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

被引：32

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

[21] COSMIC-RAY ABUNDANCES FOR Z GREATER-THAN 60 - HEAO-O HEAVY-NUCLEI EXPERIMENT
WADDINGTON, CJ
BINNS, WR
FICKLE, R
GARRARD, TL
ISRAEL, MH
KLARMANN, J
STONE, EC
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1980, 25 (04): : 563 - 563
[22] EFFECTS OF PARTIAL DECONVOLUTION OF THE UHCRE DATA ON THE INFERRED R-PROCESS CONTRIBUTION TO COSMIC-RAY ABUNDANCES FOR 74-LESS-THAN-OR-EQUAL-TO-Z-LESS-THAN-OR-EQUAL-TO-86
BOSCH, J
EISLOFFEL, J
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1995, 361 (1-2): : 342 - 348
[23] ENERGY-SPECTRA AND ABUNDANCES OF COSMIC-RAY NUCLEI 24 LESS-THAN-OR-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 28 FOR ENERGIES ABOVE 1 GEV-AMU
MEYER, P
MINAGAWA, G
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1980, 25 (04): : 564 - 564
[24] TESTS FOR ORIGIN AND TRANSFORMATIONS OF COSMIC-RAYS WITH 3 LESS-THAN-OR-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 40
TSAO, CH
ADAMS, JH
SHAPIRO, MM
SILBERBERG, R
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1981, 26 (04): : 556 - 556
[25] EVIDENCE FOR DIFFERENCES IN THE THERMAL HISTORIES OF ANTARCTIC AND NON-ANTARCTIC H-CHONDRITES WITH COSMIC-RAY EXPOSURE AGES LESS-THAN 20 MA
SEARS, DWG
BENOIT, P
BATCHELOR, JD
GEOCHIMICA ET COSMOCHIMICA ACTA, 1991, 55 (04) : 1193 - 1197
[26] RIGIDITY DEPENDENCE OF RELATIVE ELEMENTAL ABUNDANCES OF COSMIC-RAYS (3 LESS-THAN-OR-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 8)
BROWN, JW
STONE, EC
VOGT, RE
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1973, 18 (04): : 540 - 540
[27] STUDY OF FOSSIL TRACKS DUE TO 50-LESS-THAN-OR-EQUAL-TO-Z-LESS-THAN-OR-EQUAL-TO-92 GALACTIC COSMIC-RAY NUCLEI IN EXTRATERRESTRIAL CRYSTALS - RESULTS AND PERSPECTIVES
PERELYGIN, VP
CHARGE COMPOSITION OF ULTRA HEAVY NUCLEI, 1995, 15 (06): : 15 - 24
[28] ENERGY-SPECTRA OF COSMIC-RAY NUCLEI - 4LESS-THAN-OR-EQUAL-TO26 AND 0.3LESS-THAN-OR-EQUAL-TOELESS-THAN-OR-EQUAL-TO2 GEV AMU-1
MAEHL, RC
ORMES, JF
FISHER, AJ
HAGEN, FA
ASTROPHYSICS AND SPACE SCIENCE, 1977, 47 (01) : 163 - 184
[29] ATOMIC BINDING-ENERGIES FROM APPROXIMATE RELATIONS INVOLVING LESS-THAN R-1 GREATER-THAN AND THE Z-1 PERTURBATION EXPANSION
CASTRO, EA
FERNANDEZ, FM
GAZZETTA CHIMICA ITALIANA, 1982, 112 (1-2): : 39 - 41
[30] EXTENSION OF THE ANALYTICAL RANGE OF TOTAL REFLECTION X-RAY-FLUORESCENCE SPECTROMETRY TO LIGHTER ELEMENTS (11 LESS-THAN-OR-EQUAL-TO Z LESS-THAN 16) AND INCREASE IN SENSITIVITY BY EXCITATION WITH TUNGSTEN L-ALPHA RADIATION
FREITAG, K
REUS, U
FLEISCHHAUER, J
SPECTROCHIMICA ACTA PART B-ATOMIC SPECTROSCOPY, 1989, 44 (05) : 499 - 504

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