Two dimensional model of the long period Variations of the Galactic Cosmic Ray Intensity

Details Two dimensional model of the long period Variations of the Galactic Cosmic Ray Intensity Two dimensional model of the long period Variations of the Galactic Cosmic Ray Intensity

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eguga..1111451s&link_type=abstract

"EGU General Assembly 2009, held 19-24 April, 2009 in Vienna, Austria http://meetings.copernicus.org/egu2009, p.11451"

Computer Science

Scientific paper

We solve numerically two-dimensional (2-D) Parker's Transport Equation describing the long period variations of the Galactic Cosmic Ray (GCR) intensity; in the model are including diffusion, convection, drifts, adiabatic cooling and the changes of the exponent ? of the power spectral density (PSD) of the interplanetary magnetic field turbulence as a time dependent parameter. A comparison of the results of solution with the neutron monitors experimental data shows a good compatibility of the proposed model of the long period modulation of the GCR intensity.

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