Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events

Details Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005soph..229..305s&link_type=abstract

Solar Physics, Volume 229, Issue 2, pp.305-312

Physics

2

Scientific paper

Outflow of slow solar wind from solar active regions has been reported in recent years by many different authors. Therefore, in this paper we have studied synoptic maps of the solar wind density (SWD) based on interplanetary scintillation (IPS) data for available parts of all the years 1991 1994 and 1997 2001 to verify correlations of maxima in SWD with sources in active regions. We have found convincing evidence that eruptive flares in active regions, and thus X-ray long-decay events (LDEs) in general, can produce short-lived enhancements of the SWD. However, we were not able to get statistically convincing evidence that active regions can be permanent sources of slow solar wind, and propose three possible reasons for this negative result.

Affiliated with

Also associated with

No associations

Rating

Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events 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 Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence Linking Slow Solar Wind Streams to Long-Decay X-Ray Events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1469527