Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum

Details Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...192..753m&link_type=abstract

Astrophysical Journal, vol. 192, Sept. 15, 1974, pt. 1, p. 753-755.

Astronomy and Astrophysics

Astrophysics

Cosmic Rays, Energy Spectra, Galactic Radiation, Monte Carlo Method, Plasma-Particle Interactions, Solar Wind, Abundance, Astronomical Spectroscopy, Mean Free Path, Nitrogen, Proton Flux Density, Scale (Ratio)

Scientific paper

A previous (Moss and Giuli, 1971) Monte Carlo analysis of the solar-wind modulation of galactic cosmic-ray rigidity spectra is extended to include particles in the C-N-O group. A solar cavity 'radius' of 7 AU is found to be consistent with observations of the C-N-O component at solar maximum. The variation in modulation between solar maximum and solar minimum may be explained solely by variation of the solar cavity size, with no change in the scattering mean free path.

Affiliated with

Also associated with

No associations

Rating

Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum 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 Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Monte Carlo analysis of the solar-wind modulation of galactic C-N-O at solar maximum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1583067