On the origin of turbulent fields in interplanetary plasmas

Details On the origin of turbulent fields in interplanetary plasmas On the origin of turbulent fields in interplanetary plasmas

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..318l&link_type=abstract

EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 318-322 (2008).

Computer Science

Interplanetary Magnetic Fields, Coronal Mass Ejection, Flare Stars, Turbulence, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

Solar coronal mass ejections are prominent example of interpenetrating particle streams with different properties: densities, speeds, temperature and composition. Such counterstreaming plasmas are quickly unstable leading to the excitation of the electrostatic and electromagnetic instabilities. Here it is shown that plasma instabilities of Weibel-type could offer plausible explanations for the origin of the two-dimensional magnetic field fluctuations observed in interplanetary space.

Affiliated with

Also associated with

No associations

Rating

On the origin of turbulent fields in interplanetary plasmas 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 On the origin of turbulent fields in interplanetary plasmas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the origin of turbulent fields in interplanetary plasmas will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1292770