Published 1975 | Version v1
Journal article Metadata-only

A theoretical model of the solar chromosphere

Creators

  • 1. Lorand Eoetvoes University, Budapest (Hungary). Astronomical Department

Description

A theoretical model of the solar chromosphere is presented. The model was calculated under the assumption of the equality of the emission coefficient of solar matter and the absorption coefficient of weak magnetodynamic shock waves generated in the convective zone. The results show that temperature increased with height. (author)

Additional details

Publishing Information

Journal Title
Bull. Astron. Inst. Czech.
Journal Volume
26
Journal Issue
5
Series
Bull. Astron. Inst. Czech.
Journal Page Range
317-319

INIS

Country of Publication
Serbia and Montenegro
Country of Input or Organization
Serbia and Montenegro
INIS RN
7224320
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSORPTION; CHROMOSPHERE; COMPUTER CALCULATIONS; EMISSION; HYDROSTATICS; MAGNETOACOUSTIC WAVES; MATHEMATICAL MODELS; SOLAR ATMOSPHERE; SUN; ULTRAHIGH TEMPERATURE
Descriptors DEC
ATMOSPHERES; HYDROMAGNETIC WAVES; STARS