The three-dimensional configuration and the effects of the "fading" of flare coronal transients.

Details The three-dimensional configuration and the effects of the "fading" of flare coronal transients. The three-dimensional configuration and the effects of the "fading" of flare coronal transients.

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..191i&link_type=abstract

Geomagn. Aeron., Vol. 29, No. 2, p. 191 - 196

Statistics

Solar Coronal Transients: Statistics

Scientific paper

On the basis of the solution of the direct problem of the projection of the coronal ejection of mass (CEM) of a given form onto the celestial plane by using the experimental data of a white-light coronagraph, the inverse problem of seeking a three-dimensional configuration in the class of oblate spheroids is solved. For flares of importance Imax = 2, with the imposition of certain conditions on the position angle, it is found that the CEM, and also the interplanetary shockwave, are oblate, with an axis ratio of ≡1.25, to the plane of the great circle passing through the flare in parallel with the magnetic axis of the nearest bipolar group.

Affiliated with

Also associated with

No associations

Rating

The three-dimensional configuration and the effects of the "fading" of flare coronal transients. 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 three-dimensional configuration and the effects of the "fading" of flare coronal transients., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The three-dimensional configuration and the effects of the "fading" of flare coronal transients. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1528671