Observation of cosmic ray decreases between 1 and 5 AU

Details Observation of cosmic ray decreases between 1 and 5 AU Observation of cosmic ray decreases between 1 and 5 AU

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh51a1465s&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH51A-1465

Physics

7514 Energetic Particles (2114)

Scientific paper

The on-going Ulysses mission provides a unique opportunity to study the propagation and modulation of galactic cosmic rays in detail from 1 to 5 AU and from 80° South to 80° North latitude. The Kiel Electron Telescope (KET) measures the intensities and energy spectra of energetic particles separating electrons, hydrogen and helium. The instrument covers an energy range from ~5MeV/n to above 2GeV/n for hydrogen and helium. The highest energy channels correspond to mean rigidities of about 6GV and 12GV. The Kiel Neutron Monitor (KNM) is one of the longest operating Neutron Monitors in the world, it has been operating continuously since the IGY 1957. It is located at 54.34°N/10.12°E and has a cutoff rigidity of 2.36GV. In this contribution we use the KET and KNM observations in order to analyze the evolution of cosmic ray decreases observed by the both particle detectors.

Affiliated with

Also associated with

No associations

Rating

Observation of cosmic ray decreases between 1 and 5 AU 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 Observation of cosmic ray decreases between 1 and 5 AU, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observation of cosmic ray decreases between 1 and 5 AU will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-968866