Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000nva..conf..303s&link_type=abstract
NEW VISTAS IN ASTROPHYSICS. Proceedings of the International School of Cosmic Ray Astrophysics 20th Anniversary, 11th Course. He
Astronomy and Astrophysics
Astrophysics
Scientific paper
TIGER is a balloon-borne cosmic-ray experiment designed to measure the elemental abundances of Galactic Cosmic Rays (GCRs) in the charge range 26≤ Z ≤40 with better than 0.25 charge unit (cu) resolution. The experiment consists of a combination of plastic scintillators, acrylic and aerogel Cherenkov detectors, and scintillating fiber hodoscopes. TIGER was flown from Fort Sumner, NM aboard a high-altitude balloon on September 24, 1997 at geomagnetic cutoffs between 4.2 GV and 3.2 GV, and atmospheric depths between 3g/cm2 and 6g/cm2. The 23.5-hour balloon flight provided a statistically significant sample of GCR nuclei through Ni and achieved charge resolution capable of resolving Co from the much more abundant Fe peak.
Barbier Loius M.
Binns Robert W.
Christian Eric R.
de Nolfo Georgia Adair
Hink Paul L.
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