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dc.contributor.authorSolanki, S. A.-
dc.contributor.authorKrivova, N. A.-
dc.contributor.authorWenzler, T.-
dc.date.accessioned2018-09-17T12:51:05Z-
dc.date.available2018-09-17T12:51:05Z-
dc.date.issued2005-
dc.identifier.issn0273-1177de_CH
dc.identifier.issn1879-1948de_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/10659-
dc.description.abstractMeasurements 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.isoende_CH
dc.publisherElsevierde_CH
dc.relation.ispartofAdvances in Space Researchde_CH
dc.rightsLicence according to publishing contractde_CH
dc.subjectSolar magnetic fieldde_CH
dc.subjectSolar–terrestrial relationsde_CH
dc.subjectSolar activityde_CH
dc.subjectSolar irradiancede_CH
dc.subject.ddc500: Naturwissenschaften und Mathematikde_CH
dc.titleIrradiance modelsde_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementSchool of Engineeringde_CH
dc.identifier.doi10.1016/j.asr.2004.12.077de_CH
zhaw.funding.euNode_CH
zhaw.issue3de_CH
zhaw.originated.zhawYesde_CH
zhaw.pages.end383de_CH
zhaw.pages.start376de_CH
zhaw.publication.statuspublishedVersionde_CH
zhaw.volume35de_CH
zhaw.publication.reviewPeer review (Publikation)de_CH
Appears in Collections:Publikationen School of Engineering

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