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Chromosperic oscillations

By R.J. Rutten

Abstract

This review concentrates on the quiet-Sun chromosphere.\ud Its internetwork areas are dynamically dominated by the\ud so-called chromospheric three-minute oscillation. They\ud are interpretationally dominated by the so-called Ca II\ud K 2V and H 2V grains. The main points of this review are\ud that the one phenomenon explains the other (both ways),\ud that the quiet-Sun chromosphere is a clapotisphere per-\ud vaded by shocks above h = 1 Mm, and that the existence\ud of the classical temperature minimum is in doubt

Topics: Natuur- en Sterrenkunde, solar oscillations, chromosphere, clapoti-sphere
Year: 1999
OAI identifier: oai:dspace.library.uu.nl:1874/2627

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