首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Evidence for large century time-scale changes in solar activity in the past 32 Kyr, based on in-situ cosmogenic C-14 in ice at Summit, Greenland
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Evidence for large century time-scale changes in solar activity in the past 32 Kyr, based on in-situ cosmogenic C-14 in ice at Summit, Greenland

机译:根据格陵兰萨米特峰在冰上的原位宇宙成因C-14,过去32年以来太阳活动在世纪大尺度上发生了变化的证据

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We present results of estimates of cosmic ray flux in Greenland at the Summit (3200 m.a.s.l, 72.6 degrees N, 38.5 degrees W), during the past 32 Kyr. We derive these estimates based on concentrations of in-situ cosmogenic C-14 produced in ice crystals. Based on the secular equilibrium concentration of in-situ produced C-14 in quartz in terrestrial rocks, we find that on century time-scales, the cosmic ray production rate of C-14 at the Summit was close to its estimated long-term average production rate, except during 3 periods: (i) during 8500-9500 yr B.P. and 27,000-32,000 yr BY, when the production rate was higher by about a factor of 2, and (ii) during 12,000-16,000 yr BY, when the production rate was lower by a factor of similar to 1.5. The observed variation in cosmic ray flux at the polar site is best attributed to changes in solar activity resulting in variable modulation of terrestrial cosmic ray flux. Changes in the geomagnetic field in the past do not affect the cosmic ray flux at polar latitudes. Likewise, climate changes do not affect the in-situ C-14 record in ice.During the first two epochs, the solar activity must have been very low, as during Maunder Minimum (virtually no sunspots), resulting in essentially no modulation of the cosmic ray flux by the solar plasma. During the low cosmic ray flux epoch, 12,000-16,000 yr B.P., the observed decrease in cosmic ray flux corresponds to high solar activity as seen in 1958 (sunspot number similar to 190).We discuss the proxy evidence from tree ring and sediment based records of atmospheric C-14/C-12 ratios during the three epochs. These records have been used as a measure of changes in cosmic ray flux, and solar activity in the past. However, since they are also appreciably affected by climatic changes, a comparison of the two records is potentially valuable for delineating the nature of past changes in solar activity, and large-scale ocean circulation and air-sea exchange. (c) 2005 Elsevier B.V. All rights reserved.
机译:在过去的32年中,我们提供了格陵兰在首脑会议(3200 m.a.s.l,72.6度,W 38.5度)上的宇宙射线通量的估计结果。我们基于冰晶中产生的原位宇宙成因C-14的浓度得出这些估计值。根据地球岩石中石英中原位生成的C-14的长期平衡浓度,我们发现,在一个世纪的时间尺度上,Summit上C-14的宇宙射线产生速率接近其估计的长期平均值生产率,以下三个时期除外:(i)在8500-9500年BP (27,000)BY,当生产率提高约2倍时;(ii)12,000-16,000 yr BY,生产率降低约1.5倍。在极地观测到的宇宙射线通量的变化最好归因于太阳活动的变化,从而导致对地面宇宙射线通量的可变调制。过去,地磁场的变化不会影响极纬度的宇宙射线通量。同样,气候变化也不会影响冰中C-14的原位记录。在前两个时期,太阳活动一定很低,如Maunder Minimum期间(几乎没有黑子),因此基本上没有调制太阳等离子体产生的宇宙射线通量。在12,000-16,000 BP的低宇宙射线通量时期,观测到的宇宙射线通量下降对应于1958年观测到的高太阳活动(太阳黑子数类似于190)。我们讨论了基于年轮和沉积物记录的替代证据三个时期的大气C-14 / C-12比值这些记录已被用作过去宇宙射线通量和太阳活动变化的量度。但是,由于它们还受到气候变化的明显影响,因此比较这两个记录对于描述过去太阳活动,大规模海洋环流和海-气交换的变化的性质具有潜在的价值。 (c)2005 Elsevier B.V.保留所有权利。

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