Published July 1975 | Version v1
Journal article Metadata-only

Heights of formation of non-magnetic solar lines suitable for velocity studies

Creators

  • 1. Sacramento Peak Observatory, Air Force Cambridge Research Laboratories, Sunspot, New Mexico 88349, USA
  • 2. Kitt Peak National Observatory, Tucson, Ariz. (USA)

Description

Heights of formation of lines that do not exhibit Zeeman splitting are calculated using an LTE, partial non-LTE, and full non LTE approach. Non-magnetic (g=0) lines are valuable for velocity investigations in quiet-Sun magnetic field regions, and a knowledge of their formation heights is useful for obtaining three dimensional velocity profiles in these regions. (Auth.)

Additional details

Identifiers

DOI
10.1007/bf00155139;

Publishing Information

Journal Title
Solar Physics
Journal Volume
43
Journal Issue
1
Series
Sol. Phys.
Journal Page Range
33-37
ISSN
0038-0938

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
7226430
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ABSORPTION SPECTRA; CHROMOSPHERE; DOPPLER EFFECT; LTE; MAGNETIC FIELDS; PHOTOSPHERE; RESPONSE FUNCTIONS; SUN; VELOCITY
Descriptors DEC
EQUILIBRIUM; FUNCTIONS; SPECTRA; STARS

Optional Information

Notes
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