Cosmic-ray proton and helium spectra: Results from the JACEE experiment

被引:292
作者
Asakimori, K [1 ]
Burnett, TH
Cherry, ML
Chevli, K
Christ, MJ
Dake, S
Derrickson, JH
Fountain, WF
Fuki, M
Gregory, JC
Hayashi, T
Holynski, R
Iwai, J
Iyono, A
Johnson, J
Kobayashi, M
Lord, J
Miyamura, O
Moon, KH
Nilsen, BS
Oda, H
Ogata, T
Olson, ED
Parnell, TA
Roberts, FE
Sengupta, K
Shiina, T
Strausz, SC
Sugitate, T
Takahashi, Y
Tominaga, T
Watts, JW
Wefel, JP
Wilczynska, B
Wilczynski, H
Wilkes, RJ
Wolter, W
Yokomi, H
Zager, E
机构
[1] Kobe Womens Jr Coll, Kobe, Hyogo, Japan
[2] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[3] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[4] Univ Alabama, Coll Sci, Huntsville, AL 35899 USA
[5] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[6] Kobe Univ, Kobe, Hyogo 657, Japan
[7] Kochi Univ, Kochi 780, Japan
[8] Waseda Univ, Tokyo, Japan
[9] Inst Nucl Phys, Krakow, Poland
[10] Okayama Univ, Okayama 700, Japan
[11] Kek Nat Lab High Energy Phys, Tsukuba, Ibaraki 305, Japan
[12] Hiroshima Univ, Hiroshima, Japan
[13] Inst Cosm Ray Res, Tokyo, Japan
[14] Tezukayama Univ, Nara, Japan
关键词
acceleration of particles; balloons; ISM : cosmic rays;
D O I
10.1086/305882
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Measurements of the cosmic-ray hydrogen and helium spectra at energies from 20 to 800 TeV are presented. The experiments were performed on a series of twelve balloon flights, including several long duration Australia to South America and Antarctic circumpolar flights. No clear evidence is seen for a spectral break. Both the hydrogen and the helium spectra are consistent with power laws over the entire energy range, with integral spectral indices 1.80 +/- 0.04 and 1.68(-0.06)(+0.04) for the protons and helium, respectively. The results are fully consistent with expectations based on supernova shock acceleration coupled with a "leaky box" model of propagation through the Galaxy.
引用
收藏
页码:278 / 283
页数:6
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