Large variations in Holocene solar activity: Constraints from 10Be in the Greenland Ice Core Project ice core
By M. Vonmoos, J. Beer, R. Muscheler. 2006
280 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/4eb6462584f5257fea3628d89d0dd321446347a5
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Citations in the corpus
- A History of Solar Activity over Millennia (2008, unknown): “The modern approach is based on a physics-based model (e.g., Solanki et al., 2004; Vonmoos et al., 2006) and allows the quantitative reconstruction of solar activity, explicitly using independent reconstructions of the geomagnetic field.”
- The AD775 cosmic event revisited: the Sun is to blame (2013, methodology): “Using the above scenario, we calculated the expected increase in 10Be by applying the production model of Kovaltsov & Usoskin (2010) and assuming an instant injection and intermediate atmospheric mixing of 10Be (McCracken 2004; Vonmoos et al. 2006).”
- 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).”
- A History of Solar Activity over Millennia (2008, methodology): “The modern approach is based on a physics-based model (e.g., Solanki et al., 2004; Vonmoos et al., 2006) and allows the quantitative reconstruction of solar activity, explicitly using independent reconstructions of the geomagnetic field.”
- An updated simulation of particle fluxes and cosmogenic nuclide production in the Earth's atmosphere (2009, background): “These results provide the basis for a quantitative reconstruction of the history of the solar activity and the geomagnetic field intensity using records of cosmogenic isotopes in natural archives such as sediments and ice cores [Vonmoos et al., 2006; Muscheler et al., 2005].”
- Dynamics of the Earth’s Particle Radiation Environment (2009, methodology): “…a set of reconstructions of the modulation potential since 1700 AD, including a model computation (Usoskin et al. 2002b) from sunspot numbers and reconstructions from cosmogenic isotopes 14C (Usoskin et al. 2006, 2007) and 10Be in polar ice cores (McCracken et al. 2004; Vonmoos et al. 2006).”
- The Solar Cycle (2007, background): “Although the variations in the calculated production rates of (14)C and (10)Be are well correlated with each other (Vonmoos et al., 2006) and with the 400-year sunspot record (Berggren et al.”
- Coupled climate model simulation of Holocene cooling events: oceanic feedback amplifies solar forcing (2006, background): “10 Be from Summit, Greenland, indicates different long-term changes compared to the 14 C production rate (Muscheler et al., 2005; Vonmoos et al., 2006).”
- SOLAR INFLUENCES ON CLIMATE (2010, unknown): “In this way, at least the past 10,000 years can be reconstructed [Vonmoos et al., 2006], although the temporal resolution is poorer, signal‐to‐noise ratio is lower, and the record must be corrected for variations in the geomagnetic field.”
- 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).”
- A new approach to the long-term reconstruction of the solar irradiance leads to large historical solar forcing (2011, methodology): “Herbst et al. (2010) analyzed the dependency of the modulation potential on the applied LIS models and show that negative values of the modulation potential in Vonmoos et al. (2006) data can be corrected with another LIS model.”
- Evidence from wavelet analysis for a mid-Holocene transition in global climate forcing (2009, background): “…be used to identify common spectral signatures for a wide range of paleoclimatic records: marine sediments (Bianchi and McCave, 1999; [Chapman and Shackleton, 2000] and [Giraudeau et al., 2000]), ice cores ([O'Brien et al., 1995] and [Vonmoos et al., 2006]) and dust records (Jackson et al., 2005).”