Solar activity during the last 1000 yr inferred from radionuclide records

By Raimund Muschelera, Fortunat Joosb, Jürg Beerc, Simon A. Müllerb, Maura Vonmoosc, Ian Snowballd. 2007

343 citations recorded by the source corpus.

Subfields: Atmospheric Science, Molecular Biology, Paleontology

View Paper: https://www.semanticscholar.org/paper/b2837cd7e4f95143ce881512ed8fbee80eeedfa6

How researchers see this paper

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

In Atmospheric Science

1. I. Usoskin
2. Catherine Constable
3. Monika Korte
4. G. Kovaltsov
5. G. Hulot
6. S. Solanki
7. Y. Gallet
8. M. Lockwood

In Molecular Biology

1. I. Usoskin
2. G. Kovaltsov
3. S. Solanki
4. M. Lockwood
5. N. Krivova
6. Catherine Constable
7. Monika Korte
8. G. Hulot

In Paleontology

1. Hans Renssen
2. Hugues Goosse
3. I. Usoskin
4. G. Kovaltsov

Citations in the corpus

• A new approach to the long-term reconstruction of the solar irradiance leads to large historical solar forcing (2011, methodology): “In additional to the10Be-based data of solar activity there are several14C-based datasets (e.g., Solanki et al. 2004; Vonmoos et al. 2006; Muscheler et al. 2007; Usoskin 2008).”
• Evolution of the solar irradiance during the Holocene (2011, methodology): “This approach, proposed Usoskin et al. (2003, 2004), is now a standard method used to reconstruct of the solar or heliospheric parameters in the past (e.g. Solanki et al. 2004; Usoskin et al. 2006a, 2007; Vonmoos et al. 2006; Muscheler et al. 2007; Steinhilber et al. 2008).”
• The Heliospheric Magnetic Field (2013, methodology): “…averages of OSF inferred from heliospheric modulation potentials consistent with the 10Be and 14C abundances, respectively, since 1610 and extended to the space age using neutron monitor records (see Muscheler et al., 2007; Lockwood and Fröhlich, 2008, and references therein for more detail).”
• Meridional transport and deposition of atmospheric 10 Be (2008, background): “Therefore, so far a rather well mixed atmosphere has been assumed for solar activity reconstructions based on 10Be from polar regions (McCracken et al., 2004a; Muscheler et al., 2007; Vonmoos et al., 2006).”
• SOLAR INFLUENCES ON CLIMATE (2010, neutral): “…(e.g., 208 year DeVries or Suess cycle, 2300 year Hallstatt cycle, and others) and also the present relatively high level of solar activity, although there is some controversy as to how unusually high it really is [Muscheler et al., 2007; Usoskin et al., 2004; Steinhilber et al., 2008].”
• An Antarctic view of Beryllium-10 and solar activity for the past millennium (2011, result): “More specifically, compared to the reconstructions by Muscheler et al. (2005) and Muscheler et al. (2007), based on 14C and 10Be records, our reconstruction has a much lower variability and lower maxima values.”
• Solar activity during the Holocene: the Hallstatt cycle and its consequence for grand minima and maxima (2016, background): “Recently, several longterm solar activity reconstructions have been published (e.g., Solanki et al. 2004; Vonmoos et al. 2006; Muscheler et al. 2007; Usoskin et al. 2007; Steinhilber et al. 2012).”
• Solar Influence on Global and Regional Climates (2012, background): “A long-standing suggestion is that cosmic rays can aid the formation of clouds (see reviews by Ney 1959; Carslaw et al. 2002; Kirkby 2007).”
• Temperature response in the Altai region lags solar forcing (2009, methodology): “(a) Solar activity proxies (group sunspot number period 1610-2000 (blue dashed) and solar modulation inferred from 1°Be (grey) and 14C (green) [Muscheler et al., 2007]) together with the Belukha temperature reconstruction (red).”
• Description of the Earth system model of intermediate complexity LOVECLIM version 1.2 (2010, methodology): “Finally, natural external forcing due to changes in solar irradiance and explosive volcanism are prescribed following the reconstructions of Muscheler et al. (2007) and Crowley et al. (2003), respectively.”
• Improving geomagnetic field reconstructions for 0–3 ka (2011, background): “…jerks (Gallet et al., 2009), geo-18 magnetic shielding for cosmic rays and cosmogenic isotope production for various kinds19 of studies (e.g. Usoskin et al., 2006; Muscheler et al., 2007; Usoskin et al., 2008; Lifton20 et al., 2008), to data assimilation for geodynamo models (Kuang et al., 2008).”
• A History of Solar Activity over Millennia (2008, methodology): “Reconstructions of solar activity often end at this point, representing solar activity by the modulation potential, as some authors (e.g., Beer et al., 2003; Vonmoos et al., 2006; Muscheler et al., 2007) believe that further steps (see subsection 3.”