Computer Science – Sound
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88.2029b&link_type=abstract
Journal of Geophysical Research, vol. 88, Mar. 1, 1983, p. 2029-2037. Research supported by the Consiglio Nazionale delle Ricer
Computer Science
Sound
11
Ion Motion, Magnetohydrodynamic Turbulence, Satellite Sounding, Solar Terrestrial Interactions, Solar Wind Velocity, Space Plasmas, Bow Waves, Explorer 50 Satellite, International Sun Earth Explorers, Interplanetary Magnetic Fields, Ion Density (Concentration)
Scientific paper
The interaction of the solar wind with ions backstreaming from the earth's bow shock is investigated using plasma and magnetic field measurements on ISEE 1 and 2 and IMP 8 at widely separated positions in the earth's foreshock. This technique separates temporal and spatial variations within the foreshock. It is found that the solar wind acceleration associated with backstreaming ions is correlated with the amplitude of the MHD turbulence and that the largest decelerations are seen close to the bow shock. The density of the backstreaming ion beam is strongly correlated with distance from the shock and decreases by about a factor of 3 in a distance of about 3 RE.
Bonifazi Carla
Lazarus Andrew J.
Moreno Giovani
Russell Christopher T.
Sullivan David J.
No associations
LandOfFree
Solar wind deceleration and MHD turbulence in the earth's foreshock region - ISEE 1 and 2 and IMP 8 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 Solar wind deceleration and MHD turbulence in the earth's foreshock region - ISEE 1 and 2 and IMP 8 observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar wind deceleration and MHD turbulence in the earth's foreshock region - ISEE 1 and 2 and IMP 8 observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1467726