On Pikel'ner's theory of prominences

Details On Pikel'ner's theory of prominences On Pikel'ner's theory of prominences

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52...37e&link_type=abstract

Solar Physics, vol. 52, Apr. 1977, p. 37-40.

Physics

10

Gas Streams, Solar Corona, Solar Prominences, Boundary Conditions, Boundary Value Problems, Condensing, Magnetic Effects, Solar Wind

Scientific paper

Pikel'ner (1971) computed a steady-state solution for coronal gas
streaming along a magnetic arch, which develops into a dense
condensation similar to prominence matter. This paper discusses the
choice of boundary conditions and presents additional solutions.

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