Measurement of 44Ti(44Sc) in meteorites

Details Measurement of 44Ti(44Sc) in meteorites Measurement of 44Ti(44Sc) in meteorites

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ncimc..16...29b&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 16 C, no. 1, p. 29-33.

Astronomy and Astrophysics

Astronomy

7

Cosmic Rays, Cosmochemistry, Meteoritic Composition, Scandium Isotopes, Titanium Isotopes, Gamma Ray Astronomy, Interplanetary Medium, X Ray Spectra

Scientific paper

The measurement of 44Ti produced by spallation reaction of cosmic rays in meteorites fell in the last hundred years can be used for investigations on century-scale variations of solar activity. The low specific activity and the interferences of natural background and of meteorite gamma emitters are the main difficulties to be surmounted in this measurement. A selective gamma spectrometer consisting of a HP Ge and a NaI(Tl) detectors in coincidence and anticoincidence has been set up in the underground (70 m w.e.) Laboratory of Monte dei Cappuccini, which allows to obtain a reliable measurement of 44Ti(44Sc).

Affiliated with

Also associated with

No associations

Rating

Measurement of 44Ti(44Sc) in meteorites 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 Measurement of 44Ti(44Sc) in meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurement of 44Ti(44Sc) in meteorites will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1276190