峨眉山大火成岩省二滩玄武岩地球化学及源区特征

大陆溢流玄武岩根据TiO2含量可划分为高钛玄武岩和低钛玄武岩，这两种不同类型的玄武岩往往有不同的空间分布特征，也具有不同的成因指示意义。峨眉山玄武岩也有高、低钛之分，且其空间分布存在明显差异。然而，在以往的峨眉山玄武岩的研究中只对高、低钛玄武岩进行对比研究，而单独对同一类型玄武岩的研究甚少，尤其是对物质来源的研究。在本论文中，作者以峨眉山大火成岩省中部二滩地区高钛玄武岩为研究对象，通过主量元素、微量元素和Sr－Nd－Pb同位素对其地球化学、岩浆过程以及物质来源进行了探讨，得出以下初步认识和结论： ⑴ 二滩高钛玄武岩可划分出Group I和Group II两种岩石类型。Group I中Sr和Zr显示明显负异常，而Group II无Sr和Zr异常。此两种类型岩石的Sr－Nd－Pb同位素地球化学特征也较为不同。 ⑵ 二滩高钛玄武岩为板内构造环境，Group I和Group II显示出碱性或钙碱性岩特征。 ⑶ Group I和Group II具有不同的熔体形成熔融程度，Group I相对低(0～3.5％)，Group II相对高(4.0～8.0％)。不同的部分熔融程度导致了控制矿物相的不同。 ⑷ Group I和Group II岩浆分别经历了不同的结晶分异过程。Group I主要显示出斜长石结晶分异趋势，Group II则主要显示出橄榄石结晶分异趋势。 ⑸ 微量不相容元素和Sr－Nd－Pb同位素特征表明，Group I和Group II均源自深部富集地幔，具有不同的物质来源，且与地幔柱有成因上的联系。 以上特征表明，二滩玄武岩与深源地幔柱有成因上的联系。这可能是深部地幔柱(来自核－幔边界或下地幔)上升过程中在不同深度携带了不同物质，这些物质发生部分熔融，从而导致了Group I和Group II的明显差异。其充分说明，二滩高钛玄武岩的物源是不均一的，反映了源区的不均一性特征。

峨眉山大火成岩省Ni-Cu-PGE矿床矿化类型变异机理研究

在峨眉山大火成岩省（ELIP）产出许多岩浆Cu-Ni-PGE岩浆硫化物矿床，如金宝山、杨柳坪、力马河、白马寨，以及大槽－阿布郎当矿化岩体。根据成矿元素组成特征，这些矿床可以区分为多种不同矿化类型，有以铂族元素为主贫铜镍的矿床，如金宝山Pt-Pd矿床；有含较高铂族元素和铜镍的矿床，如杨柳坪Ni-Cu-PGE矿床；也有贫铂族元素富铜镍的矿床，以力马河和白马寨Ni-Cu矿床最为典型。造成峨眉山大火成岩省中Ni-Cu-PGE岩浆硫化物矿床矿化类型变异的原因是什么？它们的母质岩浆性质如何，产生于怎样的熔融程度？既然能形成岩浆硫化物矿床，造成硫化物熔离的原因有哪些，什么因素起到了关键作用？这些矿化类型多样的Ni-Cu-PGE矿床的成矿岩浆有何差异？产生差异的原因是什么？带着这些疑问，通过借鉴国内外Ni-Cu-PGE岩浆硫化物矿床研究的经验，本文以金宝山铂钯矿、力马河镍矿及大槽－阿布郎当岩体的地球化学研究为基础，结合近几年来前人对杨柳坪，白马寨等矿床的系统研究，本文试图解决上述疑问。现在取得的主要认识有： 1） 根据成矿元素组成特征，可以把峨眉山大火成岩省中（ELIP）存在的Ni-Cu-PGE岩浆硫化物矿床分成多种不同的矿化类型，包括PGE矿床（例如金宝山Pt-Pd矿），Ni-Cu-PGE矿床（例如杨柳坪矿床），Ni-Cu矿床（例如力马河和白马寨矿床），以及弱矿化或不含矿的超镁铁质堆晶岩体（例如大槽－阿布郎当岩体）。通过对ELIP中几种类型Cu-Ni-PGE矿床成矿母岩浆的研究发现，它们均具有类似峨眉山苦橄岩的成分特征，表明母岩浆形成于较高程度的地幔部分熔融，并富集Ni和PGE。 2）硫化物熔离的多阶段性是导致矿床类型变异的一个重要因素。早期结晶矿物的分离结晶导致了金宝山母岩浆出现S的饱和，少量的浸染状硫化物被携带进入岩浆通道中发生了沉淀，继续富集PGE，形成了金宝山矿体。杨柳坪的母岩浆先发生了少量早期硫化物熔离丢失，PGE弱亏损的岩浆在后期上升过程中由于强烈的地壳混染，发生了大量硫化物熔离并发生堆积，形成杨柳坪矿体。力马河和白马寨的母岩浆在早期发生了较多的硫化物丢失，PGE强烈亏损的岩浆发生了二次以上的硫化物熔离，形成了力马河和白马寨矿体。 3） R因子（岩浆与熔离硫化物的比例）是决定ELIP中Cu-Ni-PGE矿床矿化类型变异的重要因素。金宝山矿床具有极高的R值（＞10000），杨柳坪和朱布矿床具有中等的R值（2000~5000），而力马河矿床近似为在经过R=2000的硫化物熔离之后，残余岩浆再经过R=200的硫化物熔离。 4） 地壳混染程度的差异可能是造成ELIP中Ni-Cu-PGE矿床矿化类型发生变异的关键因素。金宝山矿床的地壳混染程度较低，可能主要是早期橄榄石和铬铁矿的分异结晶导致了岩浆中硫化物出现了饱和。对于大槽－阿布郎当矿化岩体，只是在岩体边缘的局部出现了硫化物熔离，可能是围岩混染造成的。对于杨柳坪Ni-Cu-PGE矿床、力马河和白马寨Ni-Cu矿床，从微量元素蛛网中明显的Nb-Ta负异常，高放射成因187Os丰度的初始Os同位素组成（γOs(t)=100~120），S同位素等反映出显著的地壳混染，因而出现大量硫化物熔离。

