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Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux. / Rozanov, E; Frohlich, C; Haberreiter, M; Peter, T; Schmutz, W.

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. 181-184 (ESA Special Publications; Vol. 508).

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

Harvard

Rozanov, E, Frohlich, C, Haberreiter, M, Peter, T & Schmutz, W 2002, Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux. 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. 181-184, SOHO-11 Symposium on From Solar Min to Max, DAVOS, Switzerland, 11/03/02.

APA

Rozanov, E., Frohlich, C., Haberreiter, M., Peter, T., & Schmutz, W. (2002). Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux. In A. Wilson (Ed.), PROCEEDINGS OF THE SOHO 11 SYMPOSIUM ON FROM SOLAR MIN TO MAX: HALF A SOLAR CYCLE WITH SOHO (pp. 181-184). (ESA Special Publications; Vol. 508). ESA Publication Division.

Vancouver

Rozanov E, Frohlich C, Haberreiter M, Peter T, Schmutz W. Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux. 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. 181-184. (ESA Special Publications).

Author

Rozanov, E ; Frohlich, C ; Haberreiter, M ; Peter, T ; Schmutz, W. / Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux. 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. 181-184 (ESA Special Publications).

BibTeX

@inproceedings{64bb78b2da78458d9e10dba4cc95e9f6,
title = "Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux.",
abstract = "We have applied a 1-D steady-state radiative-convective model with interactive photochemistry to estimate the sensitivity of temperature and ozone mixing ratio to the observed variability of the extraterrestrial spectral solar irradiance. We have carried out several runs using the spectral solar flux for minimum and maximum solar activity conditions. The results show that the ozone and temperature in the stratosphere are mostly sensitive to the solar flux variations in the spectral area between 200 and 220 rim, where they positively correlate with solar flux intensity. In the upper stratosphere and mesosphere the effects of the solar flux variability in the Lyman-alpha line and Schumann-Runge band are found to be very important. The obtained results have an implication for the optimal choice of wavelength to be measured from a satellite and for the understanding of what kind of radiation code should be used in a GCM aimed to study solar-climate connections.",
keywords = "VARIABILITY, STRATOSPHERE, CLIMATE, MIDDLE, CYCLE, MODEL",
author = "E Rozanov and C Frohlich and M Haberreiter and T Peter and W Schmutz",
year = "2002",
language = "Английский",
isbn = "92-9092-818-2",
series = "ESA Special Publications",
publisher = "ESA Publication Division",
pages = "181--184",
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 - Estimation of the ozone and temperature sensitivity to the variation of spectral solar flux.

AU - Rozanov, E

AU - Frohlich, C

AU - Haberreiter, M

AU - Peter, T

AU - Schmutz, W

PY - 2002

Y1 - 2002

N2 - We have applied a 1-D steady-state radiative-convective model with interactive photochemistry to estimate the sensitivity of temperature and ozone mixing ratio to the observed variability of the extraterrestrial spectral solar irradiance. We have carried out several runs using the spectral solar flux for minimum and maximum solar activity conditions. The results show that the ozone and temperature in the stratosphere are mostly sensitive to the solar flux variations in the spectral area between 200 and 220 rim, where they positively correlate with solar flux intensity. In the upper stratosphere and mesosphere the effects of the solar flux variability in the Lyman-alpha line and Schumann-Runge band are found to be very important. The obtained results have an implication for the optimal choice of wavelength to be measured from a satellite and for the understanding of what kind of radiation code should be used in a GCM aimed to study solar-climate connections.

AB - We have applied a 1-D steady-state radiative-convective model with interactive photochemistry to estimate the sensitivity of temperature and ozone mixing ratio to the observed variability of the extraterrestrial spectral solar irradiance. We have carried out several runs using the spectral solar flux for minimum and maximum solar activity conditions. The results show that the ozone and temperature in the stratosphere are mostly sensitive to the solar flux variations in the spectral area between 200 and 220 rim, where they positively correlate with solar flux intensity. In the upper stratosphere and mesosphere the effects of the solar flux variability in the Lyman-alpha line and Schumann-Runge band are found to be very important. The obtained results have an implication for the optimal choice of wavelength to be measured from a satellite and for the understanding of what kind of radiation code should be used in a GCM aimed to study solar-climate connections.

KW - VARIABILITY

KW - STRATOSPHERE

KW - CLIMATE

KW - MIDDLE

KW - CYCLE

KW - MODEL

M3 - статья в сборнике материалов конференции

SN - 92-9092-818-2

T3 - ESA Special Publications

SP - 181

EP - 184

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: 122467105