Complex structure of the magnetic field of the CP star HD32633

Details Complex structure of the magnetic field of the CP star HD32633 Complex structure of the magnetic field of the CP star HD32633

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008astbu..63..259g&link_type=abstract

Astrophysical Bulletin, Volume 63, Issue 3, pp.259-263

Astronomy and Astrophysics

Astrophysics

2

96.12.Hg, 96.15.Gh

Scientific paper

The method of “virtual magnetic charges” is used to analyze the structure of the magnetic field of the CP star HD32633. The phase relation of its magnetic field differs strongly from a sine wave. The structure of the star’s field can be described fairly well by two dipoles located in the opposite regions of the star near its rotation equator. Each of these dipoles produces two pairs of magnetic spots of opposite polarity similar to sunspots. The dipoles are located at a distance of Δ a=0.6 R from the center, where R is the radius of the star. The field strength at the poles is equal to ±42 and ±19 kG.

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