Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...354..277z&link_type=abstract
Astronomy and Astrophysics, v.354, p.277-279 (2000)
Astronomy and Astrophysics
Astrophysics
3
Sun: Oscillations, Sun: Chromosphere, Magnetohydrodynamics (Mhd)
Scientific paper
The influence of magnetic field on the spectrum of 5-min solar oscillations has been investigated. The calculations have been made within a model of the two-layer shell. The lower non-magnetized layer is characterized by linear decrease of temperature with height while in the upper layer with homogeneous horizontal magnetic field temperature increase, and reaches a coronal value at the height of about 2500km. It is shown that, accounting for resonant absorption, the spectrum of 5-min oscillations has fine structure, which is most noticeable in high - degree modes.
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