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Please use this identifier to cite or link to this item: https://doi.org/10.21256/zhaw-4713
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dc.contributor.authorWenzler, T.-
dc.contributor.authorSolanki, S. K.-
dc.contributor.authorKrivova, N. A.-
dc.date.accessioned2018-09-17T12:51:41Z-
dc.date.available2018-09-17T12:51:41Z-
dc.date.issued2005-
dc.identifier.issn0004-6361de_CH
dc.identifier.issn1432-0746de_CH
dc.identifier.urihttps://digitalcollection.zhaw.ch/handle/11475/10660-
dc.description.abstractTotal solar irradiance is reconstructed using data from the spectromagnetograph on Kitt Peak for 1992-2003 (covering parts of cycles 22 and 23) and compared with observational data. The model assumes that solar irradiance variations are caused by surface magnetism and its single free parameter is kept at the same value for both cycles. A good correspondence is found for the whole period of time, with no bias between the two cycles on time-scales longer than the solar rotation period. This is in agreement with the recent results of de Toma et al. (2004), but it is in contrast to the earlier analysis of de Toma et al. (2001), and suggests that the source of the irradiance variations is the same for cycles 22 and 23, namely the evolution of the magnetic flux at the solar surface.de_CH
dc.language.isoende_CH
dc.publisherEDP Sciencesde_CH
dc.relation.ispartofAstronomy & Astrophysicsde_CH
dc.rightsLicence according to publishing contractde_CH
dc.subjectSun: activityde_CH
dc.subjectSun: magnetic fieldsde_CH
dc.subjectSun: solar-terrestrial relationsde_CH
dc.subject.ddc500: Naturwissenschaftende_CH
dc.titleCan surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23?de_CH
dc.typeBeitrag in wissenschaftlicher Zeitschriftde_CH
dcterms.typeTextde_CH
zhaw.departementSchool of Engineeringde_CH
dc.identifier.doi10.21256/zhaw-4713-
dc.identifier.doi10.1051/0004-6361:20041956de_CH
zhaw.funding.euNode_CH
zhaw.issue3de_CH
zhaw.originated.zhawYesde_CH
zhaw.pages.end1061de_CH
zhaw.pages.start1057de_CH
zhaw.publication.statuspublishedVersionde_CH
zhaw.volume432de_CH
zhaw.publication.reviewPeer review (Publikation)de_CH
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Wenzler, T., Solanki, S. K., & Krivova, N. A. (2005). Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? Astronomy & Astrophysics, 432(3), 1057–1061. https://doi.org/10.21256/zhaw-4713
Wenzler, T., Solanki, S.K. and Krivova, N.A. (2005) ‘Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23?’, Astronomy & Astrophysics, 432(3), pp. 1057–1061. Available at: https://doi.org/10.21256/zhaw-4713.
T. Wenzler, S. K. Solanki, and N. A. Krivova, “Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23?,” Astronomy & Astrophysics, vol. 432, no. 3, pp. 1057–1061, 2005, doi: 10.21256/zhaw-4713.
WENZLER, T., S. K. SOLANKI und N. A. KRIVOVA, 2005. Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? Astronomy & Astrophysics. 2005. Bd. 432, Nr. 3, S. 1057–1061. DOI 10.21256/zhaw-4713
Wenzler, T., S. K. Solanki, and N. A. Krivova. 2005. “Can Surface Magnetic Fields Reproduce Solar Irradiance Variations in Cycles 22 and 23?” Astronomy & Astrophysics 432 (3): 1057–61. https://doi.org/10.21256/zhaw-4713.
Wenzler, T., et al. “Can Surface Magnetic Fields Reproduce Solar Irradiance Variations in Cycles 22 and 23?” Astronomy & Astrophysics, vol. 432, no. 3, 2005, pp. 1057–61, https://doi.org/10.21256/zhaw-4713.


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