Magnetospheric and exospheric imaging in the extreme ultraviolet

Details Magnetospheric and exospheric imaging in the extreme ultraviolet Magnetospheric and exospheric imaging in the extreme ultraviolet

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17..267c&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, March 1990, p. 267-270. Research supported by the Lockheed Missiles and

Physics

13

Exosphere, Extreme Ultraviolet Radiation, Image Processing, Magnetosphere-Ionosphere Coupling, Magnetospheric Ion Density, Charge Exchange, Computerized Simulation, Line Spectra, Oxygen Spectra

Scientific paper

Extreme ultraviolet line emissions by exospheric oxygen ions and neutrals of ionospheric origin can be used to form images of the dynamic magnetospheric regions with sufficient speed to provide a new global means of observing the dynamics of magnetosphere-ionosphere coupling processes. Computer simulations of such exospheric images based on the latest measurements of ion outflow, on known or estimated solar fluxes, and on known emission and excitation rates are shown. An evaluation of the current and foreseeable EUV imaging technology relevant to magnetospheric imaging is also given.

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