On a halo of icy bodies as a possible source of flareups of cometary brightness - Mathematical model of a flareup

Details On a halo of icy bodies as a possible source of flareups of cometary brightness - Mathematical model of a flareup On a halo of icy bodies as a possible source of flareups of cometary brightness - Mathematical model of a flareup

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..335a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Mar.-Apr. 1986, p. 335-348) Soviet Astronomy (ISSN 0038-5301), vol. 30, Mar.-Apr. 1986, p. 2

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Brightness Distribution, Cometary Atmospheres, Ice, Solar Activity Effects, Solar Corpuscular Radiation, Differential Equations, Integral Equations, Particle Size Distribution, Solar Wind, Temporal Distribution

Scientific paper

A mathematical model is proposed for the mechanism of flareups of the brightness of comets, based on the process of fragmentation of unstable icy bodies contained in their atmospheres under the action of particles of high-velocity corpuscular streams of the solar wind. The model well explains the set of phenomena observed during flareups of cometary brightness.

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