Computer Science
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...44b&link_type=abstract
Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 7, p. 44-47.
Computer Science
Convection-Diffusion Equation, Cosmic Rays, Diurnal Variations, Interplanetary Medium, Solar Activity Effects, Amplitude Distribution Analysis, Anisotropy, Phase Deviation
Scientific paper
An analysis of diurnal values of cosmic-ray (CR) anisotropy components obtained from the global network of neutron monitors for the 1970s and 1980s shows a specific relationship between the amplitude and phase of the solar-diurnal variation. This relationship and differences in the anisotropy for two different solar minima are explained by the convective-diffusive model of anisotropy, taking into account all three components of the CR gradient. Distributions of the radial and latitudinal CR gradients in the solar wind in the vicinity of the earth are calculated for the 1974-1977 and 1984-1987 periods.
Belov Anatoly V.
Dorman Lev I.
Eroshenko Eugenia A.
Rudnev Yu. F.
No associations
LandOfFree
Relationship between the amplitude and phase of cosmic-ray anisotropy near two minima of solar activity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Relationship between the amplitude and phase of cosmic-ray anisotropy near two minima of solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relationship between the amplitude and phase of cosmic-ray anisotropy near two minima of solar activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1231828