地幔柱与岩浆成矿-峨嵋山大火成岩省地震波速层物相解释及典型PGE矿床成岩成矿机制研究

地幔柱概念在19世纪60至70年代就被提出，但是由于板块构造理论在解释地球上岩浆活动的分布规律时取得了空前的成功，在当时这一理论是被排斥的。板块边界概念可以解释地球上绝大部分的岩浆产出，但在解释板内岩浆的成因时往往显得力不从心，尽管这些岩浆的体积只占地球岩浆总量的2％。地幔柱理论模型发展到现在得到不同学科的支持。地质学、地球化学、地球物理学、古生物学、比较行星学、实验岩石学等等都提供了直接或间接的证据，证明地幔柱几乎存在整个地：质历史时期。当前地幔柱理论中在地球化学领域有两大研究热点：高钦低钦玄武岩的起源以及地幔柱中是否存在循环俯冲洋壳物质。完全解决这些问题才可能深入系统地建立地慢柱成矿作用模型。现在已经建立了一些矿床类型与地慢柱作用的联系：如现在认为赋存在金伯利岩中的金刚石矿床的形成与地慢柱作用密不可分，一些岩浆硫化物矿床和岩浆氧化物矿床很显然是地慢柱岩浆作用形成的，如西伯利亚火成岩省的Noril'sk-Talnakh铜镍铂族元素矿床以及KeweenawaJI大陆裂谷体系的Dultlth杂岩体的Cu-Ni矿床。另外还有赋存在大型基性一超基性层状岩体中的PGE、Ni和cu矿床，如Great Dyke和布什维尔德杂岩体。一些超大型热液矿床也与地慢柱有可能的联系（Pirajno，2000）：如270oMa形成的超大型Kidd Creek火山成因块状硫化物矿床（Bleeker et al.，1 999；Wynan et al.，1999）和南澳大利亚1600Ma形成的超大型olymPicD翻矿床。本文的研究工作包含两方面内容：通过热力学计算峨眉山玄武岩在深部的结晶分异，对峨眉山大火成岩省的岩浆量分布和岩浆氧化物矿床（华Ti磁铁矿矿床）的分布以及下地壳高波速层的物相进行理论解释；对峨眉山大火成岩省金宝山PGE典型矿床进行成岩成矿的地球化学研究，预测整个大火成岩省的岩浆硫化物矿床产出位置。大多数峨眉山玄武岩的 MgO＜7％，Ni为4-232ppm，它们是原始岩浆结晶分异后的产物。峨眉山玄武岩省下地壳和上地幔之间存在厚度为：8-25km1，P彼速为7.1-7.8km／s的附加层（高地震波速层）。滇西地区出露的洲套第三纪富碱斑岩，地球化学和同位素研究表明斑岩的岩浆源是来自“壳一慢混合层”，源区的形成时代为220-25Ma，与峨眉山玄武岩的形成时代一致。所以有理由认为该附加层是由峨眉山玄武岩在此结晶分异形成的。与地慢柱有关的洋岛Hawaii、Marquesas Islands；海底高原Oniong Java、大陆火山岩省ColumbiaRiver Plateaus地震彼研究都表明在上地慢顶部有一高速附加层，Farnetani etal.（1996）的研歼表明高速附加层是由来自地幔柱的岩浆在此结晶分异形成的。玄武岩是一种混合的部分熔融产物，是不同成分的地幔橄榄岩在不同的压力下熔出的。这种降压熔融高温高压实验是做不到的。熔出的熔体成分是温度、压力及橄榄岩成分（源区）的函数，形成的岩浆是一个多压熔融的集合体。热力学计算能够较为精确地计算出生成的岩浆成分和约束岩浆产生的过程。岩浆的结晶分异也是同样的情形，尤其是分离结晶过程，实验岩石学是很精确难模拟其过程的。热力学计算使用的MELTS程序，MELTS适用范围很广，适用于模拟岩石熔融生成岩浆和岩浆的冷却结晶。现今峨眉山大火成岩省的地壳厚度为40恤，这被认为是后期褶皱加厚的缘故。根据峨眉山玄武岩中辉石斑晶成分和玄武岩本身成分计算出分异结晶的压力为6kb，那么当时的地壳厚度约为20km：选择氧逸度为QFM，这一氧逸度范围认为是大多数大陆溢流玄武岩结晶分异时的氧化还原环境。热力学计算结果通过峨眉山玄武岩成分进行约束和验证。Al2O3、NaZO＋K 20、CaO与MgO计算的演化趋势线与实际观察的演化符合较好，橄榄石和斜方辉石的结晶使得CaO随着MgO的降低而增高；当单斜辉石成为液相线矿物时，cao也随着Mgo的降低而降低了。单斜辉石在岩浆演化到MgO＝10．