The ultralarge-scale magnetic field of the sun

Details The ultralarge-scale magnetic field of the sun The ultralarge-scale magnetic field of the sun

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..246k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, May 1979, p. 246-250.) Soviet Astronomy Letters, vol. 5, May-June 1979, p. 130-133.

Astronomy and Astrophysics

Astronomy

1

Field Strength, Solar Magnetic Field, Interplanetary Magnetic Fields, Magnetic Flux, Polarity, Solar Corona

Scientific paper

A method is proposed for investigating the ultralarge-scale solar magnetic field, which is responsible for generating the interplanetary magnetic field. Noneclipse observations of the outer (3-10 solar radii) corona in white light are analyzed, and both the sign and the inversion line of the ultralarge-scale field on the sun are determined. From these results and measurements of the magnetic flux of the sun as a star, an estimate is obtained for the strength of the ultralarge-scale field.

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