Published March 4, 2011
| Version v1
Journal article
Modeling of continuous absorption of electromagnetic radiation in dense partially ionized plasmas
- 1. Institute of Physics, Belgrade University, Pregrevica 118, Zemun, 11080 Belgrade (Serbia)
- 2. UPMC Univ Paris 6, Laboratoire des Plasmas Denses, 3 rue Galilee, 94200 Ivry sur Seine (France)
Description
A new modeling way of describing the continuous absorption of electromagnetic (EM) radiation in a dense partially ionized hydrogen plasma is tested in this work. It is shown that the obtained results give a possibility of calculating spectral absorption coefficients which characterize the relevant absorption processes in partially ionized hydrogen plasmas with electron densities Ne ∼ 1019 cm-3 and temperatures T ∼ 2 x 104 K. A key parameter of the used procedure is determined empirically. The calculation method is applied to the wavelength region 300 nm < λ < 500 nm. The presented results can be of interest for dense laboratory plasmas as well as for partially ionized layers of different stellar atmospheres.
Availability note (English)
Available from http://dx.doi.org/10.1088/1751-8113/44/9/095502Additional details
Identifiers
- DOI
- 10.1088/1751-8113/44/9/095502;
- PII
- S1751-8113(11)74164-6;
Publishing Information
- Journal Title
- Journal of Physics. A, Mathematical and Theoretical (Online)
- Journal Volume
- 44
- Journal Issue
- 9
- Journal Page Range
- [17 p.]
- ISSN
- 1751-8121
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43067299
- Subject category
- S97: MATHEMATICAL METHODS AND COMPUTING; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION; CALCULATION METHODS; ELECTROMAGNETIC RADIATION; ELECTRON DENSITY; HYDROGEN; MATHEMATICAL MODELS; PLASMA; SIMULATION; STELLAR ATMOSPHERES
- Descriptors DEC
- ATMOSPHERES; ELEMENTS; NONMETALS; RADIATIONS; SORPTION