CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration

Details CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..aprh14006n&link_type=abstract

American Physical Society, April Meeting, April 28 - May 1, 2001 Washington, DC Bulletin of the American Physical Society, Vol.

Statistics

Scientific paper

The secondary electron-capture decay isotopic abundances of 37Ar, 44Ti, 49V, 51Cr, 55Fe, 57Co and their decay products 37Cl, 44Ca, 49Ti, 51V, 55Mn, and 57Fe have been measured by the Cosmic Ray Isotope Spectrometer (CRIS) with sufficient statistics to examine energy dependence of their abundances relative to nearby stable isotopes. We compare these abundances with galactic propagation model calculations and find that they are in qualitative agreement with electron-capture decay during propagation. These results can be used to set limits on the amount of reacceleration that may have occurred as the cosmic rays encountered supernova shocks or turbulent magnetic fields.

Affiliated with

Also associated with

No associations

Rating

CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration 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 CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CRIS measurements of 37Ar, 44Ti, 49V, 51Cr, 55Fe, and 57Co: Limits on Galactic Cosmic Ray Reacceleration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1184167