Solar sources of high-velocity streams in the solar wind

Details Solar sources of high-velocity streams in the solar wind Solar sources of high-velocity streams in the solar wind

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....1002p&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #1002

Physics

Scientific paper

The relationship between the interplanetary shocks and solar flares was studied by the "marked stream" method. There is shown that the direction of the magnetic field within the front region of high-velocity streams in the solar wind approximately coincides with that in the flare region at the Sun. This suggests that the high-velocity streams and associated with them interplanetary shocks really originate in the flare regions, and the magnetic field carried by them is in essence the extension of the magnetic field of corresponding active regions on the Sun. This once more confirms the supposition on the high-velocity streams to be driven by some processes developing in active regions on the Sun during solar flares.

Affiliated with

Also associated with

No associations

Rating

Solar sources of high-velocity streams in the solar wind 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 sources of high-velocity streams in the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar sources of high-velocity streams in the solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-841296