Reconstruction of solar UV irradiance

N. A. Krivova; S. K. Solanki

doi:10.1016/j.asr.2004.12.027

Reconstruction of solar UV irradiance

N. A. Krivova
, S. K. Solanki

Research output: Contribution to journal › Article › peer-review

18 Citations (Scopus)

Abstract

Understanding solar influence on the Earth's climate requires a reconstruction of solar irradiance for the pre-satellite period. Considerable advances have been made in modelling the irradiance variations at wavelengths longer than 200 nm. At shorter wavelengths, however, the LTE approximation usually taken in such models fails, which makes a reconstruction of the solar UV irradiance a rather intricate problem. We choose an alternative approach and use the observed SUSIM UV spectra to extrapolate available models to shorter wavelengths.

Original language	English
Pages (from-to)	361-364
Number of pages	4
Journal	Advances in Space Research
Volume	35
Issue number	3
DOIs	https://doi.org/10.1016/j.asr.2004.12.027
Publication status	Published - 2005

Keywords

Solar UV radiation
Solar activity
Solar irradiance
Solar-terrestrial relations

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10.1016/j.asr.2004.12.027

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title = "Reconstruction of solar UV irradiance",

abstract = "Understanding solar influence on the Earth's climate requires a reconstruction of solar irradiance for the pre-satellite period. Considerable advances have been made in modelling the irradiance variations at wavelengths longer than 200 nm. At shorter wavelengths, however, the LTE approximation usually taken in such models fails, which makes a reconstruction of the solar UV irradiance a rather intricate problem. We choose an alternative approach and use the observed SUSIM UV spectra to extrapolate available models to shorter wavelengths.",

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AU - Krivova, N. A.

AU - Solanki, S. K.

PY - 2005

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AB - Understanding solar influence on the Earth's climate requires a reconstruction of solar irradiance for the pre-satellite period. Considerable advances have been made in modelling the irradiance variations at wavelengths longer than 200 nm. At shorter wavelengths, however, the LTE approximation usually taken in such models fails, which makes a reconstruction of the solar UV irradiance a rather intricate problem. We choose an alternative approach and use the observed SUSIM UV spectra to extrapolate available models to shorter wavelengths.

KW - Solar UV radiation

KW - Solar activity

KW - Solar irradiance

KW - Solar-terrestrial relations

UR - https://www.scopus.com/pages/publications/20444436412

U2 - 10.1016/j.asr.2004.12.027

DO - 10.1016/j.asr.2004.12.027

M3 - Article

AN - SCOPUS:20444436412

SN - 0273-1177

VL - 35

SP - 361

EP - 364

JO - Advances in Space Research

JF - Advances in Space Research

IS - 3

ER -

Reconstruction of solar UV irradiance

Abstract

Keywords

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