Standard

Representation of opacity data in solar model atmosphere calculations. / Haberreiter, M; Rozanov, E; Ruedi; Schmutz, W.

STELLAR ATMOSPHERE MODELING. ed. / Hubeny; D Mihalas; K Werner. Astronomical Society of the Pacific, 2003. p. 165-168 (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES; Vol. 288).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review

Harvard

Haberreiter, M, Rozanov, E, Ruedi & Schmutz, W 2003, Representation of opacity data in solar model atmosphere calculations. in Hubeny, D Mihalas & K Werner (eds), STELLAR ATMOSPHERE MODELING. ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES, vol. 288, Astronomical Society of the Pacific, pp. 165-168, International Workshop on Stellar Atmosphere Modeling, TUBINGEN, Germany, 8/04/02.

APA

Haberreiter, M., Rozanov, E., Ruedi, & Schmutz, W. (2003). Representation of opacity data in solar model atmosphere calculations. In Hubeny, D. Mihalas, & K. Werner (Eds.), STELLAR ATMOSPHERE MODELING (pp. 165-168). (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES; Vol. 288). Astronomical Society of the Pacific.

Vancouver

Haberreiter M, Rozanov E, Ruedi, Schmutz W. Representation of opacity data in solar model atmosphere calculations. In Hubeny, Mihalas D, Werner K, editors, STELLAR ATMOSPHERE MODELING. Astronomical Society of the Pacific. 2003. p. 165-168. (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES).

Author

Haberreiter, M ; Rozanov, E ; Ruedi ; Schmutz, W. / Representation of opacity data in solar model atmosphere calculations. STELLAR ATMOSPHERE MODELING. editor / Hubeny ; D Mihalas ; K Werner. Astronomical Society of the Pacific, 2003. pp. 165-168 (ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES).

BibTeX

@inproceedings{c7ffdb02537e466497c74966d0becd68,
title = "Representation of opacity data in solar model atmosphere calculations",
abstract = "We present synthetic solar intensity spectra in the UV calculated with the code COSI (COde for Solar Irradiance). We have evaluated the dominant solar opacity sources, and find it necessary to include the complex bound-free cross sections of the lower levels of neutral metals. Here we evaluate the quality of our implementation using a coarse frequency discretization and find such a description to be sufficient for atmosphere calculations.",
author = "M Haberreiter and E Rozanov and Ruedi and W Schmutz",
year = "2003",
language = "Английский",
isbn = "1-58381-131-1",
series = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",
publisher = "Astronomical Society of the Pacific",
pages = "165--168",
editor = "Hubeny and D Mihalas and K Werner",
booktitle = "STELLAR ATMOSPHERE MODELING",
address = "Соединенные Штаты Америки",
note = "null ; Conference date: 08-04-2002 Through 12-04-2002",

}

RIS

TY - GEN

T1 - Representation of opacity data in solar model atmosphere calculations

AU - Haberreiter, M

AU - Rozanov, E

AU - Ruedi, null

AU - Schmutz, W

PY - 2003

Y1 - 2003

N2 - We present synthetic solar intensity spectra in the UV calculated with the code COSI (COde for Solar Irradiance). We have evaluated the dominant solar opacity sources, and find it necessary to include the complex bound-free cross sections of the lower levels of neutral metals. Here we evaluate the quality of our implementation using a coarse frequency discretization and find such a description to be sufficient for atmosphere calculations.

AB - We present synthetic solar intensity spectra in the UV calculated with the code COSI (COde for Solar Irradiance). We have evaluated the dominant solar opacity sources, and find it necessary to include the complex bound-free cross sections of the lower levels of neutral metals. Here we evaluate the quality of our implementation using a coarse frequency discretization and find such a description to be sufficient for atmosphere calculations.

M3 - статья в сборнике материалов конференции

SN - 1-58381-131-1

T3 - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES

SP - 165

EP - 168

BT - STELLAR ATMOSPHERE MODELING

A2 - Hubeny, null

A2 - Mihalas, D

A2 - Werner, K

PB - Astronomical Society of the Pacific

Y2 - 8 April 2002 through 12 April 2002

ER -

ID: 122465307