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Measurement of the Iron Spectrum in Cosmic Rays from 10 GeV/n to 2.0 TeV/n with the Calorimetric Electron Telescope on the International Space Station

Authors :
O Adriani
Y Akaike
K Asano
Y Asaoka
E Berti
G Bigongiari
W R Binns
M Bongi
P Brogi
Alessandro Bruno
J H Buckley
Nicholas Wade Cannady
G Castellini
C Checchia
M L Cherry
G Collazuol
K Ebisawa
H Fuke
S Gonzi
T Gregory Guzik
Thomas Hams
K Hibino
M Ichimura
K Ioka
W Ishizaki
M H Israel
K Kasahara
J Kataoka
R Kataoka
Y Katayose
C Kato
N Kawanaka
Y Kawakubo
K Kobayashi
K Kohri
J F Krizmanic
J T Link
J W Mitchell
A A Moiseev
G A De Nolfo
K Sakai
M Sasaki
Source :
Physical Review Letters. 126(12)
Publication Year :
2021
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2021.

Abstract

The Calorimetric Electron Telescope (CALET), in operation on the International Space Station since 2015, collected a large sample of cosmic-ray iron over a wide energy interval. In this paper a measurement of the iron spectrum is presented in the range of kinetic energy per nucleon from 10GeV/n to 2.0 TeV/n allowing the inclusion of iron in the list of elements studied with unprecedented precision by space-borne instruments. The measurement is based on observations carried out from January 2016 to May 2020. The CALET instrument can identify individual nuclear species via a measurement of their electric charge with a dynamic range extending far beyond iron (up to atomic number Z = 40). The energy is measured by a homogeneous calorimeter with a total equivalent thickness of 1.2 proton interaction lengths preceded by a thin (3 radiation lengths) imaging section providing tracking and energy sampling. The analysis of the data and the detailed assessment of systematic uncertainties are described and results are compared with the findings of previous experiments. The observed differential spectrum is consistent within the errors with previous experiments. In the region from 50 GeV/n to 2 TeV/ n our present data are compatible with a single power law with spectral index−2.60±0.03.

Subjects

Subjects :
Astrophysics

Details

Language :
English
ISSN :
10797114 and 00319007
Volume :
126
Issue :
12
Database :
NASA Technical Reports
Journal :
Physical Review Letters
Notes :
NNX16AB99G, , NNX16AC02G, , NNH-14ZDA001N-APRA-0075, , JSPS-26220708, , JSPS-19H0560, , JSPS-17H02901, , JSPS-0K22352, , JSPS-S1101021
Publication Type :
Report
Accession number :
edsnas.20220000237
Document Type :
Report
Full Text :
https://doi.org/10.1103/PhysRevLett.126.241101