Bibcode
Kneer, F.; Trujillo-Bueno, J.
Bibliographical reference
Astronomy and Astrophysics (ISSN 0004-6361), vol. 183, no. 1, Sept. 1987, p. 91-97.
Advertised on:
9
1987
Citations
14
Refereed citations
12
Description
Energy transport by radiation is an important contribution to the energy
budget in stellar atmospheric structures. In this paper, radiative
relaxation of small-scale structures is investigated. The authors show
in a linear analysis: (1) Already at structural lengths of 10 opacity
scale heights, horizontal photon exchange is important for the energy
budget. (2) In atmospheric layers near continuum optical depth
τc = 1 and below, the continuum absorption and emission
processes dominate the radiative relaxation. (3) Weak spectral lines or
lines with σlɛ ≤ 1 have little influence on
the energy exchange. (4) At large heights, transport in few spectral
lines with σlɛ very large 1 can compete with
continuum processes.