Computer Science – Numerical Analysis
Scientific paper
Jan 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ncimb..25..191c&link_type=abstract
Nuovo Cimento, Sezione B, vol. 25 B, Jan. 11, 1975, p. 191-207. Consiglio Nazionale delle Ricerche
Computer Science
Numerical Analysis
Fokker-Planck Equation, Interplanetary Space, Particle Motion, Solar Corpuscular Radiation, Boundary Conditions, Boundary Value Problems, Cosmic Rays, Energy Transfer, Numerical Analysis, Particle Flux Density, Solar Wind
Scientific paper
The numerical solution of the spherically symmetric, steady-state Fokker-Planck equation of transport in a system of reference anchored at the earth with the energy variable (T), as measured in a frame moving with the solar wind, shows a good fit to recorded data in interplanetary space during 1965-1968. The boundary condition for a steady-state particle injection at the solar surface considers the energy transformation from the fixed frame into the moving one. Another possible introduction of boundary conditions via the differential current density is also discussed. Densities and gradients in an energy range of about 6 orders of magnitude centered around 1 GeV/nucleon and radial distances up to 5 AU are illustrated in stereographic projections. The radial anisotropy is also presented.
Cecchini Simone
Martinic Nicholas J.
No associations
LandOfFree
Interplanetary propagation of steady solar injected particles 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 Interplanetary propagation of steady solar injected particles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interplanetary propagation of steady solar injected particles will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1751167