The Extreme Ultraviolet Imager Investigation for the IMAGE Mission

By B. Sandel, A. Broadfoot, C. Curtis, R. King, Thomas C. Stone, R. Hill, J. Chen, O. Siegmund, R. Raffanti, D. Allred and 2 more. 2000

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Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere (2003, background): “The cameras’ fields of view are offset relative to one another (Sandel et al., 2000).”
Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, methodology): “IMAGE has made remote, global observations with the Extreme UltraViolet (EUV) instrument (Sandel et al. 2000) and the Radio Plasma Imager (RPI) instrument (Reinisch et al. 2000), from points both outside and within the plasmasphere (e.g., Carpenter et al. 2002; Sandel et al. 2003).”
Cluster observations of EMIC triggered emissions in association with Pc1 waves near Earth's plasmapause (2010, background): “It did, however, get to high enough latitude in the Northern Hemisphere about 2 hours later at 09:57:41 UT and obtained an Extreme Ultraviolet Imager (EUV) snapshot of the plasmasphere [Sandel et al., 2000].”
Initial results from the IMAGE Extreme Ultraviolet Imager (2001, methodology): “The IMAGE EUV instrument is a set of three wide-field (30◦) cameras [Sandel et al., 2000] that are tuned for the 30.4-nm resonance line of He+.”
Global response of the plasmasphere to a geomagnetic disturbance (2003, background): “Lemaire [2001] proposes that in conjunction with enhanced magnetospheric convection, convective instabilities and interchange motion in the postmidnight local time sector contribute to the formation of a new boundary.”