Three-dimensional propagation of CMEs in the heliosphere

Details Three-dimensional propagation of CMEs in the heliosphere Three-dimensional propagation of CMEs in the heliosphere

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..665p&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 665-668 (1999).

Physics

Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A 3-D hydrodynamic numerical model is used to investigate the essential physics of the large-scale interaction between CMEs and the structured background solar wind. A tilted-dipole steady outflow configuration is established by numerical relaxation between 0.14 and 5.04 AU. Time-dependent velocity and pressure pulses are introduced at the inner boundary at differing locations with respect to the corotating streamer belt flow. Results show that CMEs may be significantly distorted due mainly to local variations in the background flow speed geometry. Thus an individual CME can present radically different appearances at various locations in the heliosphere.

Affiliated with

Also associated with

No associations

Rating

Three-dimensional propagation of CMEs in the heliosphere 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 Three-dimensional propagation of CMEs in the heliosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-dimensional propagation of CMEs in the heliosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1496614