宇宙气暴对西阿尔卑斯、Viso山地区过敏原基质(土壤)发育的影响

IF 0.6 Q4 GEOSCIENCES, MULTIDISCIPLINARY Studia Quaternaria Pub Date : 2018-06-01 DOI:10.2478/squa-2018-0001
W. Mahaney, L. West, Alison Milan, D. Krinsley, P. Somelar, S. Schwartz, M. Milner, C. Allen
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引用次数: 6

摘要

虽然关于Viso山西阿尔卑斯地区的宇宙撞击事件已经写了很多,该事件与12.8 ka的新仙女木边界(YDB)和新仙女木(YD)的开始密切相关,但受影响的陆地表面被认为包含在三个大陆上发现的类似的黑色垫层沉积物。虽然其他地方的工作主要集中在从湖泊和冰芯中回收的沉积物,埋藏的湖泊/冲积记录,以及表面冰川和副冰川记录,但没有人追踪沉积物的山脉形态序列,目的是研究地表受到高温时发生在YDB的冰消退沉积物中的初始风化/土壤形态形成,这可能是Mahaney等人(2016a)从宇宙空气爆炸中假设的。在b ølling- allero ød间冰期,随着冰川退缩,陆地表面迅速无冰,~13.5 ~ 12.8 ka的风化过程导致了陆地表面逐渐无冰的风化和土壤形态形成。为了确定alallerd中晚期的暴露土地特征,可以利用反向地层土壤形态发生的时间回溯,从已知的小冰期(LIA)(即时间零)到LIA (~0.45 ~ ~0.10 ka),至少到新冰期中期(~2 ka),来回答几个问题。在宇宙撞击/空气爆炸(YDB)之前,在Allerød结束时可能存在的土壤剖面状态是什么?假设这些晚期allero ød的未成熟风化风化剖面近似于今天看到的<1 ka旧剖面,并且假设地表在~12.8 ka时遭受了一个假设的瞬间温度从环境温度上升到~2200°C,那么对常驻沉积物的预期影响是什么?为了验证中lg (YDB)与YD的关系,我们对中lg—YD两套沉积物的古土壤进行了分析,验证了气爆颗粒局限于晚Allerød古土壤,并利用相对年龄测定标准验证了重叠的YD—中lg冰碛在时间上密切相关。这些都是关于黑垫的一些问题,我们试图通过参考Mt. Viso地区的Guil河上游和Po河来回答这些问题。
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Cosmic Airburst on Developing Allerød Substrates (Soils) in the Western Alps, Mt. Viso Area
Abstract Although much has been written about a cosmic impact event in the Western Alps of the Mt. Viso area, the event closely tied with the Younger Dryas Boundary (YDB) of 12.8 ka and onset of the Younger Dryas (YD), the affected land surface is considered to contain a similar black mat suite of sediment found on three continents. While work elsewhere has focused on recovered sediment from lake and ice cores, buried lacustrine/alluvial records, and surface glacial and paraglacial records, no one has traced a mountain morphosequence of deposits with the objective of investigating initial weathering/ soil morphogenesis that occurred in ice recessional deposits up to the YDB when the surface was subjected to intense heat, presumably, as hypothesized by Mahaney et al. (2016a) from a cosmic airburst. With the land surface rapidly free of ice following glacial retreat during the Bølling-Allerød interstadial, weathering processes ~13.5 to 12.8 ka led to weathering and soil morphogenesis in a slow progression as the land surface became free of ice. To determine the exposed land character in the mid- to late-Allerød, it is possible to utilize an inverted stratigraphic soil morphogenesis working backward in time, from known post-Little Ice Age (LIA) (i.e. time-zero) through LIA (~0.45 to ~0.10 ka), to at least the middle Neoglacial (~2 ka), to answer several questions. What were the likely soil profile states in existence at the end of the Allerød just prior to the cosmic impact/airburst (YDB)? Assuming these immature weathered regolith sections of the Late Allerød approximated the <1 ka old profiles seen today, and assuming the land surface was subjected to a hypothesized instant temperature burst from ambient to ~2200°C at ~12.8 ka, what would be the expected effect on the resident sediment? To test the mid-LG (YDB) to YD relationship we analyzed the paleosols in both suites of deposits - mid-LG to YD - to test that the airburst grains are restricted to Late Allerød paleosols and using relative-age-determination criteria, that the overlapping YD to mid-LG moraines are closely related in time. These are some of the questions about the black mat that we seek to answer with reference to sites in the upper Guil and Po rivers of the Mt. Viso area.
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来源期刊
Studia Quaternaria
Studia Quaternaria GEOSCIENCES, MULTIDISCIPLINARY-
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期刊介绍: Studia Quaternaria is designed to publish scientific works concerning the Quaternary, on local, regional and global scale. Studia Quaternaria is interested in all fields of research dealing with stratigraphy and reconstruction of the past environments, including palaeogeography, palaeoecology, palaeoclimatology, palaeohydrology etc. The journal is also open to studies of natural environmental processes, and to recognition of mechanisms involved in the dynamics of our environment. The clue is that the Quaternary is still ongoing and vivid, and understanding of its past and present development support each other.
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