Observations of Irradiance Variations

By C. Fröhlich. 2000

159 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Artificial Intelligence, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/5db5490e1961beb808094becee496ff7bec1b535

How researchers see this paper

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

In Aerospace Engineering

1. S. Solanki
2. N. Krivova
3. T. Wenzler
4. Paulina Jofré
5. A. Korn
6. C. Soubiran
7. F. Th'evenin
8. B. Gustafsson

In Artificial Intelligence

1. S. Solanki
2. N. Krivova
3. C. Fröhlich
4. K. L. Yeo
5. Karl-Heinz Glassmeier
6. J. Lean
7. W. Schmutz
8. Paulina Jofré

In Atmospheric Science

1. S. Solanki
2. N. Krivova
3. J. Lean
4. Greg Kopp
5. K. L. Yeo
6. Karl-Heinz Glassmeier
7. C. Soubiran
8. U. Heiter

Citations in the corpus

• Evidence of a long-term trend in total solar irradiance (2009, unknown): “A detailed reanalysis of the HF long-term behaviour by Fröhlich (2000, 2006) and comparison with ERBE data and the Kitt-Peak reconstruction (Wenzler et al. 2006) confirm the need of the correction of HF.”
• Reconstruction of solar irradiance variations in cycles 21-23 based on surface magnetic fields (2006, methodology): “Total solar irradiance reconstructions based on NSO-512 and NSO-SPM data are compared with the newest PMOD composite of TSI (version 41) from the Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center (PMOD/WRC) in Switzerland (Fröhlich 2000, 2003b, 2006), which is compiled from mu”
• Solar radiative output and its variability: evidence and mechanisms (2004, background): “Fröhlich and Lean (1998b,a) and Fröhlich (2000, 2003) provide a detailed description of the corrections, summarized as follows.”
• Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, background): “There are at present three composites published in the literature: ACRIM (Willson & Mordvinov 2003), IRMB (Dewitte et al. 2004b; Mekaoui & Dewitte 2008) and PMOD (Fröhlich 2000).”
• Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, methodology): “4.1 and 22 The adopted TSI value is about 0.4% or 5 Wm−2 lower than even earlier TSI measurements with different instruments (e.g. Fröhlich 2000), resulting in a downward revision of 0.1% or about 6 K from the previously used canonical value of 5777 K for the solar Teff .”
• Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “A detailed re-analysis of the HF long-term behaviour by Fröhlich (2000, 2006) and comparison with ERBE data and the Kitt-Peak reconstruction (Wenzler et al. 2006) confirm the need for a correction of HF.”