Plasma waves in coronal mass ejections: Ulysses observations

Details Plasma waves in coronal mass ejections: Ulysses observations Plasma waves in coronal mass ejections: Ulysses observations

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..673l&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 673-676 (1999).

Computer Science

3

Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The occurrence and properties of plasma waves associated with coronal mass ejections (CMEs) are investigated using the plasma wave instruments of the Unified Radio and Plasma Wave (URAP) experiment of the Ulysses spacecraft. Several CMEs observed by Ulysses at heliographic latitudes from the ecliptic plane to S60° are examined. Four wave modes are observed within the CMEs. 1) Electric waves at a few kHz, which are interpreted as Doppler shifted ion acoustic waves. They tend to occur in the region where the proton temperature is low. In all the cases that we studied, the electron temperature for the periods of enhanced ion acoustic like waves is greater than the proton temperature, although sometimes they are comparable (1

Affiliated with

Also associated with

No associations

Rating

Plasma waves in coronal mass ejections: Ulysses 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 Plasma waves in coronal mass ejections: Ulysses observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Plasma waves in coronal mass ejections: Ulysses observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1496624