Precipitation Diffusion Model of Solar-Wind Particles for Sky Brightness Variation

Details Precipitation Diffusion Model of Solar-Wind Particles for Sky Brightness Variation Precipitation Diffusion Model of Solar-Wind Particles for Sky Brightness Variation

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..439u&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

Scientific paper

The solar-cycle sky brightness variation discovered by Sakurai (Earth
Planets Space, 54, 153--157, 2002) is interpreted in terms of the
precipitation diffusion model of solar-wind particles. Implication in
the solar-cycle global warming is also discussed.

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