Transport and chemical loss rates in Saturn's inner plasma disk
Author:
Affiliation:
1. Swedish Institute of Space Physics; Uppsala Sweden
2. Department of Physics and Astronomy; Uppsala University; Uppsala Sweden
3. Laboratory for Atmospheric and Space Physics University of Colorado; Boulder Colorado USA
Funder
Swedish National Space Board
Swedish Research Council
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Reference47 articles.
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2. A noon-to-midnight electric field and nightside dynamics in Saturn's inner magnetosphere, using microsignature observations;Andriopoulou;Icarus,2012
3. Plasma electrons in Saturn's magnetotail: Structure, distribution and energisation;Arridge;Planet. Space Sci.,2009
4. Collisional spreading of Enceladus neutral cloud;Cassidy;Icarus,2010
5. Rate of radial transport of plasma in Saturn's inner magnetosphere;Chen;J. Geophys. Res.,2010
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1. Predictive model linking super-rotation, magnetospheric generation and atmospheric heating;Open Astronomy;2020-12-31
2. Density Structures, Dynamics, and Seasonal and Solar Cycle Modulations of Saturn's Inner Plasma Disk;Journal of Geophysical Research: Space Physics;2017-12
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