EFFECTIVE ATTENUATION LENGTHS OF COSMIC-RAYS PRODUCING BE-10 AND AL-26 IN QUARTZ - IMPLICATIONS FOR EXPOSURE AGE DATING

被引:119
|
作者
BROWN, ET [1 ]
BROOK, EJ [1 ]
RAISBECK, GM [1 ]
YIOU, F [1 ]
KURZ, MD [1 ]
机构
[1] WOODS HOLE OCEANOG INST,DEPT CHEM,WOODS HOLE,MA 02543
关键词
D O I
10.1029/92GL00266
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We have measured cosmic ray produced Be-10 (t1/2 = 1.5 My) and Al-26 (t1/2 = 0.72 My) as functions of depth in a core of quartz sandstone bedrock collected in South Victoria Land, Antarctica. These data were used to place limits on the exposure age and erosion rate of the exposed surface, and to calculate the effective attenuation lengths of cosmic rays producing these nuclides. These latter results indicate that the production attenuation length for Al-26 (156 +13/-12 g cm-2) is comparable to that for Be10 (145 +8/-6 g cm2 This suggests that the production ratio Al-26:Be-10 does not vary substantially with depth in a rock, and that its value at the surface of exposed rock is not strongly affected by erosional losses, allowing wider use of the ratio in determining exposure ages.
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页码:369 / 372
页数:4
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共 35 条
  • [1] PRODUCTION OF BE-10 AND AL-26 BY COSMIC-RAYS IN TERRESTRIAL QUARTZ INSITU AND IMPLICATIONS FOR EROSION RATES
    NISHIIZUMI, K
    LAL, D
    KLEIN, J
    MIDDLETON, R
    ARNOLD, JR
    [J]. NATURE, 1986, 319 (6049) : 134 - 136
  • [2] BE-10 AND AL-26 IN INDIVIDUAL COSMIC SPHERULES
    NISHIIZUMI, K
    ARNOLD, JR
    CHAFFEE, MW
    FINKEL, RC
    SOUTHON, J
    BROWNLEE, DE
    HARVEY, RP
    [J]. METEORITICS, 1992, 27 (03): : 269 - 270
  • [3] BE-10 ABUNDANCE AND AGE OF COSMIC-RAYS - BALLOON MEASUREMENT
    HAGEN, FA
    FISHER, AJ
    ORMES, JF
    [J]. ASTROPHYSICAL JOURNAL, 1977, 212 (01): : 262 - 277
  • [4] BE-10 AND AL-26 IN INDIVIDUAL COSMIC SPHERULES FROM ANTARCTICA
    NISHIIZUMI, K
    ARNOLD, JR
    BROWNLEE, DE
    CAFFEE, MW
    FINKEL, RC
    HARVEY, RP
    [J]. METEORITICS, 1995, 30 (06): : 728 - 732
  • [5] New interpretation of the Be-10 and Al-26 content in cosmic spherules
    Zoppi, U
    Matsuzaki, H
    Kobayashi, K
    Imamura, M
    Nagai, H
    Hatori, S
    Nakano, C
    Sunohara, Y
    [J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS, 1997, 123 (1-4): : 319 - 323
  • [6] AGE OF GALACTIC COSMIC-RAYS DERIVED FROM ABUNDANCE OF BE-10
    GARCIAMUNOZ, M
    MASON, GM
    SIMPSON, JA
    [J]. ASTROPHYSICAL JOURNAL, 1977, 217 (03): : 859 - 877
  • [7] DATA ON AL-26 COSMOGENIC ISOTOPE AND INTENSITY OF COSMIC-RAYS IN PAST
    BLINOV, AV
    KONSTANTINOV, AN
    [J]. IZVESTIYA AKADEMII NAUK SSSR SERIYA FIZICHESKAYA, 1977, 41 (02): : 446 - 452
  • [8] COSMIC-RAY PRODUCED BE-10 AND AL-26 IN ANTARCTIC ROCKS - EXPOSURE AND EROSION HISTORY
    NISHIIZUMI, K
    KOHL, CP
    ARNOLD, JR
    KLEIN, J
    FINK, D
    MIDDLETON, R
    [J]. EARTH AND PLANETARY SCIENCE LETTERS, 1991, 104 (2-4) : 440 - 454
  • [9] BE-10 AND AL-26 CONTENTS OF EUCRITES - IMPLICATIONS FOR PRODUCTION-RATES AND EXPOSURE AGES
    AYLMER, D
    HERZOG, GF
    KLEIN, J
    MIDDLETON, R
    [J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 1988, 52 (06) : 1691 - 1698
  • [10] Stable magnesium isotopes, Al-26, Be-10, and Mg-26/Al-26 exposure ages of iron meteorites
    Xue, S
    Herzog, GF
    Souzis, A
    Ervin, MH
    Lareau, RT
    Middleton, R
    Klein, J
    [J]. EARTH AND PLANETARY SCIENCE LETTERS, 1995, 136 (3-4) : 397 - 406