Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference

Details Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7527999.&link_type=abstract

Conf. held at Munich, Aug. 1975

Other

Conferences, Cosmic Rays, Hydrogen, Interstellar Extinction, Radiation Sources, Galactic Radiation, Gamma Rays, Particle Interactions, Photons, Sas, Supernova Remnants

Scientific paper

The galactic distribution of H2 was studied through gamma radiation and through X-ray, optical, and infrared absorption measurements from SAS-2 and other sources. A comparison of the latitude distribution of gamma-ray intensity with reddening data shows reddening data to give the best estimate of interstellar gas in the solar vicinity. The distribution of galactic cosmic ray nucleons was determined and appears to be identical to the supernova remnant distribution. Interactions between ultrahigh energy cosmic-ray nuclei and intergalactic photon radiation fields were calculated, using the Monte Carlo method.

Affiliated with

No affiliations

Also associated with

No associations

Rating

Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference 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 Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Selected Theoretical Studies Group contributions to the 14th International Cosmic Ray conference will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1757748