Oscillations trapped in a chromosphere with a horizontal magnetic field

Details Oscillations trapped in a chromosphere with a horizontal magnetic field Oscillations trapped in a chromosphere with a horizontal magnetic field

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..712z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Sept. 1985, p. 712-716) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Sept.-O

Astronomy and Astrophysics

Astronomy

Chromosphere, Magnetohydrodynamic Waves, Solar Atmosphere, Solar Magnetic Field, Solar Oscillations, Conducting Fluids, Solar Temperature

Scientific paper

The propagation of adiabatic MHD waves in a conductive isothermal atmosphere in the presence of a horizontal magnetic field and gravity is considered. It is shown that the oscillations may be trapped in the middle layer of a three-layer atmosphere with temperatures T1 > T2 > T3 for discrete frequencies. In the presence of a horizontal magnetic field the solar chromospheric trapped waves have periods in the range of 250 - 2730 s.

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