Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere

By B. Sandel, J. Goldstein, Dennis L. Gallagher, M. Spasojević. 2003

211 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/03fdca9d9929cc3fa68236ab5c934e70865077eb

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In Astronomy and Astrophysics

1. R. Thorne
2. Nigel P. Meredith
3. Binbin Ni
4. R. Horne
5. Danny Summers
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In Nuclear and High Energy Physics

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Citations in the corpus

• Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, methodology): “Figure 25 gives an example of such channel development on 10 June 2001 in the pre-midnight sector, when a plume wrapped around the main body of the plasmasphere (Sandel et al. 2003).”
• Global response of the plasmasphere to a geomagnetic disturbance (2003, background): “…this bulge is indicated as the local time between the open square and open right-facing triangle in Figure 3a. [22] EUV commonly observes variations in the plasmapause radius with local time on the order of 1–2 RE during quiet periods that can persist for as long as 60 hours [Sandel et al., 2003].”
• 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].”
• Simultaneous remote sensing and in situ observations of plasmaspheric drainage plumes (2004, background): “The existing EUV database contains many examples of plumes during and/or after geomagnetic disturbance times [Burch et al., 2001a, 2001b; Foster et al., 2002; Goldstein et al., 2002, 2003a, 2003c, 2003b; Sandel et al., 2004; Moldwin et al., 2004; Spasojević et al., 2003, 2004].”
• Localized aurora beyond the auroral oval (2007, background): “This value is consistent with the observed range of 70–90% plasmasphere corotation [Sandel et al., 2003; Adrian et al., 2004].”
• The Plasmasphere Boundary Layer (2004, methodology): “Furthermore, in the global scale plasmasphere observations from IMAGE there is much that is not predicted by the simple MHD theory (e.g. Spasojević, 2003; Sandel et al., 2003; Goldstein et al., 2004).”