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dc.contributor.authorKrivova, N. A.-
dc.contributor.authorSolanki, S. A.-
dc.contributor.authorWenzler, T.-
dc.date.accessioned2018-09-17T12:41:14Z-
dc.date.available2018-09-17T12:41:14Z-
dc.date.issued2009-
dc.identifier.issn0094-8276de_CH
dc.identifier.issn1944-8007de_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/10648-
dc.description.abstractA gap in the total solar irradiance (TSI) measurements between ACRIM-1 and ACRIM-2 led to the ongoing debate on the presence or not of a secular trend between the minima preceding cycles 22 (in 1986) and 23 (1996). It was recently proposed to use the SATIRE model of solar irradiance variations to bridge this gap. When doing this, it is important to use the appropriate SATIRE-based reconstruction, which we do here, employing a reconstruction based on magnetograms. The accuracy of this model on months to years timescales is significantly higher than that of a model developed for long-term reconstructions used by the ACRIM team for such an analysis. The constructed `mixed' ACRIM - SATIRE composite shows no increase in the TSI from 1986 to 1996, in contrast to the ACRIM TSI composite. de_CH
dc.language.isoende_CH
dc.publisherWileyde_CH
dc.relation.ispartofGeophysical research lettersde_CH
dc.rightsLicence according to publishing contractde_CH
dc.subject.ddc500: Naturwissenschaften und Mathematikde_CH
dc.titleACRIM-gap and total solar irradiance revisited : is there a secular trend between 1986 and 1996?de_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementSchool of Engineeringde_CH
dc.identifier.doi10.1029/2009GL040707de_CH
zhaw.funding.euNode_CH
zhaw.issue20/L20101de_CH
zhaw.originated.zhawYesde_CH
zhaw.publication.statuspublishedVersionde_CH
zhaw.volume36de_CH
zhaw.publication.reviewPeer review (Publikation)de_CH
Appears in Collections:Publikationen School of Engineering

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