Reconstruction of solar total irradiance since 1700 from the surface magnetic flux

By N. Krivova, L. Balmaceda, S. Solanki. 2007

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Subfields: Astronomy and Astrophysics, Molecular Biology, Oceanography

View Paper: https://www.semanticscholar.org/paper/c37a2e58c6cafa9091551e6f5ecd72f470d7b577

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Citations in the corpus

Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “The different versions of the model differ by the data used to deduce the surface coverage of sunspots and faculae (see Krivova et al. 2007, 2011b; Vieira et al. 2011).”
The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets (2015, methodology): “Finally, Vieira et al. (2011) adapted the models by Solanki et al. (2002) and Krivova et al. (2007) for use with 14 C data (red colour tones).”
Solar change and climate: an update in the light of the current exceptional solar minimum (2010, methodology): “To do this, Krivova et al. (2007) had to effectively relate facular occurrence to sunspots, constrained by the open solar ﬂux.”
A History of Solar Activity over Millennia (2008, background): “For example, the time evolution of the total (or open) solar magnetic flux is extensively debated (e.g., Lockwood et al., 1999; Wang et al., 2005; Krivova et al., 2007).”
Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “In contrast to the Kitt-Peak reconstruction the Krivova et al. (2007) one does not reproduce the details of the intra-cycle variability properly, because it is focused on the long-term variations back to the 17th century.”
Solar activity during the Holocene: the Hallstatt cycle and its consequence for grand minima and maxima (2016, methodology): “This modulation potential was furthermore converted into decadal (solar-cycle averaged) sunspot number through the open solar magnetic flux model (Solanki et al. 2000; Krivova et al. 2007), which relates the solar surface magnetic cycle to the emerging magnetic flux (Cameron & Schüssler 2015).”
Climate and carbon-cycle variability over the last millennium (2010, background): “The data set has daily sampling from 1627 AD onward (Krivova et al., 2007; Balmaceda et al., 2007).”
Evidence of a long-term trend in total solar irradiance (2009, unknown): “Both Wang et al. (2005) and Krivova et al. (2007) use either the total photospheric magnetic field or the sum of the open field and the fields from the ephemeral regions for the secular change and determine it in the same way as for the intra-cycle variability.”
The Heliospheric Magnetic Field (2013, background): “One approach is to assume various OSF contributions decay with different timescales (Krivova et al., 2007; Vieira and Solanki, 2010).”
A new approach to the long-term reconstruction of the solar irradiance leads to large historical solar forcing (2011, background): “Recent reconstructions based on the magnetic field surface distribution (Wang et al. 2005; Krivova et al. 2007) and on extrapolation of the assumed correlation between TSI and the open magnetic flux (Lockwood et al. 1999) during the last three minima (Steinhilber et al. 2009; Fröhlich 2009)…”
SOLAR INFLUENCES ON CLIMATE (2010, unknown): “on multidecadal to centennial time scales [Krivova et al., 2007], for example, to what extent TSI and SSI are reduced during the Maunder Minimum, although estimates have converged somewhat in recent years.”
Are there connections between the Earth's magnetic field and climate? (2007, methodology): “The total solar irradiance curve based on sunspot data S(t) is an update of Solanki (2002) by Krivova et al. (2007).”
Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, methodology): “…time scales, with the PMOD TSI composite (Wenzler et al., 2009; Ball et al., 2012), SORCE/TIM TSI measurements (Ball et al., 2011, 2012), UARS/SUSIM spectral irradiance (Krivova et al., 2006, 2009; Unruh et al., 2012), as well1170 as with UARS/SUSIM and UARS/SOLSTICE Ly-α mea- surements (Figs.”
Evolution of the solar irradiance during the Holocene (2011, methodology): “Most of these models are based on the records of sunspot number, which are available since approximately 1610 AD (e.g., SATIRE-T, Balmaceda 2007; Krivova et al. 2007, 2010a; and other models, Lean et al. 1995; Solanki & Fligge 1999; Wang et al. 2005; Tapping et al. 2007; Crouch et al. 2008), but…”