Calculations of soft auroral bremsstrahlung and K alpha line emission at satellite altitude

Details Calculations of soft auroral bremsstrahlung and K alpha line emission at satellite altitude Calculations of soft auroral bremsstrahlung and K alpha line emission at satellite altitude

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jatp...39..913l&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 39, Aug. 1977, p. 913-919.

Physics

Auroral Irradiation, Bremsstrahlung, High Altitude Environments, K Lines, X Ray Spectra, Auroral Zones, Computer Programs, Electronic Spectra, Emission Spectra, Prediction Analysis Techniques, Radiant Flux Density, Satellite Observation

Scientific paper

Satellite altitude (835 km) fluxes of 0.1-10 keV auroral X-rays are calculated for some typical forms of incident electron spectra. Both bremsstrahlung and K alpha line emission are included. These calculations indicate that K alpha emission can increase the observable intensity of satellite altitude auroral X-rays by up to 100 times, thereby making soft X-rays an ideal medium for producing images of the auroral morphology.

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