Astronomy and Astrophysics – Astronomy
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.6509g&link_type=abstract
American Astronomical Society, 200th AAS Meeting, #65.09; Bulletin of the American Astronomical Society, Vol. 34, p.752
Astronomy and Astrophysics
Astronomy
Scientific paper
The magnetic nature of coronal mass ejections has been inferred from the fact that they originate from closed magnetic field regions on the Sun such as active regions and filament regions. Although we have no direct measurement of the magnetic fields of CMEs, we can obtain useful information on the magnetic structure of CMEs from coronal observations at various wavelengths. The CME is a multithermal structure with temperatures ranging from a few kilokelvin to several megakelvin, so we need multi-wavelength observations to get a global picture of CMEs. A wide range of ground and space based instruments routinely observe CMEs. We present several examples of CMEs observed in X-ray, white light, EUV and radio wavelengths that help us understand the magnetic structure of CMEs.
No associations
LandOfFree
Evidence from Coronal Observations of Magnetic Field Structure in CMEs 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 Evidence from Coronal Observations of Magnetic Field Structure in CMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence from Coronal Observations of Magnetic Field Structure in CMEs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1720023