Reconstruction of solar irradiance variations in cycles 21-23 based on surface magnetic fields

By T. Wenzler, S. Solanki, N. Krivova, C. Fröhlich. 2006

138 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c408f305b10c2988ec5bd05156790e82577a146f

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. S. Solanki
2. N. Krivova
3. C. Fröhlich
4. J. Haigh
5. K. L. Yeo
6. Karl-Heinz Glassmeier
7. I. Usoskin
8. L. Vieira

In Astronomy and Astrophysics

1. N. Krivova
2. S. Solanki
3. I. Usoskin
4. J. Haigh
5. M. Lockwood
6. C. Fröhlich
7. L. Vieira
8. Karl-Heinz Glassmeier

Citations in the corpus

• Solar Irradiance Variability Since 1978 (2007, methodology): “The close agreement with the reconstruction from the Kitt-Peak magnetograms by Wenzler (2005) and also with the 3-component proxy model shown by Fröhlich (2006) supports the PMOD composite as the most reliable representation of the solar irradiance variability during the last three solar cycles.”
• Evolution of the solar irradiance during the Holocene (2011, methodology): “The measured solar irradiance can be reproduced on the basis of the assumption that its variability is related to the evolution of the magnetic features lying on the solar surface (Krivova et al. 2003; Wenzler et al. 2006).”
• Evidence of a long-term trend in total solar irradiance (2009, unknown): “These models (e.g. Wenzler et al. 2006; Fröhlich 2009; Unruh et al. 2008) are based on contrast functions, area, and center-to-limb variations in the effect of the different magnetic elements involved and explain more than 80% of the variance on time scales from days to 11 years.”
• Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “Therefore the average ratio of umbral to sunspot area was determined for the period after 1992 and assumed to be the same over the earlier period (Wenzler et al. 2006).”
• Solar Irradiance Variability and Climate (2013, methodology): “With time, more physics-based models have been developed (e.g., Ermolli, Criscuoli & Giorgi 2011; Fligge, Solanki & Unruh 2000; Fontenla et al. 2011; Krivova et al. 2003; Shapiro et al. 2010; Wenzler et al. 2006).”
• Reconstruction of solar total irradiance since 1700 from the surface magnetic flux (2007, methodology): “For a reconstruction of solar irradiance in cycles 21– 23 based on National Solar Observatory Kitt Peak (NSO KP) data, Wenzler et al. (2005, 2006) found φsat = 310–320 G to be more adequate.”
• SOLAR INFLUENCES ON CLIMATE (2010, unknown): “The second uses solar magnetograms and the SATIRE irradiance modeling [Wenzler et al., 2006].”
• Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “This is the reason why we did not adopt either of the corrections to pre-1990 KP512 magnetograms proposed by Wenzler et al. (2006) and Ball et al. (2012) or subtract the zero level bias determined here from the magnetogram signal, leaving the KP512 magnetograms as they are for the solar irradiance…”