3％时成为液相线矿物。整个计算过程中斜长石未成为液相线矿物，这与大多数玄武岩不具有Eu异常是一致的，并月＿Al2O3随着MgO的减小单调增加也说明了这点。不过大多数峨眉山玄武岩常含有斜长石斑晶，这是低压下结晶分异的结果。由于斜长石密度小，所有很难与高铁玄武岩分离。整个计算的难点也是创新点是波速计算。通过分离的堆晶矿物组合中各种矿物的成分和质量分数计算的附加层波速比观察值高，不过堆积岩体常常会有残留岩浆存在矿物晶粒间，这样会降低岩石的压缩波速。大型基性一超基性岩体常常会残留有或者捕获5-30％的岩浆。假定两个高波速附加层分别捕获7叭，和巧％的残留岩浆，计算的结果就大体等于观察值。热力学和质量平衡计算研究表明：高地震波速层为橄榄辉石岩一辉石岩的巨型侵入岩体；峨眉山中岩区的岩浆量最大也符合含V-Ti磁铁矿矿床只产在中岩区，如太和、白马、攀枝花、红格等岩体；西岩区的岩浆量最小表明几乎没有可能在西岩区形成有规模的V-Ti磁铁矿矿床，实际观察仅仅只见到数量少而小的岩体；东岩区下地壳厚达20灿1的高波速层暗示东岩区上地壳的侵入岩体积也应该具有相当规模，应该是V－Ti磁铁矿矿床成矿区。目前在东岩区很少发现与峨眉山玄武岩有关的岩浆矿床的主要原因是：东岩区的剥蚀深度不够，没有可观的侵入岩体出露，而中岩区侵入岩都侵入在元古代地层中。按照质量平衡的计算方法，最保守的估算整个峨眉地慢柱岩浆事件产生的岩浆量为8.9*106km3，上地壳峨眉山玄武岩和侵入岩体积为3.9*106km3。如果按照初始覆盖面积5x106km2计算（与西伯利亚暗色岩初始覆盖面积相当），喷发高峰期为2Ma，计算的喷发速率为3.9km3／year。这并不亚于西伯利亚暗色岩的喷发速率4km3／year。这对于研究峨眉山大火成岩浆事件与二叠·三叠交界或end-QuadaluPian生物灭绝之间的可能联系具有重要意义。本文另一方面的研究工作是：首先系统地介绍了岩浆硫化物矿床的基本原理，然后通过金宝山PGE矿床实例研究，提出金宝山岩体成岩模式，并且对整个峨眉山大火成岩省的岩浆硫化物矿床产出位置进行理论预测。详细地球化学研究表明金宝山镁铁一超镁铁岩是峨眉山大火成岩省古老火山岩浆房的残留物。岩体主要由底部超镁铁岩和上部镁铁岩组成，两种岩石的质量大致相同。根据超镁铁岩的矿物组合计算的成岩时的氧逸度较高，热力学方法计算的成岩压力为2kb左右。超镁铁岩的包嵌结构和铁铁岩的微晶一细晶结构说明超镁铁岩为镁铁岩结晶的矿物堆积形成的。镁铁一超镁铁岩的蚀变程度不同以及Sc、Sr、Eu等元素在两类岩石中的不同特征指示了整个成岩过程。金宝山岩体的原始岩浆 MgO=8％说明高镁玄武岩并不是形成PGE矿床的必要条件。金宝山的成岩模式是：在火山喷发前，岩浆侵位时橄榄石和少量铬尖晶石先结晶，沉淀在岩浆房底部；随后结晶的是斜方辉石和斜长石，斜方辉石也沉淀在岩浆房底部，斜长石由于密度较小集中中岩浆房上部，岩浆房的中部是：少量的斜长石小斑晶。由于斜方辉石和斜长石的结晶，这样岩浆中的Sc、Sr和Eu就会亏损，也是岩浆房底部堆积岩的原始捕获岩浆。火山喷发后，由于压力的突然降低，岩浆房底部的堆晶会发生再熔融，几乎消耗掉所有的斜方辉石，橄榄石也呈熔蚀状浑圆形态，重新熔融的斜方辉石导致超镁铁岩中残留岩浆比原始捕获岩浆更加富Sc，这种岩浆由于富MgO和在快速冷却的环境下同时结晶，最终形成光性方位一致的单刹辉石。喷发后岩浆房空间的剩余导致围岩-灰岩进入，造成岩浆房中剩余岩浆强烈的碳酸盐化。峨眉山玄武岩Cr-Mg#的相关关系定义一条正常玄武岩演化线。大多数这些玄武岩的Ni也保持了这种演化关系，其中低钦玄武岩和过渡型高钦玄武岩Ni-Mg＃相关关系远离了正常演化线，这些玄武岩的Cu-Mg#相关关系也有类似的情形。峨眉山低钦和过渡类型高钦玄武岩Ni和 Cu的非正常亏损，表明它们在地表下经历了硫饱和事件。金宝山岩浆硫化物矿床成岩模型的建立，为在整个大火成岩省寻找岩浆硫化物矿床提供了一种新认识。低钦和过渡型高钦玄武岩的古老火山口下部是岩浆硫化物矿床的所在地。

