Control of plasmaspheric dynamics by both convection and sub‐auroral polarization stream

By J. Goldstein, B. Sandel, M. Hairston, P. Reiff. 2003

141 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/7db6cc6a68e8c95891b8dde0a45870821e2f823e

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In Astronomy and Astrophysics

1. R. Thorne
2. Nigel P. Meredith
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4. R. Horne
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Citations in the corpus

• Simultaneous remote sensing and in situ observations of plasmaspheric drainage plumes (2004, methodology): “The average EUV lower threshold is known (in terms of total electron density) to be 40 e cm 3 [Goldstein et al., 2003c].”
• Electron scattering by whistler-mode ELF hiss in (2008, background): “…of evolving plasmaspheric plumes have been provided by the extreme ultraviolet (EUV) imager of the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) satellite [e.g., Sandel et al., 2003; Goldstein et al., 2003, 2004, 2005; Spasojeviç et al., 2003, 2004; Burch, 2006; Goldstein, 2006].”