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Spiral structure of the magnetic field in AO 0953 over a stable spot.
A two-dimensional high-altitude structure of the coronal magnetic field,
with the power tube extending up the ~0.4о-wide spiral was
observed over a stable spot in the active region AO 0953. The magnetic
field of around 600Gs is located at a rather high altitude in the solar
corona (up to 25 thousand km). Radio astronomical multifrequency
polarization observations of sources with the RATAN-600 were used.
In collaboration with St. Petersburg University.
(Contacts: V.M. Bogod)
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