Pre-eruptive uplift in the Emeishan? [Correspondence]

In their correspondence, He and colleagues question our conclusion of little or no uplift preceding Emeishan volcanism that we reported in our letter1. Debate concerns the nature of the contact between the Maokou limestone and Emeishan volcanics, the depositional environment and volumetric significance of mafic hydromagmatic deposits (MHDs), and evidence for symmetrical domal thinning. MHDs in the Daqiao section are separated from the Maokou limestone by 100 m of subaerial basaltic lavas, but elsewhere MHDs — previously interpreted as basal conglomerates2, 3 — directly overlie the Maokou2, 3. MHDs thus feature strongly in basal sections of the Emeishan lava succession, as also recently shown4 elsewhere in the Emeishan. An irregular surface at the top of the Maokou limestone has been interpreted as an erosional unconformity2, 3, but clastic deposits presented as evidence of this erosion2, 3 are MHDs produced by explosive magma–water interaction1. A clear demonstration that this irregular top surface is an erosional truncation of limestone reef facies (slope/rim, flat, lagoonal) is currently lacking, but is critical because reefs and carbonate platforms show considerable natural relief of tens of metres. The persistent hot, wet climate since the Oligocene has produced well-developed weathering profiles on exposed Palaeozoic marine sedimentary sequences5, but weathering and karst relief of the uppermost Maokou limestone underlying the flood basalts have not been properly documented, nor shown to be of middle Permian age and immediately preceding emplacement of the large igneous province.

