Dynamical consequences of two modes of centrifugal instability in Jupiter's outer magnetosphere

By M. Kivelson, D. Southwood. 2004

159 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8d43b3146f1e4537041aea863d47f53d79d88cbf

How researchers see this paper

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In Astronomy and Astrophysics

1. Fran Bagenal
2. P. Delamere

In Molecular Biology

1. Fran Bagenal
2. P. Delamere

Citations in the corpus

• Solar wind interaction with Jupiter's magnetosphere (2009, methodology): “Bagenal [2007] and arguments by Kivelson and Southwood [2005] that opening reconnection on the dayside plus closing reconnection within the tail (providing a coherent Dungey‐like convection) is not the dominant physical process mediating the Jupiter’s interaction with the solar wind.”
• Flow of mass and energy in the magnetospheres of Jupiter and Saturn (2011, background): “At some point either the coupling to the planet breaks down completely (Kivelson and Southwood [2005] suggest via ballooning mode instability) or the field”