Cosmic ray reentrant electron albedo: High-Energy Antimatter Telescope balloon measurements from Fort Sumner, New Mexico

被引:14
作者
Barwick, SW [1 ]
Beatty, JJ
Bower, CR
Chaput, CJ
Coutu, S
de Nolfo, GA
DuVernois, MA
Ficenec, D
Knapp, J
Lowder, DM
McKee, S
Muller, D
Musser, JA
Nutter, SL
Schneider, E
Swordy, SP
Tarle, G
Tomasch, AD
Torbet, E
机构
[1] Univ Calif Irvine, Dept Phys, Irvine, CA 92717 USA
[2] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
[3] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[4] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA
[5] Univ Michigan, Dept Phys, Randall Lab, Ann Arbor, MI 48109 USA
[6] Millenium Pharmaceut Inc, Cambridge, MA 02140 USA
[7] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[8] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[9] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[10] Eastern New Mexico Univ, Dept Phys Sci, Portales, NM 88130 USA
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1998年 / 103卷 / A3期
关键词
D O I
10.1029/97JA03174
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The High-Energy Antimatter Telescope (HEAT) balloon cosmic ray detector flew from Fort Sumner, New Mexico on May 3-5, 1994. The instrument measured electron and positron abundances and spectra from similar to 1 to 100 GeV at a vertical geomagnetic cutoff rigidity that varied between 4.0 and 4.5 GV. The intensities of electrons and positrons have been measured as a function of atmospheric depth between 3.8 and 7.4 g cm(-2) of overburden. At magnetic rigidities below cutoff, the intensity of downward moving e(+/-) consists of secondary (spallogenic) particles and the reentrant (or return) albedo. We determine the contribution of the reentrant electron albedo and compare it with earlier measurements and limits at similar geomagnetic cutoff levels. In the range of 1.0-2.4 GeV, the reentrant albedo component amounts to 40% of the total electron intensity observed.
引用
收藏
页码:4817 / 4823
页数:7
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