|Publication type:||Article in scientific journal|
|Type of review:||Peer review (publication)|
|Authors:||Solanki, S. A.|
Krivova, N. A.
|Published in:||Advances in Space Research|
|Publisher / Ed. Institution:||Elsevier|
|Subjects:||Solar magnetic field; Solar–terrestrial relations; Solar activity; Solar irradiance|
|Subject (DDC):||500: Natural sciences|
|Abstract:||Measurements of solar irradiance have revealed variations at all the sampled time scales (ranging from minutes to the length of the solar cycle). One important task of models is to identify the causes of the observed (total and spectral)irradiance variations. Another major aim is to reconstruct irradiance over time scales longer than sampled by direct measurements in order to consider if and to what extent solar irradiance variations may be responsible for global climate change. Here, we describe recent efforts to model solar irradiance over the current and the previous two solar cycles. These irradiance models are remarkably successful in reproducing the observed total and spectral irradiance, although further improvements are still possible.|
|Fulltext version:||Published version|
|License (according to publishing contract):||Licence according to publishing contract|
|Departement:||School of Engineering|
|Appears in collections:||Publikationen School of Engineering|
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Solanki, S. A., Krivova, N. A., & Wenzler, T. (2005). Irradiance models. Advances in Space Research, 35(3), 376–383. https://doi.org/10.1016/j.asr.2004.12.077
Solanki, S.A., Krivova, N.A. and Wenzler, T. (2005) ‘Irradiance models’, Advances in Space Research, 35(3), pp. 376–383. Available at: https://doi.org/10.1016/j.asr.2004.12.077.
S. A. Solanki, N. A. Krivova, and T. Wenzler, “Irradiance models,” Advances in Space Research, vol. 35, no. 3, pp. 376–383, 2005, doi: 10.1016/j.asr.2004.12.077.
Solanki, S. A., et al. “Irradiance Models.” Advances in Space Research, vol. 35, no. 3, 2005, pp. 376–83, https://doi.org/10.1016/j.asr.2004.12.077.
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