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dc.contributor.authorKrivova, N. A.-
dc.contributor.authorSolanki, S. K.-
dc.contributor.authorWenzler, T.-
dc.contributor.authorPodlipnik, B.-
dc.date.accessioned2018-09-17T12:44:25Z-
dc.date.available2018-09-17T12:44:25Z-
dc.date.issued2009-
dc.identifier.issn2169-897Xde_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/10652-
dc.description.abstractVariations of the solar UV irradiance are an important driver of chemical and physical processes in the Earth's upper atmosphere and may also influence global climate. Here we reconstruct solar UV irradiance in the range 115–400 nm over the period 1974–2007 by making use of the recently developed empirical extension of the Spectral And Total Irradiance Reconstruction (SATIRE) models employing Solar Ultraviolet Spectral Irradiance Monitor (SUSIM) data. The evolution of the solar photospheric magnetic flux, which is a central input to the model, is described by the magnetograms and continuum images recorded at the Kitt Peak National Solar Observatory between 1974 and 2003 and by the Michelson Doppler Imager instrument on SOHO since 1996. The reconstruction extends the available observational record by 1.5 solar cycles. The reconstructed Ly-α irradiance agrees well with the composite time series by Woods et al. (2000). The amplitude of the irradiance variations grows with decreasing wavelength and in the wavelength regions of special interest for studies of the Earth's climate (Ly-α and oxygen absorption continuum and bands between 130 and 350 nm) is 1–2 orders of magnitude stronger than in the visible or if integrated over all wavelengths (total solar irradiance). de_CH
dc.language.isoende_CH
dc.publisherWileyde_CH
dc.relation.ispartofJournal of Geophysical Research: Atmospheresde_CH
dc.rightsLicence according to publishing contractde_CH
dc.subject.ddc500: Naturwissenschaftende_CH
dc.titleReconstruction of solar UV irradiance since 1974de_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementSchool of Engineeringde_CH
dc.identifier.doi10.1029/2009JD012375de_CH
zhaw.funding.euNode_CH
zhaw.issueD1/D00I04de_CH
zhaw.originated.zhawYesde_CH
zhaw.publication.statuspublishedVersionde_CH
zhaw.volume114de_CH
zhaw.publication.reviewPeer review (Publikation)de_CH
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Krivova, N. A., Solanki, S. K., Wenzler, T., & Podlipnik, B. (2009). Reconstruction of solar UV irradiance since 1974. Journal of Geophysical Research: Atmospheres, 114(D1/D00I04). https://doi.org/10.1029/2009JD012375
Krivova, N.A. et al. (2009) ‘Reconstruction of solar UV irradiance since 1974’, Journal of Geophysical Research: Atmospheres, 114(D1/D00I04). Available at: https://doi.org/10.1029/2009JD012375.
N. A. Krivova, S. K. Solanki, T. Wenzler, and B. Podlipnik, “Reconstruction of solar UV irradiance since 1974,” Journal of Geophysical Research: Atmospheres, vol. 114, no. D1/D00I04, 2009, doi: 10.1029/2009JD012375.
KRIVOVA, N. A., S. K. SOLANKI, T. WENZLER und B. PODLIPNIK, 2009. Reconstruction of solar UV irradiance since 1974. Journal of Geophysical Research: Atmospheres. 2009. Bd. 114, Nr. D1/D00I04. DOI 10.1029/2009JD012375
Krivova, N. A., S. K. Solanki, T. Wenzler, and B. Podlipnik. 2009. “Reconstruction of Solar UV Irradiance since 1974.” Journal of Geophysical Research: Atmospheres 114 (D1/D00I04). https://doi.org/10.1029/2009JD012375.
Krivova, N. A., et al. “Reconstruction of Solar UV Irradiance since 1974.” Journal of Geophysical Research: Atmospheres, vol. 114, no. D1/D00I04, 2009, https://doi.org/10.1029/2009JD012375.


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