Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Solanki, S. A. | - |
| dc.contributor.author | Krivova, N. A. | - |
| dc.contributor.author | Wenzler, T. | - |
| dc.date.accessioned | 2018-09-17T12:51:05Z | - |
| dc.date.available | 2018-09-17T12:51:05Z | - |
| dc.date.issued | 2005 | - |
| dc.identifier.issn | 0273-1177 | de_CH |
| dc.identifier.issn | 1879-1948 | de_CH |
| dc.identifier.uri | https://digitalcollection.zhaw.ch/handle/11475/10659 | - |
| dc.description.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. | de_CH |
| dc.language.iso | en | de_CH |
| dc.publisher | Elsevier | de_CH |
| dc.relation.ispartof | Advances in Space Research | de_CH |
| dc.rights | Licence according to publishing contract | de_CH |
| dc.subject | Solar magnetic field | de_CH |
| dc.subject | Solar–terrestrial relations | de_CH |
| dc.subject | Solar activity | de_CH |
| dc.subject | Solar irradiance | de_CH |
| dc.subject.ddc | 500: Naturwissenschaften | de_CH |
| dc.title | Irradiance models | de_CH |
| dc.type | Beitrag in wissenschaftlicher Zeitschrift | de_CH |
| dcterms.type | Text | de_CH |
| zhaw.departement | School of Engineering | de_CH |
| dc.identifier.doi | 10.1016/j.asr.2004.12.077 | de_CH |
| zhaw.funding.eu | No | de_CH |
| zhaw.issue | 3 | de_CH |
| zhaw.originated.zhaw | Yes | de_CH |
| zhaw.pages.end | 383 | de_CH |
| zhaw.pages.start | 376 | de_CH |
| zhaw.publication.status | publishedVersion | de_CH |
| zhaw.volume | 35 | de_CH |
| zhaw.publication.review | Peer review (Publikation) | de_CH |
| Appears in collections: | Publikationen School of Engineering | |
Files in This Item:
There are no files associated with this item.
Show simple item record
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., N. A. KRIVOVA und T. WENZLER, 2005. Irradiance models. Advances in Space Research. 2005. Bd. 35, Nr. 3, S. 376–383. DOI 10.1016/j.asr.2004.12.077
Solanki, S. A., N. A. Krivova, and T. Wenzler. 2005. “Irradiance Models.” Advances in Space Research 35 (3): 376–83. https://doi.org/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.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.