Published December 1, 1990
| Version v1
Journal article
Hydrogen stark profiles for astrophysics
Creators
- 1. Department Atomes et Moleules en Astrophysique et URA812 du CNRS Observatoires de Paris, 5 Place. J. Janssen, 92195 Meudon Cedex, France (France)
Description
A large number of hydrogen line profiles are calculated in the framework of the model microfield method with specific modification for electronic contributions. Profiles of the Lyman, Balmer and Paschen series have been obtained from the center to the Holtsmark wings of the lines
Additional details
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 216
- Journal Issue
- 1
- Series
- AIP Conf. Proc.
- Journal Page Range
- 607-608
- ISSN
- 0094-243X
- CODEN
- APCPC
Conference
- Title
- 10. international conference on spectral line shapes.
- Dates
- 25-29 Jun 1990.
- Place
- Austin, TX (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22052754
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- HYDROGEN; HYDROGEN IONS; LYMAN LINES; PLASMA DENSITY; SPECTRAL SHIFT; STARK EFFECT; STELLAR ATMOSPHERES
- Descriptors DEC
- ATMOSPHERES; CHARGED PARTICLES; ELEMENTS; IONS; NONMETALS
Optional Information
- Secondary number(s)
- CONF-9006278--.