he在西大西洋的分布

W.J. Jenkins , W.B. Clarke
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引用次数: 124

摘要

对250多个大西洋海水样本的溶解氦同位素进行了分析,并出现了独特的模式。过量的氦有两种成分:一种是由核时代氚的原位衰变产生的,另一种是由固体地球演化而来的原始成分。从北纬5°到赤道的西侧边界处,约3公里深处有一个突出的特征。这种特征的来源很可能是在吉布斯断裂带,我们认为原始的3He被释放到向西流动的底水中。南大西洋剖面清楚地显示了富含3he的环极水的影响,这些水是由向北流动的南极中间水携带的。当与o¨stlund, Dorsey和Rooth (1974, Earth and Planetary Science Letters, 23, 69-86)在相同位置和深度测量的氚浓度相结合时,上层1公里的过量3He产生了“氚-氦年龄”,在某些情况下,它代表了与大气平衡和采样之间的时间间隔。
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The distribution of 3He in the western Atlantic ocean

Over 250 samples of Atlantic seawater have been analyzed for the dissolved helium isotopes, and distinctive pattern has emerged. Two components of excess 3He are seen: a component due to in situ decay of nuclear-era tritium, and a primordial component evolved from the solid Earth. A prominent feature at about 3-km depth can be traced from 5°N along the western boundary to the equator. The source of this feature is most probably in the Gibbs fracture zone, where we suppose that primordial 3He is released into westward-flowing bottom water. The South Atlantic profiles clearly show the effect of 3He-rich CCircumpolar Water, entrained by Antarctic Intermediate Water flowing northward. The excess 3He in the upper 1 km, when combined with tritum concentrations measured byO¨stlund, Dorsey and Rooth (1974, Earth and Planetary Science Letters, 23, 69–86) at the same locations and depths, yields ‘tritium-helium ages’, which in some cases represent the time interval between equilibration wwith the atmosphere and sampling.

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