Large igneous provinces and silicic large igneous provinces : progress in our understanding over the last 25 years

Large Igneous Provinces are exceptional intraplate igneous events throughout Earth’s history. Their significance and potential global impact is related to the total volume of magma intruded and released during these geologically brief events (peak eruptions are often within 1-5 Myrs duration) where millions to tens of millions of cubic kilometers of magma are produced. In some cases, at least 1% of the Earth’s surface has been directly covered in volcanic rock, being equivalent to the size of small continents with comparable crustal thicknesses. Large Igneous Provinces are thus important, albeit episodic episodes of new crust addition. However, most magmatism is basaltic so that contributions to crustal growth will not always be picked up in zircon geochronology studies that better trace major episodes of extension-related silicic magmatism and the silicic Large Igneous Provinces. Much headway has been made on our understanding of these anomalous igneous events over the last 25 years, driving many new ideas and models. This includes their: 1) global spatial and temporal distribution, with a long-term average of one event approximately every 20 Myrs, but a clear clustering of events at times of supercontinent break-up – Large Igneous Provinces are thus an integral part of the Wilson cycle and are becoming an increasingly important tool in reconnecting dispersed continental fragments; 2) compositional diversity that in part reflects their crustal setting of ocean basins, and continental interiors and margins where in the latter setting, LIP magmatism can be silicicdominant; 3) mineral and energy resources with major PGE and precious metal resources being hosted in these provinces, as well as magmatism impacting on the hydrocarbon potential of volcanic basins and rifted margins through enhancing source rock maturation, providing fluid migration pathways, and trap formation; 4) biospheric, hydrospheric and atmospheric impacts, with Large Igneous Provinces now widely regarded as a key trigger mechanism for mass extinctions, although the exact kill mechanism(s) are still being resolved; 5) role in mantle geodynamics and thermal evolution of the Earth, by potentially recording the transport of material from the lower mantle or core-mantle boundary to the Earth's surface and being a fundamental component in whole mantle convection models; and 6) recognition on the inner planets where the lack of plate tectonics and erosional processes and planetary antiquity means that the very earliest record of LIP events during planetary evolution may be better preserved than on Earth.

30 million years of Permian volcanism recorded in the Choiyoi igneous province (W Argentina) and their source for younger ash fall deposits in the Parana Basin: SHRIMP U-Pb zircon geochronology evidence

We present four SHRIMP U-Pb zircon ages for the Choiyoi igneous province from the San Rafael Block, central-western Argentina. Dated samples come from the Yacimiento Los Reyunos Formation (281.4 +/- 2.5 Ma) of the Cochico Group (Lower Choiyoi section: andesitic breccias, dacitic to rhyolitic ignimbrites and continental conglomerates). Agua de los Burros Formation (264.8 +/- 2.3 Ma and 264.5 +/- 3.0 Ma) and Cerro Carrizalito Formation (251.9 +/- 2.7 Ma Upper Choiyoi section: rhyolitic ignimbrites and pyroclastic flows) spanning the entire Permian succession of the Choiyoi igneous province. A single ziron from the El Imperial Formation, that is overlain unconformably by the Choiyoi succession, yielded an early Permian age (297.2 +/- 5.3 Ma). while the main detrital zircon population indicated an Ordovician age (453.7 +/- 8.1 Ma). The new data establishes a more precise Permian age (Artinskian-Lopingian) for the section studied spanning 30 Ma of volcanic activity. Volcanological observations for the Choiyoi succession support the occurrence of explosive eruptions of plinian to ultraplinian magnitudes, capable of injecting enormous volumes of tephra in the troposphere-stratosphere. The new SHRIMP ages indicate contemporaneity between the Choyoi succession and the upper part of the Parana Basin late Paleozoic section, from the Irad up to the Rio do Rasto formations, encompassing about 24 Ma. Geochemical data show a general congruence in compositional and tectonic settings between the volcanics and Parana Basin Permian ash fall derived layers of bentonites. Thickness and granulometry of ash fall layers broadly fit into the depletion curve versus distance from the remote source vent of ultraplinian eruptions. Thus, we consider that the Choiyoi igneous province was the source of ash fall deposits in the upper Permian section of the Parana Basin. Data presented here allow a more consistent correlation between tectono-volcanic Permian events along the paleo-Pacific margin of southwestern Gondwana and the geological evolution of neighboring Paleozoic foreland basins in South America and Africa. (C) 2010 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

