Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU?

Details Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU? Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU?

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..137b&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 137-140 (1999).

Physics

8

Scientific paper

At 1 AU in 1998, when solar activity was increasing, the distribution of hour averages of the solar wind speed was approximately lognormal. There was no distinct separation between fast and slow flows. The density, temperature and magnetic field strength also had lognormal distributions. It was possible to identify distinct structures such as corotating streams and magnetic clouds during some intervals. We suggest that coexistence of a simple statistical structure and deterministic physical structures is the consequence of the dynamical evolution and interactions of the flows between the sun and 1 AU and a relatively complex source signal.

Affiliated with

Also associated with

No associations

Rating

Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU? 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 Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fast and Slow Flows in the Solar Wind Near the Ecliptic at 1 AU? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1277411