Turbosphere and turbopause in the solar wind formation region

Details Turbosphere and turbopause in the solar wind formation region Turbosphere and turbopause in the solar wind formation region

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..381v&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 381-384 (1999).

Physics

2

Particle Emission, Solar Wind, Magnetohydrodynamics And Plasmas

Scientific paper

The MHD classification of the regimes is based on the relative values of the phase velocities versus the turbulent velocity dispersion σ and regular flow velocity V. Concepts of the turbosphere and the turbopause around the Sun are introduced as follows. In the solar atmosphere near the Sun one has σ>V. This domain may be termed as the turbosphere around the Sun. An opposite situation, σ

Affiliated with

Also associated with

No associations

Rating

Turbosphere and turbopause in the solar wind formation region 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 Turbosphere and turbopause in the solar wind formation region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbosphere and turbopause in the solar wind formation region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1496115