Elemental abundances in corotating events

Details Elemental abundances in corotating events Elemental abundances in corotating events

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..190v&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 190 (SEE N85-34729 23-92)

Physics

Energetic Particles, Particle Acceleration, Solar Cycles, Solar Flares, Solar Wind, Algorithms, International Sun Earth Explorer 3, Interplanetary Magnetic Fields

Scientific paper

Large, persistent solar-wind streams in 1973 and 1974 produced corotating interaction regions which accelerated particles to energies of a few MeV/nucleon. The proton to helium ratio (H/He) was remarkably constant at a value (22 + or 5) equal to that in the solar wind (21 + or - 3), suggesting that particles were being accelerated directly out of the solar wind. Preliminary results were presented from a similar study approximately 11 years (i.e., one solar cycle) later. Corotating events have been identified by surveying the solar wind data, energetic particle time-histories and anisotropies. This data was all obtained from the ISEE-3/ICE spacecraft. These events also show H/He ratios similar to that in the solar wind. It is found that in these cases there is evidence for H/He ratios which are significantly different from that of the solar wind but which are consistent with the range of values found in solar flare events.

Affiliated with

Also associated with

No associations

Rating

Elemental abundances in corotating events 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 Elemental abundances in corotating events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elemental abundances in corotating events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-755892