Computer Science
Scientific paper
May 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ssrv...97..289m&link_type=abstract
Space Science Reviews, v. 97, Issue 1/4, p. 289-292 (2001).
Computer Science
Scientific paper
We present and compare observations of energetic protons during the two first transits of the Ulysses spacecraft from low to high latitudes in the southern heliosphere. Protons in the energy range 1.8 3.8 MeV from the COSPIN experiment are studied for global trends and in relation to some ambient structures in the solar wind (corotating interaction region, forward/reverse shock). The global trends show the large dependence on the heliospheric condition and solar activity, including indications of a larger ambient particle population during the rising phase of solar activity and more efficient solar wind particle accelerators during the declining phase. More enhancements in the proton flux intensity are time associated with forward shocks than reverse contrary to first pass. Recurrent structures are found even during the second transit. Some latitude dependent periodicities are observed that could relate to the differential solar rotation.
Forsyth Robert J.
Goldstein Bruce E.
Marsden Richard G.
Moullard O.
Sanderson T. R.
No associations
LandOfFree
Energetic Ions Observed at Low to High Latitudes in the Southern Heliosphere During Declining and Rising Solar Activity 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 Energetic Ions Observed at Low to High Latitudes in the Southern Heliosphere During Declining and Rising Solar Activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energetic Ions Observed at Low to High Latitudes in the Southern Heliosphere During Declining and Rising Solar Activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-949008