Solar flare effects on neutral gas glow in interplanetary space

Details Solar flare effects on neutral gas glow in interplanetary space Solar flare effects on neutral gas glow in interplanetary space

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..369g&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, April 1989, p. 369-377.

Physics

1

Interplanetary Space, Neutral Gases, Resonance Lines, Solar Flares, Heliosphere, Interstellar Matter, Line Of Sight, Solar System

Scientific paper

Simultaneous measurements of solar emission bursts and variations in the neutral gas glow in the heliosphere are suggested as a way to derive the neutral atom number density distribution along the line-of-sight. The magnitude and occurrence frequency of solar flares in EUV are studied using the relation between EUV flare emission enhancement and apparent solar flare area in H-alpha. Analytical expressions are obtained for glow temporal variations for several model number density distributions. A space experiment using a radar-like remote probing technique is proposed to study the neutral gas characteristics inside the heliosphere.

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