Analysis of solar activity during the period of Halley encounter

Details Analysis of solar activity during the period of Halley encounter Analysis of solar activity during the period of Halley encounter

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250a.157v&link_type=abstract

In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas p 157-159 (SEE N87

Physics

Halley'S Comet, Solar Activity Effects, Solar Radiation, Coronal Holes, Solar Flares, Solar Wind

Scientific paper

Chromospheric flares and coronal holes occurring during Halley encounter are discussed. Chromospheric flares are sources of X and UV radiation, and coronal holes are regions of solar wind emission. The X and UV radiation can influence the comet only if the source is directly visible on the solar disk. Charged particles of solar wind move in an orbit which has the form of an Archimedes spiral and this makes possible influence from sources that are up to 40 deg behind the visible solar limb.

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