Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating in the Solar Wind

Details Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating in the Solar Wind Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating in the Solar Wind

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973apj...179..931p&link_type=abstract

Astrophysical Journal, Vol. 179, pp. 931-938 (1973)

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1973ApJ...179..931P

Affiliated with

Also associated with

No associations

Rating

Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating 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 Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating in the Solar Wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electrostatic Turbulence at Colliding Plasma Streams as the Source of Ion Heating in the Solar Wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1444404