The cosmic ray composition as viewed from the chemical abundances of the solar system

Details The cosmic ray composition as viewed from the chemical abundances of the solar system The cosmic ray composition as viewed from the chemical abundances of the solar system

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3...25s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 25-28 (SEE N85-34862 23-93)

Computer Science

Chemical Composition, Chemical Elements, Chondrites, Cosmic Rays, Cosmochemistry, Point Sources, Allende Meteorite, Atomic Weights, Nebulae, Protostars, Refractory Materials, Supernovae

Scientific paper

It is shown that the chemical composition of cosmic rays at their sources for the elements up to the atomic number as 80 is quite similar to that of the carbonaceous chondrites, which have been keeping the properties of the protosolar nebula. In particular, the similarity between these two compositions is significant to the elements classified as refractory and siderphile, in addition to the elements, Ca and Al. These results as cited above suggest that cosmic rays, being currently observed near the Earth, may have been accelerated from the matter with the composition similar to that which is found of these chondrites as Allende.

Affiliated with

Also associated with

No associations

Rating

The cosmic ray composition as viewed from the chemical abundances of the solar system 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 cosmic ray composition as viewed from the chemical abundances of the solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The cosmic ray composition as viewed from the chemical abundances of the solar system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-754796