Propagation of energetic particles to high heliographic latitudes

Details Propagation of energetic particles to high heliographic latitudes Propagation of energetic particles to high heliographic latitudes

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh11a0374s&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH11A-0374

Physics

2118 Energetic Particles, Solar, 2159 Plasma Waves And Turbulence

Scientific paper

We present observations of energetic particles in the energy range 0.3 MeV to 100 MeV made by the COSPIN instrument on board the Ulysses spacecraft during the recent second northern polar pass. At this time, the Ulysses spacecraft was at high heliographic latitude and was immersed in high speed solar wind flow coming from the northern polar coronal hole. Three large solar energetic particle events were observed at this time. We present a detailed analysis of the propagation of these energetic particles in the relatively homogeneous plasma of the high speed flow. We examine the particle time intensity profiles and anisotropies over a wide range of energies, and discuss this in the context of current propagation models.

Affiliated with

Also associated with

No associations

Rating

Propagation of energetic particles to high heliographic latitudes 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 Propagation of energetic particles to high heliographic latitudes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of energetic particles to high heliographic latitudes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1434620