Computer Science
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989chjss...9..117w&link_type=abstract
Chinese Journal of Space Science (ISSN 0254-6124), vol. 9, April 1989, p. 117-126. In Chinese, with abstract in English.
Computer Science
Energetic Particles, Magnetic Field Reconnection, Solar Wind, Anisotropy, Solar Magnetic Field, Solar Terrestrial Interactions
Scientific paper
By comparing the intensity and anisotropy of the ion bursts (E above 125 keV/Q, Q above 1) observed simultaneously by the IMP-H and IMP-J satellite upstream of the bow shock in the time of January 21-22, 1976, it is shown that for four bursts a-d, when IMP-H is farther from the earth than IMP-J, (1) in the a and b bursts, the intensity observed by IMP-H is larger than that by IMP-J, and the anisotropy measurement made by IMP-J is flowing in a direction from the sun to the earth; (2) in the burst c, there is the same direction as the a and b bursts in the anisotropy, but the intensity observed by IMP-H is smaller than that by IMP-J; and (3) in the burst d, the characteristics of the intensity and anisotropy are both opposite to that in the a and b bursts. The phenomena can be interpreted satisfactorily by supposing that there are magnetic field reconnections in the solar wind which could produce energetic particles in the medium.
Lin Jin-Yun
Wu Ji-Ping
No associations
LandOfFree
The probability of the magnetic field reconnection in the solar wind and its observational evidence 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 probability of the magnetic field reconnection in the solar wind and its observational evidence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The probability of the magnetic field reconnection in the solar wind and its observational evidence will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1736700