The primary results of research on solar oscillations by using magnetic field telescope.

Details The primary results of research on solar oscillations by using magnetic field telescope. The primary results of research on solar oscillations by using magnetic field telescope.

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pyuno...2....1z&link_type=abstract

Publications of the Yunnan Observatory, No. 2, p. 1 - 9

Physics

Scientific paper

The time series data of λ5324.19 Å velocity field from Magnetic Field Telescope at Beijing Observatory have been analysed. Two (l-ν) spectra for zonal modes and sectorial modes were obtained respectively. Five-minute oscillation and the oscillation with period longer than ten minutes exist in both power spectra. From the power spectrum, the authors have recognized f mode, p1 modes and p2 modes with the degree between 10 and 60. Also both power spectra indicate the oscillations with period of 48.3 min and degree l equal to 12 and 20, they can be classfied into g modes with order n probably equal to 7 and 10 respectively.

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