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Detailed Reference Information |
Usoskin, I.G., Alanko-Huotari, K., Kovaltsov, G.A. and Mursula, K. (2005). Heliospheric modulation of cosmic rays: Monthly reconstruction for 1951–2004. Journal of Geophysical Research 110. doi: 10.1029/2005JA011250. issn: 0148-0227. |
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The differential energy spectrum of galactic cosmic rays in the vicinity of the Earth can be parameterized by the so-called force field model which has only one parameter, the modulation potential $phi$, for a given local interstellar spectrum. Here we present the series of monthly values of the modulation potential $phi$ since February 1951, reconstructed using the data from the worldwide neutron monitor network and calibrated with precise balloon and space-borne direct measurements of cosmic ray energy spectrum. This work provides a long series of a parameter allowing for a quantitative estimate of the average monthly differential energy spectrum of cosmic rays near the Earth. A comparison with other occasional direct measurements of cosmic ray spectra confirms the reliability of the present reconstruction. The results can be applied in studies of long-term solar-terrestrial relations and the global evolution of the heliosphere. |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Interplanetary Physics, Cosmic rays, Interplanetary Physics, Solar cycle variations, Interplanetary Physics, Interplanetary magnetic fields, Space Weather, Space radiation environment, Global Change, Solar variability, cosmic rays, heliosphere, solar activity |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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