Solar Origin and Interplanetary Evolution of Stream Interfaces

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

17

Scientific paper

In a Corotating Interaction Region (CIR) the stream interface is identified as a relatively sharp density drop, temperature rise, and flow shear in the solar wind, and is now generally believed to mark the boundary between solar wind which was originally slow when it left the Sun and solar wind which was originally fast. This paper summarises some important facts and open questions about the origin and nature of the boundary between fast and slow solar wind near the Sun, the evolution of stream interfaces with heliocentric distance in the inner heliosphere, and their relationship.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Solar Origin and Interplanetary Evolution of Stream Interfaces 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 Solar Origin and Interplanetary Evolution of Stream Interfaces, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Origin and Interplanetary Evolution of Stream Interfaces will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1577776

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.