1. ZHAW digitalcollection
  2. School of Engineering
  3. Publikationen
  4. Publikationen School of Engineering
Full metadata record
DC FieldValueLanguage
dc.contributor.authorHaberreiter, M.-
dc.contributor.authorKrivova, N. A.-
dc.contributor.authorSchmutz, W.-
dc.contributor.authorWenzler, T.-
dc.date.accessioned2018-09-17T12:50:29Z-
dc.date.available2018-09-17T12:50:29Z-
dc.date.issued2005-
dc.identifier.issn0273-1177de_CH
dc.identifier.issn1879-1948de_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/10658-
dc.description.abstractThe variability of the solar UV irradiance has strong effects on the terrestrial atmosphere. In order to study the solar influence for times when no UV observations are available, it is necessary to reconstruct the variation of the UV irradiance with time on the basis of proxies. We present reconstructions of the solar UV irradiance based on the analysis of space-based and ground-based magnetograms of the solar disk going back to 1974. With COde for Solar Irradiance (COSI) we calculate solar intensity spectra for the quiet Sun and different active regions and combine them according to their fractional area on the solar disk, whereby their time-dependent contributions over the solar cycle lead to a variability in radiation. COSI calculates the continuum and line formation under conditions which are out of local thermodynamic equilibrium (non-LTE). The applied temperature and density structures include the chromosphere and transition region, which is particularly important for the UV. The reconstructions are compared with observations.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 UV spectrumde_CH
dc.subjectRadiative transfer modelde_CH
dc.subjectSolar activityde_CH
dc.subjectNon-LTEde_CH
dc.subject.ddc500: Naturwissenschaftende_CH
dc.titleReconstruction of the solar UV irradiance back to 1974de_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementSchool of Engineeringde_CH
dc.identifier.doi10.1016/j.asr.2005.04.039de_CH
zhaw.funding.euNode_CH
zhaw.issue3de_CH
zhaw.originated.zhawYesde_CH
zhaw.pages.end369de_CH
zhaw.pages.start365de_CH
zhaw.publication.statuspublishedVersionde_CH
zhaw.volume35de_CH
zhaw.publication.reviewPeer 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
Haberreiter, M., Krivova, N. A., Schmutz, W., & Wenzler, T. (2005). Reconstruction of the solar UV irradiance back to 1974. Advances in Space Research, 35(3), 365–369. https://doi.org/10.1016/j.asr.2005.04.039
Haberreiter, M. et al. (2005) ‘Reconstruction of the solar UV irradiance back to 1974’, Advances in Space Research, 35(3), pp. 365–369. Available at: https://doi.org/10.1016/j.asr.2005.04.039.
M. Haberreiter, N. A. Krivova, W. Schmutz, and T. Wenzler, “Reconstruction of the solar UV irradiance back to 1974,” Advances in Space Research, vol. 35, no. 3, pp. 365–369, 2005, doi: 10.1016/j.asr.2005.04.039.
HABERREITER, M., N. A. KRIVOVA, W. SCHMUTZ und T. WENZLER, 2005. Reconstruction of the solar UV irradiance back to 1974. Advances in Space Research. 2005. Bd. 35, Nr. 3, S. 365–369. DOI 10.1016/j.asr.2005.04.039
Haberreiter, M., N. A. Krivova, W. Schmutz, and T. Wenzler. 2005. “Reconstruction of the Solar UV Irradiance back to 1974.” Advances in Space Research 35 (3): 365–69. https://doi.org/10.1016/j.asr.2005.04.039.
Haberreiter, M., et al. “Reconstruction of the Solar UV Irradiance back to 1974.” Advances in Space Research, vol. 35, no. 3, 2005, pp. 365–69, https://doi.org/10.1016/j.asr.2005.04.039.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.