Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure

Details Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh32a..02p&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH32A-02

Physics

7534 Radio Emissions, 7845 Particle Acceleration, 7851 Shock Waves (4455)

Scientific paper

Observations of the electron foreshock region of CME-driven IP shocks by the Wind spacecraft reveal mesoscale (several RE) nonplanar shock structure associated with the source regions of type II radio bursts. We analyze three shocks and infer the shock-parallel and shock-perpendicular scale of the structure. We offer speculative causes of the structure morphology. It is possible that the fine structure observed in type II emission is related to the mesoscale structure of these IP shocks.

Affiliated with

Also associated with

No associations

Rating

Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure 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 Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Shock Structure at Interplanetary Type II Bursts: A possible role in type II fine structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1026513