On the possibility of detecting solar flare effects in the zodiacal light

Details On the possibility of detecting solar flare effects in the zodiacal light On the possibility of detecting solar flare effects in the zodiacal light

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23.1329m&link_type=abstract

Planetary and Space Science, vol. 23, Sept. 1975, p. 1329-1335.

Physics

2

Brightness, Solar Activity Effects, Solar Flares, Zodiacal Light, Atmospheric Models, Dust, Ice Nuclei, Metal Particles, Plasma-Particle Interactions, Shock Fronts

Scientific paper

To evaluate possible effects of solar flares on the brightness of the inner zodiacal light, it is necessary to consider the brightness contribution along the line of sight and as a function of sun-particle distance. For this purpose, models of the brightness contribution along the line of sight are presented for both dielectric and metallic particles with a spatial distribution of the form 1, 1/r, and 1/r-squared. These models are discussed in terms of the geometry of shock front interaction. A reported zodiacal light enhancement following a solar flare (Blackwell and Ingham, 1961) is analyzed on the basis of the shock front geometry.

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