Far Ultraviolet Imaging from the Image Spacecraft

By S. Mende, H. Heetderks, H. Frey, M. Lampton, S. Geller, J. Stock, R. Abiad, O. Siegmund, A. Tremsin, S. Habraken. 2000

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Relationship between interplanetary parameters and the magnetopause reconnection rate quantified from observations of the expanding polar cap (2012, methodology): “Figure 1, modified from Milan [2009], shows the relationship between the open/closed topology of the magnetosphere and the mapping of open field lines into the polar ionospheres to form the polar caps, the dim regions encircled by the auroral ovals.”
The THEMIS Array of Ground-based Observatories for the Study of Auroral Substorms (2008, background): “Thus many authors successfully pursued space-based substorm studies by using the ultraviolet imagers on POLAR (Torr et al. 1995) and IMAGE (Mende et al. 2000) (Fig.”
Localized aurora beyond the auroral oval (2007, methodology): “IMAGE carries two separate instruments of the Far Ultraviolet (FUV) imaging system: the Wideband Imaging Camera (WIC) with a passband of 140–180 nm and the Spectrographic Imager with the proton aurora and the 135.6 nm oxygen line channels [Mende et al., 2000].”