department of Physics and AstronomyUniversity of Montana Missoula Montana USA

10. Office for Space ResearchAcademy of Athens Athens Greece

Funder

Agenzia Spaziale Italiana

National Aeronautics and Space Administration

Jet Propulsion Laboratory

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021648

Reference92 articles.

1. EXOS D (Akebono) suprathermal mass spectrometer observations of the polar wind

2. Altitude profile of the polar wind velocity and its relationship to ionospheric conditions

3. Dynamics of the Saturnian inner magnetosphere: First inferences from the Cassini magnetometers about small-scale plasma transport in the magnetosphere

4. Magnetic signatures of plasma-depleted flux tubes in the Saturnian inner magnetosphere

5. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates

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