Physics
Scientific paper
May 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh42a04w&link_type=abstract
American Geophysical Union, Spring Meeting 2001, abstract #SH42A-04 INVITED
Physics
2111 Ejecta, Driver Gases, And Magnetic Clouds, 2134 Interplanetary Magnetic Fields, 2169 Sources Of The Solar Wind, 7513 Coronal Mass Ejections
Scientific paper
The large amount of data obtained during this solar cycle on both the solar and interplanetary characteristics of coronal mass ejections (CMEs) provides an unprecedented opportunity for major advances in our understanding of the structure and development of CMEs. Recent spectroscopic and imaging studies with the SOHO instruments, TRACE, and Yohkoh SXT have provided insights into the solar dynamics and source regions of CMEs as well as their evolution through the corona. In situ observations at 1 AU by the ACE and Wind spacecraft and elsewhere in the heliosphere by PVO, NEAR and Ulysses have revealed new insights into the magnetic and plasma structures within CMEs that can be related to their solar origins. Observations of halo CMEs have been particularly useful for these studies and have been the bases of joint campaigns involving the Sun-to-Earth connections of transient disturbances. I will discuss these observations in the context of comparison of the solar and interplanetary structures of CMEs.
No associations
LandOfFree
Relating CME Structures Observed Near the Sun to Interplanetary Signatures 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 Relating CME Structures Observed Near the Sun to Interplanetary Signatures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relating CME Structures Observed Near the Sun to Interplanetary Signatures will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1275370