Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U.

Details Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U. Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U.

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...72..335l&link_type=abstract

Space Science Reviews, Volume 72, Issue 1-2, pp. 335-338

Computer Science

1

Scientific paper

We report the results of a study of the 12-hour average distribution functions of high Z nuclei as measured over a 10-day interval on the Ulysses spacecraft at a helioradius of˜5.2 A.U. We use the good time and atomic mass resolution of the composition aperture of the HI-SCALE instrument to determine the form of the distribution functions for C, O, Ne, Mg, Si, and Fe over the energy range ˜0.5 16 MeV/nucl. We find that the distribution functions of these ions can be organized by characteristic velocities that have values ranging between˜2000 3500 km/sec over this interval.

Affiliated with

Also associated with

No associations

Rating

Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U. 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 Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Study of distribution functions of interplanetary particles accelerated at co-rotating interaction region at˜5A.U. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1694691