Please use this identifier to cite or link to this item:
https://doi.org/10.21256/zhaw-4710Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Wenzler, T. | - |
| dc.contributor.author | Solanki, S. K. | - |
| dc.contributor.author | Krivova, N. A. | - |
| dc.contributor.author | Fluri, D. M. | - |
| dc.date.accessioned | 2018-09-17T12:46:05Z | - |
| dc.date.available | 2018-09-17T12:46:05Z | - |
| dc.date.issued | 2004 | - |
| dc.identifier.issn | 0004-6361 | de_CH |
| dc.identifier.issn | 1432-0746 | de_CH |
| dc.identifier.uri | https://digitalcollection.zhaw.ch/handle/11475/10654 | - |
| dc.description | All A&A articles are in open access one year after their publication date (August 2013). | de_CH |
| dc.description.abstract | To be able to use both space- and ground-based solar magnetograms and construct long time series of derived parameters it is important to cross-calibrate them so that we can estimate their reliability and combine them. Using two different techniques, we compare magnetograms as well as continuum images recorded by the Spectropolarimeter (SPM) on Kitt Peak and the Michelson Doppler Interferometer (MDI) on board SoHO.We find that the result obtained depends on the method used. The method we favour gives almost identical umbral and penumbral areas and very similar total magnetic fluxes in faculae. The magnetic fluxes in umbrae and penumbrae returned by the two instruments, however, differ considerably. We also demonstrate that SPM data can be employed to reconstruct total solar irradiance variations with almost the same accuracy as recently shown for MDI data. | de_CH |
| dc.language.iso | en | de_CH |
| dc.publisher | EDP Sciences | de_CH |
| dc.relation.ispartof | Astronomy & Astrophysics | de_CH |
| dc.rights | Licence according to publishing contract | de_CH |
| dc.subject | Sun: activity | de_CH |
| dc.subject | Methods: data analysis | de_CH |
| dc.subject | Sun: solar-terrestrial relations | de_CH |
| dc.subject | Sun: faculae, plages | de_CH |
| dc.subject.ddc | 500: Naturwissenschaften | de_CH |
| dc.title | Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions | de_CH |
| dc.type | Beitrag in wissenschaftlicher Zeitschrift | de_CH |
| dcterms.type | Text | de_CH |
| zhaw.departement | School of Engineering | de_CH |
| dc.identifier.doi | 10.21256/zhaw-4710 | - |
| dc.identifier.doi | 10.1051/0004-6361:20041313 | de_CH |
| zhaw.funding.eu | No | de_CH |
| zhaw.issue | 3 | de_CH |
| zhaw.originated.zhaw | Yes | de_CH |
| zhaw.pages.end | 1043 | de_CH |
| zhaw.pages.start | 1031 | de_CH |
| zhaw.publication.status | publishedVersion | de_CH |
| zhaw.volume | 427 | de_CH |
| zhaw.publication.review | Peer review (Publikation) | de_CH |
| Appears in collections: | Publikationen School of Engineering | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 2004_Wenzler_Comparison_between_KPVT_SPM_and_SoHO_MDI_magnetograms.pdf | 1.76 MB | Adobe PDF |  View/Open |
Show simple item record
Wenzler, T., Solanki, S. K., Krivova, N. A., & Fluri, D. M. (2004). Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions. Astronomy & Astrophysics, 427(3), 1031–1043. https://doi.org/10.21256/zhaw-4710
Wenzler, T. et al. (2004) ‘Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions’, Astronomy & Astrophysics, 427(3), pp. 1031–1043. Available at: https://doi.org/10.21256/zhaw-4710.
T. Wenzler, S. K. Solanki, N. A. Krivova, and D. M. Fluri, “Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions,” Astronomy & Astrophysics, vol. 427, no. 3, pp. 1031–1043, 2004, doi: 10.21256/zhaw-4710.
WENZLER, T., S. K. SOLANKI, N. A. KRIVOVA und D. M. FLURI, 2004. Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions. Astronomy & Astrophysics. 2004. Bd. 427, Nr. 3, S. 1031–1043. DOI 10.21256/zhaw-4710
Wenzler, T., S. K. Solanki, N. A. Krivova, and D. M. Fluri. 2004. “Comparison between KPVT/SPM and SoHO/MDI Magnetograms with an Application to Solar Irradiance Reconstructions.” Astronomy & Astrophysics 427 (3): 1031–43. https://doi.org/10.21256/zhaw-4710.
Wenzler, T., et al. “Comparison between KPVT/SPM and SoHO/MDI Magnetograms with an Application to Solar Irradiance Reconstructions.” Astronomy & Astrophysics, vol. 427, no. 3, 2004, pp. 1031–43, https://doi.org/10.21256/zhaw-4710.
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