Computer Science – Numerical Analysis
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16...30d&link_type=abstract
(Geomagnetizm i Aeronomiia, vol. 16, Jan.-Feb. 1976, p. 30-36.) Geomagnetism and Aeronomy, vol. 16, Aug. 1976, p. 17-20. Transl
Computer Science
Numerical Analysis
1
Cosmic Rays, Density Distribution, Diffusion Coefficient, Interplanetary Magnetic Fields, Interplanetary Space, Particle Diffusion, Solar Activity Effects, Astronomical Models, Galactic Radiation, Numerical Analysis, Solar Wind Velocity, Steady State, Sunspot Cycle, Tensors
Scientific paper
The steady-state equation describing anisotropic diffusion of galactic cosmic rays is solved numerically taking account of real changes in solar activity with heliocentric latitude for the period from 1958 to 1968. The density distribution of galactic cosmic rays in interplanetary space is obtained as a function of heliocentric distance and latitude for each year of the 11-year cycle. Latitudinal density distributions of cosmic rays with a 1.2-GeV hardness are also determined for two different modulation-region radii as well as for heliocentric distances of 1.2 and 5 AU.
Dorman Lev I.
Milovidova N. P.
No associations
LandOfFree
Anisotropic cosmic-ray diffusion in interplanetary space. I - Density distribution 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 Anisotropic cosmic-ray diffusion in interplanetary space. I - Density distribution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Anisotropic cosmic-ray diffusion in interplanetary space. I - Density distribution will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1872724