Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Track parameters in olivine crystals from pallasite Marjalahti were
recorded. Some results of comparison of obtained nucleus abundance
distribution data with the results of satellite apparatus measuring and
Sun and solar system values are presented.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values 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 Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Abundance of the Super-Heavy (Z>55) Galactic Cosmic Ray Nuclei by the Meteorite Track Data: Comparison with the Satellite Apparatus Measuring and the Sun and Solar System Values will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-889412

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.