Computer Science – Numerical Analysis
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..473z&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 473-476 (SEE N85-34729 23-92)
Computer Science
Numerical Analysis
Diffusion Coefficient, Drift Rate, Galactic Cosmic Rays, Interplanetary Space, Models, Modulation, Numerical Analysis, Particles, Solar Magnetic Field, Electron Emission, Proton Beams, Rates (Per Time), Solar Activity
Scientific paper
A numerical model is presented of the propagation of galactic cosmic rays in the interplanetary space for the case when the modulation depth determined by the level of the solar activity changed in time. The contribution of the particle drift in the regular field was also calculated and the agreement with experimental data is shown about the ratio of protons and electrons in two solar activity minima.
Churunova L. F.
Kryakunova O. N.
Shvartsman Ya. E.
Zusmanovich A. G.
No associations
LandOfFree
The influence of nonstationarity of the solar activity and general solar field on modulation of cosmic rays 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 The influence of nonstationarity of the solar activity and general solar field on modulation of cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The influence of nonstationarity of the solar activity and general solar field on modulation of cosmic rays will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-756464