Temperature distribution in the transition region and inner corona

descriptionPublicationkeyboard_double_arrow_right Article 01 May 1979 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 62, pages 93-105 (issn: 0038-0938, eissn: 1573-093X,

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Authors: Badr� Alam; S. M. Razaullah Ansari; Abdul Qaiyum;

doi: 10.1007/bf00150136

Temperature distribution in the transition region and inner corona

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Abstract

The energy balance equation for a general solar atmosphere without assuming the plane-parallel approximation is solved analytically. This leads to models for both the transition region and inner corona as well as for the outer corona. The form of the latter is very similar to that of the hydrostatic conduction model of Chapman (1957). However, in this paper we confine ourselves only to the former.

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