Initial results from the IMAGE Extreme Ultraviolet Imager

By B. Sandel, R. King, W. T. Forrester, Dennis L. Gallagher, A. Broadfoot, C. Curtis. 2001

195 citations recorded by the source corpus.

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In Astronomy and Astrophysics

Citations in the corpus

The Plasmasphere Boundary Layer (2004, methodology): “One is the operation since May 2000 of the EUV instrument on the IMAGE satellite, which is providing for the first time global images of the plasmasphere (Sandel et al., 2001, 2003).”
Simultaneous remote sensing and in situ observations of plasmaspheric drainage plumes (2004, background): “[3] Global plasmasphere imaging by the IMAGE satellite extreme ultraviolet (EUV) imager [Burch, 2000] has proved the existence of plasmaspheric plumes [Sandel et al., 2001].”
Control of plasmaspheric dynamics by both convection and sub‐auroral polarization stream (2003, background): “[4] The IMAGE satellite extreme ultraviolet (EUV) imager [Sandel et al., 2001] obtains full global plasmasphere images by detecting 30.4 nm light resonantly scattered by plasmaspheric He+ ions.”
Identifying the plasmapause in IMAGE EUV data using IMAGE RPI in situ steep density gradients (2003, methodology): “[5] The Extreme Ultraviolet (EUV) instrument on the IMAGE satellite [Burch, 2000] is the first instrument to provide full global images of the plasmasphere on a routine basis [Sandel et al., 2000, 2001].”
A new model of the location of the plasmapause: CRRES results (2002, background): “[24] Recent IMAGE EUV images show that the EUV plasmapause often shows a duskside bulge and drainage plume as well as surface ‘‘biteouts’’ and shoulders [Sandel et al., 2001].”
Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, background): “Those structures are now known as “plasmaspheric plumes” (e.g., Elphic et al. 1996; Ober et al. 1997; Sandel et al. 2001).”
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].”
Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere (2003, methodology): “The EUV instrument images the distribution of cold He+ in Earth’s plasmasphere with a time resolution of 10 minutes and a spatial resolution of 0.1 RE (at apogee) or better (Sandel et al., 2001).”
A quantitative explanation for the phenomenon known as storm‐enhanced density (2004, background): “From a UV imager viewpoint, the structure appears to peal off the plasmasphere and become entrained sunward [Sandel et al., 2001].”
Kinetic simulations of ring current evolution during the Geospace Environment Modeling challenge events (2006, background): “The Extreme Ultraviolet (EUV) imager [Sandel et al., 2001] obtains images of the plasmasphere with a lower sensitivity threshold equivalent to total ion density of 40 cm 3.”