The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments

Details The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ssrv...97..123v&link_type=abstract

Space Science Reviews, v. 97, Issue 1/4, p. 123-127 (2001).

Computer Science

8

Scientific paper

The source region of solar wind plasma is observed to be directly reflected in the compositional pattern of both elemental and charge state compositions. Slow solar wind associated with streamers shows higher freeze-in temperatures and larger FIP enhancements than coronal hole associated wind. Also, the variability of virtually all compositional parameters is much higher for slow solar wind compared to coronal hole associated wind. We show that these compositional patterns persist even though stream-stream interactions complicate the identification based on in situ plasma parameters.

Affiliated with

Also associated with

No associations

Rating

The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments 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 The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-948737