The effect of the solar magnetic field on dust-particle orbits in the F corona

Details The effect of the solar magnetic field on dust-particle orbits in the F corona The effect of the solar magnetic field on dust-particle orbits in the F corona

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....96.1447r&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 96, Oct. 1988, p. 1447-1454.

Astronomy and Astrophysics

Astronomy

7

Gravitational Fields, Light Scattering, Solar Corona, Solar Eclipses, Solar Magnetic Field, Zodiacal Dust, Interplanetary Magnetic Fields, Light Speed, Lorentz Force, Solar Wind Velocity

Scientific paper

In order to determine whether the solar magnetic field can align circumsolar dust into rings such as those described by Mizutani et al. (1984), the solar magnetic field is divided into its various multipole components and theoretical expressions are derived to determine the effect of each of these components on the orbital elements of circumsolar dust. Simulations are then carried out to determine the effect of a dynamic solar magnetic field on such particles using actual values of the solar magnetic field supplied by Hoeksema (1984). These results are compared to observations of the F corona.

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