Long-period network oscillations in the solar chromosphere

Details Long-period network oscillations in the solar chromosphere Long-period network oscillations in the solar chromosphere

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.274l...1l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 1, pp. L1-L4.

Astronomy and Astrophysics

Astronomy

16

Mhd, Sun: Chromosphere, Sun: Magnetic Fields, Sun: Oscillations, Sun: Transition Region

Scientific paper

Recent observations of solar chromospheric oscillations have revealed two different types: 3-min intranetwork oscillations above the supergranule cells; and long-period (~5 to 20 min) oscillations associated with the bright chromospheric network. It has been speculated previously that the long-period network oscillations could be somehow related to low-frequency magneto-gravity waves in magnetized boundary lanes surrounding supergranules. We explore this scenario and examine its feasibility, as well as constraints based on a magnetohydrodynamic (MHD) model for the long-period solar network oscillations.

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