Rocket-borne EUV-visible emission measurements

Details Rocket-borne EUV-visible emission measurements Rocket-borne EUV-visible emission measurements

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jatp...47..147s&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 47, Jan.-Mar. 1985, p. 147-158. Research supported by the

Physics

7

Auroral Arcs, Auroral Spectroscopy, Extreme Ultraviolet Radiation, Rocket-Borne Instruments, Ultraviolet Photometry, Visual Photometry, Diffuse Radiation, Electron Precipitation, Emission Spectra, Energy Budgets, Radiant Flux Density, Upper Atmosphere, Vertical Distribution

Scientific paper

The results from auroral measurements with spectrometers and photometers are reported for three successful rocket flights with the spectra (50-640 nm) and height profiles presented. The ratios of 391.4/557.7 nm show characteristic differences for diffuse, pulsating and stable arc conditions met. The total energy content in the electromagnetic radiation measured is 0.61 mW/sq m for the diffuse aurora (1980) and 0.67 mW/sq for the stable arc (1981). The spatial distribution of selected emissions exhibit distinct differences for the the auroral events observed.

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