COSMIC-RAY ABUNDANCES OF ELEMENTS WITH ATOMIC-NUMBER 26 LESS-THAN Z LESS-THAN 40 MEASURED ON HEAO-3

被引：31

作者：

BINNS, WR

FICKLE, RK

GARRARD, TL

ISRAEL, MH

KLARMANN, J

STONE, EC

WADDINGTON, CJ

机构：

[1] WASHINGTON UNIV,MCDONNELL CTR SPACE SCI,ST LOUIS,MO 63110

[2] MCDONNELL DOUGLAS CORP,MCDONNELL DOUGLAS RES LABS,ST LOUIS,MO 63166

[3] UNIV MINNESOTA,SCH PHYS & ASTRON,MINNEAPOLIS,MN 55455

[4] CALTECH,DOWNS LAB,PASADENA,CA 91125

来源：

ASTROPHYSICAL JOURNAL | 1981年 / 247卷 / 03期

关键词：

D O I：

10.1086/183602

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L115 / L118

页数：4

共 42 条

[31] THE ELEMENTAL COMPOSITION OF COSMIC-RAY NUCLEI FROM 1-10 GEV-NUC FOR 7 LESS-THAN-OR-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 28
DWYER, R
MEYER, P
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1980, 25 (04): : 564 - 564
[32] X-RAY-PRODUCTION FOR SELECTED ELEMENTS FROM Z= 29 TO Z= 51 IN THE REGION WHERE IK-E LESS-THAN .1 FOR INCIDENT PROTONS DEUTERONS AND ALPHA-PARTICLES
RICE, R
BASBAS, G
DUGGAN, JL
MCDANIEL, FD
MEHTA, R
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1979, 24 (09): : 1197 - 1198
[33] INTERSTELLAR PROPAGATION OF GALACTIC COSMIC-RAY NUCLEI 2 LESS-THAN-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 8 IN ENERGY RANGE 10-1000 MEV PER NUCLEON
MASON, GM
ASTROPHYSICAL JOURNAL, 1972, 171 (01): : 139 - &
[34] GAMMA-RAY SELF-ABSORPTION CORRECTIONS FOR E-GAMMA GREATER-THAN 0.6 MEV AND MU LESS-THAN 3CM-1
HOROWITZ, YS
MORDECHAI, S
DUBI, A
NUCLEAR INSTRUMENTS & METHODS, 1974, 122 (03): : 399 - 404
[35] MEASUREMENTS OF L X-RAY-FLUORESCENCE CROSS-SECTIONS AND YIELDS FOR ELEMENTS IN THE ATOMIC RANGE 41-LESS-THAN-OR-EQUAL-TO-Z-LESS-THAN-OR-EQUAL-TO-52 AT 5.96 KEV
GARG, RR
PURI, S
SINGH, S
MEHTA, D
SHAHI, JS
GARG, ML
SINGH, N
MANGAL, PC
TREHAN, PN
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS, 1992, 72 (02): : 147 - 152
[36] PHASE-DIAGRAM OF KMN1-XCAXF3(X LESS-THAN 0.05) DETERMINED BY HIGH-RESOLUTION X-RAY-SCATTERING
GIBAUD, A
SHAPIRO, SM
NOUET, J
YOU, H
PHYSICAL REVIEW B, 1991, 44 (06): : 2437 - 2443
[37] OBSERVATIONS OF HIGH-DENSITY EFFECTS ON SPECTRAL-LINE SHAPES IN A DENSE (NE LESS-THAN 1018CM-3) Z-PINCH DISCHARGE
BAKER, EAM
BURGESS, DD
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1979, 12 (13) : 2097 - 2113
[38] COSMIC-RAY ENERGY-SPECTRA BETWEEN 10 AND SEVERAL HUNDRED GEV PER ATOMIC MASS UNIT FOR ELEMENTS FROM AR-18 TO NI-28 - RESULTS FROM HEAO-3
BINNS, WR
GARRARD, TL
ISRAEL, MH
JONES, MD
KAMIONKOWSKI, MP
KLARMANN, J
STONE, EC
WADDINGTON, CJ
ASTROPHYSICAL JOURNAL, 1988, 324 (02): : 1106 - 1117
[39] A COMPARISON OF SECONDARY-ELECTRON YIELDS FROM ACCELERATED WATER CLUSTED IONS (M/Z LESS-THAN 50 000) STRIKING AL2O3 AND COPPER SURFACES
BEUHLER, RJ
JOURNAL OF APPLIED PHYSICS, 1983, 54 (07) : 4118 - 4126
[40] Measurement of M shell X-ray production cross sections and fluorescence yields for the elements in the atomic range 70<=Z not less than or equal to 92 at 5.96 keV
Ertugrul, M
Tirasoglu, E
Kurucu, Y
Erzeneoglu, S
Durak, R
Sahin, Y
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS, 1996, 108 (1-2): : 18 - 22

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