Propagation of the phase of solar modulation

Details Propagation of the phase of solar modulation Propagation of the phase of solar modulation

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..400f&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 400-403 (SEE N85-34729 23-92)

Physics

Galactic Radiation, Periodic Variations, Pulse Modulation, Radiant Flux Density, Solar Cosmic Rays, Wave Propagation, Diffusion Coefficient, Field Strength, Heuristic Methods, Magnetic Fields, Neutral Sheets, Proton Scattering, Protons, Solar Wind, Time Dependence

Scientific paper

The phase of the 11-year galactic cosmic-ray variation, due to a varying rate of emission of long-lived propagating regions of enhanced scattering, travels faster than the scattering regions themselves. The radial speed of the 11-year phase in the quasi-steady force-field approximation is exactly twice the speed of the individual, episodic decreases. A time-dependent numerical solution for 1-GeV protons at 1 and 30 AU gives a phase speed which is 1.85 times the propagation speed of the individual decreases.

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