Creation and destruction of transitory coronal holes and their fast solar wind streams

Details Creation and destruction of transitory coronal holes and their fast solar wind streams Creation and destruction of transitory coronal holes and their fast solar wind streams

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jgra..108.1013n&link_type=abstract

Journal of Geophysical Research (Space Physics), Volume 108, Issue A1, pp. SSH 3-1, CiteID 1013, DOI 10.1029/2002JA009326

Astronomy and Astrophysics

Astrophysics

3

Solar Physics, Astrophysics, And Astronomy: Coronal Holes, Interplanetary Physics: Corotating Streams, Interplanetary Physics: Sources Of The Solar Wind, And Astronomy: Magnetic Fields

Scientific paper

A qualitative model is proposed whereby foot point exchange diffusion of open field lines from a solar active region may have led to the formation of a coronal hole and a corotating stream of fast solar wind. The solar wind speed changed from fast back to slow when the coronal hole was later disrupted by the emergence of a new active region. A corollary of this model is that a corotating interplanetary field line may have both fast and slow solar wind at different places along its length.

Affiliated with

Also associated with

No associations

Rating

Creation and destruction of transitory coronal holes and their fast solar wind streams 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 Creation and destruction of transitory coronal holes and their fast solar wind streams, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Creation and destruction of transitory coronal holes and their fast solar wind streams will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1530124