Resonant absorption and the spectrum of 5-min oscillations of the Sun. III. Influence of inhomogeneity of the canopy magnetic field on fine structure

Details Resonant absorption and the spectrum of 5-min oscillations of the Sun. III. Influence of inhomogeneity of the canopy magnetic field on fine structure Resonant absorption and the spectrum of 5-min oscillations of the Sun. III. Influence of inhomogeneity of the canopy magnetic field on fine structure

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...369..672z&link_type=abstract

Astronomy and Astrophysics, v.369, p.672-676 (2001)

Astronomy and Astrophysics

Astrophysics

4

Sun: Oscillations, Chromosphere, Mhd

Scientific paper

We studied influence of magnetic field on the spectrum of 5-min solar oscillations. The calculations were made within a two-layer shell model. The lower non-magnetized layer is characterized by a linear decrease in temperature with height while in the upper layer (with an inhomogeneous horizontal magnetic field) the temperature increases and reaches the coronal value at a height of about 2500 km. The fine structure of the spectrum of 5-min oscillations was calculated for f-, p_1- and p_2- modes for large k.

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