Evolution of the Sun's Spectral Irradiance Since the Maunder Minimum

By J. Lean. 2000

644 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/6c467d941db0b4b5e433deb8422fb614a0f7f386

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In Astronomy and Astrophysics

Citations in the corpus

Solar Forcing for CMIP6 (v3.1) (2016, methodology): “A special focus lies on the comparison of the new CMIP6 dataset with its predecessor NRLSSI1(CMIP5).”
A reconstruction of radiocarbon production and total solar irradiance from the Holocene 14 C and CO 2 records: implications of data and model uncertainties (2013, background): “This is also reflected in the large spread in past and recent reconstructions of TSI variability on multi-decadal to centennial timescales (e.g.Bard et al., 2000; Lean, 2000; Wang et al., 2005; Steinhilber et al., 2009; Steinhilber et al., 2012; Shapiro et al., 2011; Schrijver et al., 2011).”
SOLAR INFLUENCES ON CLIMATE (2010, neutral): “…et al., 2007]; the solar rotation and diameter [Nesme‐Ribes et al., 1993; Mendoza, 1997]; a combination of R and its 11 year running mean, R11 [e.g., Lean, 2000a, 2000b], or a combination of R and L [e.g., Solanki and Fligge, 2000]; sunspot group areas [Fligge and Solanki, 1998]; Greenwich sunspot…”
Coupled climate model simulation of Holocene cooling events: oceanic feedback amplifies solar forcing (2006, neutral): “%) based on Lean (2000).”
Solar Influence on Global and Regional Climates (2012, background): “…of observed UV spectral solar irradiance (SSI) had shown little variation in the spectral shape, such that at all wavelengths they exhibit similar temporal variations to TSI (Lean et al. 1997), and this has been reﬂected in centennial reconstructions of SSI (Lean 2000; Krivova et al. 2009).”
Modeling the Sun’s Magnetic Field and Irradiance since 1713 (2005, methodology): “3 in Lean 2000).”
Total solar irradiance during the Holocene (2009, result): “This is smaller by a factor of 2–4 compared to records [Lean et al., 1995; Lean, 2000] that have been used in climate model studies.”
Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “Either the PF and PS time series are regressed together against the observed irradiance, S or F(λ), or the observations are first corrected for sunspot effects then the residual time series, S −PS or F(λ)−PS(λ), is linearly regressed against PF (Lean et al. 1997; Fröhlich and Lean 1998a; Lean 2000).”
Cycles and trends in solar irradiance and climate (2010, neutral): “1362.0 Reconstructed total solar irradiance 1361.5 1361.0 1360.5 W m −2 1360.0 1359.5 1359.0 1358.5 200 Lean, 2000 Sunspot numbers Maunder minimum Dalton minimum Modern maximum Tapping et al, 2007 Wang, Lean, Sheeley, 2005 150 100 50 0 1700 Cosmogenic isotopes Time (years) −5000 −10 −5 0 5 10 15 20…”
Efficacy of climate forcings (2005, background): “Solar irradiance change has a strong spectral dependence [Lean, 2000], and resulting climate changes may include indirect effects of induced ozone change [RFCR; Haigh, 1999; Shindell et al.”
Solar Irradiance Variability and Climate (2013, methodology): “16(a), but for the difference between solar cycle maximum and minimum conditions, based on spectral variability of Lean (2000) (see Sect.”
Solar cycle signals in sea level pressure and sea surface temperature (2010, methodology): “Any strong signal in SSTs would likely also be seen in near surface air temperature but two independent studies (Stott and Jones, 2009), using an optimal detection technique, and Lean and Rind (2008), using multiple regression analysis) both show very little solar signal in the tropics on centennial”