Solar modulation parameter for cosmic rays since 1936 reconstructed from ground-based neutron monitors and ionization chambers
By I. Usoskin, Galina Bazilevskaya, G. Kovaltsov. 2011
282 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ea7d7edec926444f1269ddf4e321d1286ae421da
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- I. Usoskin
- Paul Charbonneau
- F. Joos
- R. Roth
- G. Kovaltsov
- Richard Harrison
- Eugene V. Rozanov
- Galina Bazilevskaya
In Nuclear and High Energy Physics
- I. Usoskin
- G. Kovaltsov
- F. Joos
- R. Roth
- Eugene V. Rozanov
- Galina Bazilevskaya
- A. Mishev
- Richard Harrison
Citations in the corpus
- Solar Forcing for CMIP6 (v3.1) (2016, methodology): “Accordingly, we use a full Monte-Carlo model CRAC:CRII (Usoskin and Kovaltsov, 2006; Usoskin et al., 2010) based on 15”
- A new model of cosmogenic production of radiocarbon 14C in the atmosphere (2012, methodology): “The modulation potentialφ varies between about 300 and 1500 MV within a modern high solar108 cycle (Usoskin et al., 2011), and can be as low as about 100 MV during the Maunder minimum (McCracken et al.,109 2004; Usoskin et al., 2007; Steinhilber et al., 2008).”
- Energetic Particle Influence on the Earth’s Atmosphere (2015, methodology): “While SEPs have higher fluxes and energy during the periods of active Sun, GCRs are inversely modulated by solar activity.”
- Interpretation of AMS-02 electrons and positrons data (2014, result): “0) GV, in accordance to results1 of combined analysis of proton and helium spectra correlated with neutron monitors data [191, 192], and compatible with our determination for the AMS-02 data taking period derived in section 2.”
- 9,400 years of cosmic radiation and solar activity from ice cores and tree rings (2012, methodology): “Land area (EDML) ice cores and (14)C from tree rings for the period 1,194–9,400 BP is extended to the present day by applying PCA to several other high-resolution (10)Be records from Greenland [NorthGRIP (15), Dye3 (16), Milcent (17)] and Antarctica [Dome Fuji (18), South Pole (19)], and to (14)C fr”
- 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): “57 W m −2) calculated in this study (black with grey 1σ error, lefty axis), and the reconstructions by Vieira et al.(2011) (VEA11, red) andSteinhilber et al.”