Slow magnetohydrodynamic oscillations of the thin magnetic flux tubes: phase relationships and solar photosphere diagnostics

  • Yu.T. Tsap Crimean Astrophysical Observatory
  • A.V. Stepanov 2Главная (Пулковская) астрономическая обсерватория РАН, Пулковское шоссе 65/1, Санкт-Петербург, 196140
  • Yu.G. Kopylova Главная (Пулковская) астрономическая обсерватория РАН, Пулковское шоссе 65/1, Санкт-Петербург, 196140

Abstract

Based on the thin flux tube approximation the phase relationships between disturbed quantities of the linear evanescent magnetohydrodynamic waves under the isothermal stratified conditions have been considered. It has been shown that the resonance (excited on the cutoff frequency) modes can be responsible for the origin of the solar photospheric oscillations revealed with the Hinode satellite.

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Published
2016-07-01
How to Cite
Tsap Y., Stepanov A., Kopylova Y., 2016. Izvestiya Krymskoi Astrofizicheskoi Observatorii, vol. 112, no. 1, pp. 94-99. Available at: https://jn.craocrimea.ru/index.php/izvcrao/article/view/168 (Accessed: 1December2020)
Section
Сonference proceedings