Solar wind distrubances in th outer heliosphere caused by successive solar flares from the same active region

Details Solar wind distrubances in th outer heliosphere caused by successive solar flares from the same active region Solar wind distrubances in th outer heliosphere caused by successive solar flares from the same active region

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.475a&link_type=abstract

In JPL Solar Wind Five p 475-480 (SEE N84-13067 03-92)

Physics

Heliosphere, Solar Activity Effects, Solar Flares, Solar Wind, Cosmic Rays, Interplanetary Magnetic Fields, Magnetohydrodynamics, Mathematical Models, Solar Physics

Scientific paper

Solar wind disturbances caused by successive flares from the same active region are traced to about 20 AU, using the modeling method developed by Hakamada and Akasofu (1982). It is shown that the flare-generated shock waves coalesce with the co-rotating interaction region of the interplanetary magnetic field, resulting in a large-scale magnetic field structure in the outer heliosphere. Such a structure may have considerable effects on the propagation of galactic cosmic rays.

Affiliated with

Also associated with

No associations

Rating

Solar wind distrubances in th outer heliosphere caused by successive solar flares from the same active region 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 distrubances in th outer heliosphere caused by successive solar flares from the same active region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar wind distrubances in th outer heliosphere caused by successive solar flares from the same active region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487805