Computer Science
Scientific paper
May 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42.1038a&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska
Computer Science
Cosmic Rays, Galactic Radiation, Interplanetary Space, Modulation, Particle Diffusion, Solar Activity, Differential Equations, Diffusion Coefficient, Finite Difference Theory, Solar Wind Velocity
Scientific paper
The finite-difference method is used to solve the differential equation which describes galactic-cosmic-ray diffusion in interplanetary space, taking into account spot zones in the distribution of solar activity. The case is considered where extremum values of the diffusion coefficient and solar-wind velocity are observed in the colatitude regions between + and - 65 and 85 deg from the solar equator. The behavior of radial and transverse cosmic-ray gradients is examined, and the results are compared with spacecraft observations.
Alaniia M. V.
Dorman Lev I.
No associations
LandOfFree
Modulation of cosmic-ray intensity in interplanetary space with allowance for SPOT zones in the distribution 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 Modulation of cosmic-ray intensity in interplanetary space with allowance for SPOT zones in the distribution of solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modulation of cosmic-ray intensity in interplanetary space with allowance for SPOT zones in the distribution of solar activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1297593