Shocks as a Universal Process

Details Shocks as a Universal Process Shocks as a Universal Process

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh54a..01r&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH54A-01

Astronomy and Astrophysics

Astrophysics

7513 Coronal Mass Ejections, 7807 Charged Particle Motion And Acceleration, 7851 Shock Waves

Scientific paper

Shock waves are ubiquitous in low density flows in astrophysics. In most cases the shocks are collisionless, though in many cases the observable consequences of the shock occur far downstream after collisions have erased the signatures of collisionless processes. This talk will concentrate on a one aspect of shock wave physics addressed by observations within the heliosphere and magnetosphere, and by observations of shock waves in supernova remnants: How is the energy dissipated in a shock partitioned among thermal and non-thermal energies of different particle species and the magnetic field.

Affiliated with

Also associated with

No associations

Rating

Shocks as a Universal Process 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 Shocks as a Universal Process, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Shocks as a Universal Process will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1694891