Multifractal properties of solar wind turbulence: theory and observations.

Details Multifractal properties of solar wind turbulence: theory and observations. Multifractal properties of solar wind turbulence: theory and observations.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kosis..34..451m&link_type=abstract

Kosmicheskie Issledovaniia, Tom 34, No. 5, p. 451 - 456

Computer Science

5

Solar Wind: Turbulence, Solar Wind: Structure

Scientific paper

A fractal model of the solar wind is presented. This model treats fluctuations of the solar wind velocity from the viewpoint of nonlinear processes originating in the convective region and photosphere of the Sun. The multifractal structure of proton velocity fluctuations in a region of heliocentric distances from 0.2 to 0.8 AU is a result of these processes. Continuous measurements of solar wind velocity aboard the ISEE-3 spacecraft during one month were used to compare the theoretical and experimental results. It is shown that fluctuations of proton velocity have a multifractal structure in a frequency range of 10-5 - 10-3Hz.

Affiliated with

Also associated with

No associations

Rating

Multifractal properties of solar wind turbulence: theory and observations. 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 Multifractal properties of solar wind turbulence: theory and observations., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multifractal properties of solar wind turbulence: theory and observations. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1137435