Anisotropies and the power requirements for galactic cosmic rays

Details Anisotropies and the power requirements for galactic cosmic rays Anisotropies and the power requirements for galactic cosmic rays

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasa...15..208c&link_type=abstract

Publications Astronomical Society of Australia, vol. 15, no. 2, p. 208-210

Astronomy and Astrophysics

Astronomy

8

Ism, Cosmic Rays

Scientific paper

Measurements of cosmic ray directional properties at about 1015 eV in both northern and southern hemispheres confirm that those particles have a unidirectional anisotropy and are flowing along the direction of our spiral arm from the inner galactic regions. On the basis of diffusive cosmic ray flow along the galactic arms, the power required for the galaxy to maintain this flow is below 1030 W.

Affiliated with

Also associated with

No associations

Rating

Anisotropies and the power requirements for galactic 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 Anisotropies and the power requirements for galactic cosmic rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Anisotropies and the power requirements for galactic cosmic rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1271684