What Can We Deduce about Coronal Mass Ejections from STEREO observations?

Details What Can We Deduce about Coronal Mass Ejections from STEREO observations? What Can We Deduce about Coronal Mass Ejections from STEREO observations?

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh21d..03l&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH21D-03

Physics

7513 Coronal Mass Ejections, 7524 Magnetic Fields

Scientific paper

Coronal mass ejections (CMEs) have been a topic of considerable scientific interest for many years. Despite years of study, many questions remains unanswered. What is the 3D structure of CMEs? How do we relate the white-light images of CMEs near the Sun to the in situ properties of ICMEs? What initiates CMEs? The STEREO mission promises to yield an impressive array of images and in situ measurements that can be brought to bear on these questions. The challenges facing the solar and heliospheric community is to utilize this data to unravel the structure and dynamics of CMEs. In this talk we will use 3D MHD simulations of CMEs to illustrate some of the challenges we face in deducing the structure of CMEs from 3 different viewpoints. We will discuss how models may help to reduce these uncertainties. Research supported by NASA and NSF.

Affiliated with

Also associated with

No associations

Rating

What Can We Deduce about Coronal Mass Ejections from STEREO observations? 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 What Can We Deduce about Coronal Mass Ejections from STEREO observations?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and What Can We Deduce about Coronal Mass Ejections from STEREO observations? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1461026