Solar wind quasi invariant within ICMEs

Details Solar wind quasi invariant within ICMEs Solar wind quasi invariant within ICMEs

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..652l&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 652-654 (2010).

Mathematics

Probability

Solar Wind, Solar Activity, Solar Corona, Probability, Magnetic Fields, Particle Emission, Solar Wind, Solar Activity, Coronal Mass Ejection, Probability Theory, Electric And Magnetic Fields, Solar Magnetism

Scientific paper

The ratio of the magnetic-to-kinetic energy densities in the solar wind is an in situ measurement that correlates well with the solar activity cycle. For this reason it has been called a ``solar wind quasi-invariant'' (QI). In this paper we investigate the probability density functions (PDFs) of QI in Interplanetary Coronal Mass Ejections (ICMEs). The obtained PDF is discussed in terms of log-normal and log-kappa functions. A comparison with the PDFs as obtained for the solar wind during maximum and minimum phases of solar cycle 23 (1996-2007) is presented.

Affiliated with

Also associated with

No associations

Rating

Solar wind quasi invariant within ICMEs 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 wind quasi invariant within ICMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar wind quasi invariant within ICMEs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1424062