On the internal structure of coronal mass ejections

Details On the internal structure of coronal mass ejections On the internal structure of coronal mass ejections

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..603v&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Physics

Coronal Mass Ejections

Scientific paper

The internal geometry of coronal mass ejections (CMEs) is complicated and prescribed by initial and boundary conditions. Simplified models of coronal and heliospheric dynamical processes are described with the main attention paid to different dimensionless parameters and dominant physical regimes for ejecta and their substructures, which are multi-scale and non-local ones. We address two open questions discussed in the literature: 1) what is the correspondence degree between the three-part structure seen in the CME images and their heliospheric counterparts measured by spacecraft? 2) Why do we see He+ ions so rarely in the driver gas? Tentative answers follow from the geometry and dynamics considerations.

Affiliated with

Also associated with

No associations

Rating

On the internal structure of coronal mass ejections 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 On the internal structure of coronal mass ejections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the internal structure of coronal mass ejections will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1422858