Magneto-gravity Waves Trapped in the Lower Solar Corona

Details Magneto-gravity Waves Trapped in the Lower Solar Corona Magneto-gravity Waves Trapped in the Lower Solar Corona

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..261l&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 261-264 (1999).

Physics

Coronal Holes, Coronal Seismology, Magneto-Gravity Waves, Solar Corona, Spicules, Supergranules, Transition Region

Scientific paper

The possibility of trapped magneto-gravity waves in the lower solar corona with an open magnetic field is discussed. Intensity variations and/or Doppler shifts of relevant UV, EUV and x-ray spectral lines in the chromosphere, transition region and lower corona may reveal the existence of such low-frequency modes (with periods longer than ˜ 1.5 hour). The spectrum may be either discrete or continuous depending on the reflection property of the narrow transition region. These modes can be utilized to probe the dynamics of the upper chromosphere, transition region and lower corona; they may also play an important role in coronal heating.

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