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Digitale Medien

A model for X-ray emission from loop prominences (1977)

Phillips, K. J. H. ; Zirker, J. B.

Springer

Solar physics 53 (1977), S. 41-58

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ISSN: 1573-093X

Quelle: Springer Online Journal Archives 1860-2000

Thema: Physik

Notizen: Abstract A study is made of X-ray line emission observed during the developing stages of a set of post-flare loop prominences. The time behaviour of the line emission can be described by a model consisting of two flux tubes containing plasma heated impulsively at the flash phase; the plasma cools by radiation and by conduction to the chromosphere. These ideas are extended to the possible formation of Hα prominences from low-lying hot loops.

Materialart: Digitale Medien

URL: http://dx.doi.org/10.1007/BF02260208

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