Standard

Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere. / Haberreiter, M; Hubeny, ; Rozanov, E; Ruedi; Schmutz, W; Wenzler, T.

PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO. ed. / A Wilson. ESA Publication Division, 2002. p. 209-212 (ESA SPECIAL PUBLICATIONS; Vol. 508).

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

Harvard

Haberreiter, M, Hubeny, , Rozanov, E, Ruedi, Schmutz, W & Wenzler, T 2002, Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere. in A Wilson (ed.), PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO. ESA SPECIAL PUBLICATIONS, vol. 508, ESA Publication Division, pp. 209-212, SOHO-11 Symposium on From Solar Min to Max, DAVOS, Switzerland, 11/03/02.

APA

Haberreiter, M., Hubeny, Rozanov, E., Ruedi, Schmutz, W., & Wenzler, T. (2002). Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere. In A. Wilson (Ed.), PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO (pp. 209-212). (ESA SPECIAL PUBLICATIONS; Vol. 508). ESA Publication Division.

Vancouver

Haberreiter M, Hubeny , Rozanov E, Ruedi, Schmutz W, Wenzler T. Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere. In Wilson A, editor, PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO. ESA Publication Division. 2002. p. 209-212. (ESA SPECIAL PUBLICATIONS).

Author

Haberreiter, M ; Hubeny, ; Rozanov, E ; Ruedi ; Schmutz, W ; Wenzler, T. / Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere. PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO. editor / A Wilson. ESA Publication Division, 2002. pp. 209-212 (ESA SPECIAL PUBLICATIONS).

BibTeX

@inproceedings{21f3582dac924808bd23b92baf47d510,
title = "Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere",
abstract = "We present our analysis of data taken by SUSIM on-board UARS. We reconstruct the variability of the UV irradiance and compare it to available data. Up to now we model the solar irradiance according to the 3-component model by Unruh et al. (1999) based on LTE synthetic spectra modeled with Kurucz' ATLAS9 code. Our new approach will be that with COSI (COde for Solar Irradiance) we model solar continuum and line formation in spherical symmetry and in non-local thermodynamic equilibrium (non-LTE). We present our first synthetic solar spectra (calculated in LTE) and validate them against spectra computed with Kurucz' ATLAS9 code.",
keywords = "Sun : UV irradiance, Sun : variability, radiative transfer, ATMOSPHERES, MODELS, STARS",
author = "M Haberreiter and Hubeny and E Rozanov and Ruedi and W Schmutz and T Wenzler",
year = "2002",
language = "Английский",
isbn = "92-9092-818-2",
series = "ESA SPECIAL PUBLICATIONS",
publisher = "ESA Publication Division",
pages = "209--212",
editor = "A Wilson",
booktitle = "PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO",
address = "Франция",
note = "null ; Conference date: 11-03-2002 Through 15-03-2002",

}

RIS

TY - GEN

T1 - Towards a spherical code for the evaluation of solar UV-bands that influence the chemical composition in the stratosphere

AU - Haberreiter, M

AU - Hubeny, null

AU - Rozanov, E

AU - Ruedi, null

AU - Schmutz, W

AU - Wenzler, T

PY - 2002

Y1 - 2002

N2 - We present our analysis of data taken by SUSIM on-board UARS. We reconstruct the variability of the UV irradiance and compare it to available data. Up to now we model the solar irradiance according to the 3-component model by Unruh et al. (1999) based on LTE synthetic spectra modeled with Kurucz' ATLAS9 code. Our new approach will be that with COSI (COde for Solar Irradiance) we model solar continuum and line formation in spherical symmetry and in non-local thermodynamic equilibrium (non-LTE). We present our first synthetic solar spectra (calculated in LTE) and validate them against spectra computed with Kurucz' ATLAS9 code.

AB - We present our analysis of data taken by SUSIM on-board UARS. We reconstruct the variability of the UV irradiance and compare it to available data. Up to now we model the solar irradiance according to the 3-component model by Unruh et al. (1999) based on LTE synthetic spectra modeled with Kurucz' ATLAS9 code. Our new approach will be that with COSI (COde for Solar Irradiance) we model solar continuum and line formation in spherical symmetry and in non-local thermodynamic equilibrium (non-LTE). We present our first synthetic solar spectra (calculated in LTE) and validate them against spectra computed with Kurucz' ATLAS9 code.

KW - Sun : UV irradiance

KW - Sun : variability

KW - radiative transfer

KW - ATMOSPHERES

KW - MODELS

KW - STARS

M3 - статья в сборнике материалов конференции

SN - 92-9092-818-2

T3 - ESA SPECIAL PUBLICATIONS

SP - 209

EP - 212

BT - PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO

A2 - Wilson, A

PB - ESA Publication Division

Y2 - 11 March 2002 through 15 March 2002

ER -

ID: 122466489