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https://doi.org/10.21256/zhaw-4713| Publikationstyp: | Beitrag in wissenschaftlicher Zeitschrift |
| Art der Begutachtung: | Peer review (Publikation) |
| Titel: | Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? |
| Autor/-in: | Wenzler, T. Solanki, S. K. Krivova, N. A. |
| DOI: | 10.21256/zhaw-4713 10.1051/0004-6361:20041956 |
| Erschienen in: | Astronomy & Astrophysics |
| Band(Heft): | 432 |
| Heft: | 3 |
| Seite(n): | 1057 |
| Seiten bis: | 1061 |
| Erscheinungsdatum: | 2005 |
| Verlag / Hrsg. Institution: | EDP Sciences |
| ISSN: | 0004-6361 1432-0746 |
| Sprache: | Englisch |
| Schlagwörter: | Sun: activity; Sun: magnetic fields; Sun: solar-terrestrial relations |
| Fachgebiet (DDC): | 500: Naturwissenschaften |
| Zusammenfassung: | Total 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. |
| URI: | https://digitalcollection.zhaw.ch/handle/11475/10660 |
| Volltext Version: | Publizierte Version |
| Lizenz (gemäss Verlagsvertrag): | Lizenz gemäss Verlagsvertrag |
| Departement: | School of Engineering |
| Enthalten in den Sammlungen: | Publikationen School of Engineering |
Dateien zu dieser Ressource:
| Datei | Beschreibung | Größe | Format | |
|---|---|---|---|---|
| 2005_Wenzel_Can_surface_magnetic_fields_reproduce_solar_irradiance_variations.pdf | 678.7 kB | Adobe PDF |  Öffnen/Anzeigen |
Zur Langanzeige
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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