Total solar irradiance during the Holocene
By F. Steinhilber, J. Beer, C. Fröhlich. 2009
915 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/aa02c3246dee6d17a76d4e37165a473604242077
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Citations in the corpus
- How will sea level respond to changes in natural and anthropogenic forcings by 2100? (2010, background): “[23] Alternative scenarios for solar forcing with a potential decrease in solar irradiance of 1W/m2 (using the lowest level recorded throughout the last 9300 years) only produce a 10–20 cm reduction in our estimate of 21st century sea level rise.”
- The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets (2015, methodology): “Steinhilber et al. (2009) first estimated the interplanetary magnetic field from the 10 Be data and then used a linear regression with the measured TSI following Fröhlich (2009).”
- 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, methodology): “Solar activity in our decadally smoothed record is during 28 % of the time higher than the modern average of 650 MeV and during 39 % of the time higher than 600 MeV, used to define periods of high activity by Steinhilber et al.(2008) (Fig.”
- Are cold winters in Europe associated with low solar activity? (2010, methodology): “Figure 1 shows that F S is highly anticorrelated with cosmic ray fluxes and also correlates very well (with a lag of 1 year) with total solar irradiance (TSI).”
- European summer temperatures since Roman times (2016, neutral): “Planet .”
- 9,400 years of cosmic radiation and solar activity from ice cores and tree rings (2012, methodology): “Figure S19 Comparison of TSI of this study with SEA09 (19).”
- SOLAR INFLUENCES ON CLIMATE (2010, neutral): “…sunspot maps [Lockwood, 2004]; p mode amplitudes (estimated from R) [Bhatnagar et al., 2002]; cosmogenic isotopes deposited in terrestrial reservoirs [Bard et al., 2000; Steinhilber et al., 2009]; and the open magnetic flux of the Sun derived from geomagnetic activity data [Lockwood, 2002].”
- A History of Solar Activity over Millennia (2008, background): “As very important for the climate research, the variations of the total solar irradiance (TSI) are sometimes reconstructed from the solar proxy data (Steinhilber et al., 2009; Vieira et al., 2011).”
- Evolution of the solar irradiance during the Holocene (2011, methodology): “Near the end of the Maunder Minimum, the difference is approximately 0.5 W/m2 if we require the TSI reconstruction by Steinhilber et al. (2009) to match the present value of the TSI.”
- A new, lower value of total solar irradiance: Evidence and climate significance (2011, methodology): “…of solar signals in climate records [Douglass and Clader, 2002; Lean and Rind, 2009], estimates of irradiance changes during the past millennium [Steinhilber et al., 2009], climate model assessments [Tung et al., 2008], and climate change simulations including those used by IPCC [2007].”
- Solar Influence on Global and Regional Climates (2012, background): “To allow studies of the remaining effect, solar variability, studies have corrected the cosmogenic isotope record to allow for the secular geomagnetic variations (e.g., Steinhilber et al. 2008, 2009).”
- A new approach to the long-term reconstruction of the solar irradiance leads to large historical solar forcing (2011, background): “…(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) resulted in a low solar forcing value within the range∆FP−M ≈ 0.1–0.2 W/m2.”