Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..529c&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 22, July-Aug. 1982, p. 529-535. In Russian.
Astronomy and Astrophysics
Astronomy
7
Interplanetary Medium, Magnetohydrodynamic Waves, Plasma Turbulence, Solar Wind, Spectral Energy Distribution, Astronomical Models, Energy Sources, Nonlinear Systems, Spherical Plasmas, Turbulence Effects
Scientific paper
It is shown that the quasi-steady turbulence spectrum in the solar wind is sustained by the concurrence of the relative intensification of turbulence associated with spherical plasma expansion and nonlinear three-wave interaction processes. The wave source is localized in regions near the sun, and the feeding of the spectral energy flux into the inertial interval is associated with an increase in the amplitude of low-frequency waves. The basic results of this model agree well with results of observations.
Chashei Igor V.
Shishov V. I.
No associations
LandOfFree
The source of turbulence energy in the solar wind 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 The source of turbulence energy in the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The source of turbulence energy in the solar wind will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-900558