Geochemistry of North Atlantic Igneous Province basalts

New Sr-Nd-Pb-Hf data require the existence of at least four mantle components in the genesis of basalts from the the North Atlantic Igneous Province (NAIP): (1) one (or more likely a small range of) enriched component(s) within the Iceland plume, (2) a depleted component within the Iceland plume (distinct from the shallow N-MORB source), (3) a depleted sheath surrounding the plume and (4) shallow N-MORB source mantle. These components have been available since the major phase of igneous activity associated with plume head impact during Paleogene times. In Hf-Nd isotope space, samples from Iceland, DSDP Leg 49 (Sites 407, 408 and 409), ODP Legs 152 and 163 (southeast Greenland margin), the Reykjanes Ridge, Kolbeinsey Ridge and DSDP Leg 38 (Site 348) define fields that are oblique to the main ocean island basalt array and extend toward a component with higher 176Hf/177Hf than the N-MORB source available prior to arrival of the plume, as indicated by the compositions of Cretaceous basalts from Goban Spur (~95 Ma). Aside from Goban Spur, only basalts from Hatton Bank on the oceanward side of the Rockall Plateau (DSDP Leg 81) lie consistently within the field of N-MORB, which indicates that the compositional influence of the plume did not reach this far south and east ~55 Ma ago. Thus, Hf-Nd isotope systematics are consistent with previous studies which indicate that shallow MORB-source mantle does not represent the depleted component within the Iceland plume (Thirlwall, J. Geol. Soc. London 152 (1995) 991-996; Hards et al., J. Geol. Soc. London 152 (1995) 1003-1009; Fitton et al., 1997 doi:10.1016/S0012-821X(97)00170-2). They also indicate that the depleted component is a long-lived and intrinsic feature of the Iceland plume, generated during an ancient melting event in which a mineral (such as garnet) with a high Lu/Hf was a residual phase. Collectively, these data suggest a model for the Iceland plume in which a heterogeneous core, derived from the lower mantle, consists of 'enriched' streaks or blobs dispersed in a more depleted matrix. A distinguishing feature of both the enriched and depleted components is high Nb/Y for a given Zr/Y (i.e. positive DeltaNb), but the enriched component has higher Sr and Pb isotope ratios, combined with lower epsilon-Nd and epsilon-Hf. This heterogeneous core is surrounded by a sheath of depleted material, similar to the depleted component of the Iceland plume in its epsilon-Nd and epsilon-Hf, but with lower 87Sr/86Sr, 208Pb/204Pb and negative DeltaNb; this material was probably entrained from near the 670 km discontinuity when the plume stalled at the boundary between the upper and lower mantle. The plume sheath displaced more normal MORB asthenosphere (distinguished by its lower epsilon-Hf for a given epsilon-Nd or Zr/Nb ratio), which existed in the North Atlantic prior to plume impact. Preliminary data on MORBs from near the Azores plume suggest that much of the North Atlantic may be 'polluted' not only by enriched plume material but also by depleted material similar to the Iceland plume sheath. If this hypothesis is correct, it may provide a general explanation for some of the compositional diversity and variations in inferred depth of melting (Klein and Langmuir, 1987 doi:10.1029/JB092iB08p08089) along the MAR in the North Atlantic.

Dinoflagellates and pollen of the Brito-Arctic Igneous Province flora, ODP Hole 104-642E

Palynological studies of the intrabasaltic sediment layers in the lower volcanic series from ODP Leg 104 outer Voring Plateau Hole 642E Cores 102 through 109 indicated abundant pollen and rarer dinoflagellate cysts. The dinoflagellates belong to the Apectodinium hyperacanthum Zone and indicate an age equivalent to nannoplankton Zones NP9-lower NP10 around the Paleocene/Eocene boundary. The pollen and spore assemblage found here in 12 of the samples from the lower volcanic series is of well- preserved and distinctive specimens and contains unusual forms of pollen from the Taxodiaceae and the Hamamelidae. It has not been transported far from vegetation that was dominated by conifer forest with some ferns and deciduous arborescent angiosperms. Nearly identical assemblages are found elsewhere in the Brito-Arctic Igneous Province, in intrabasaltic sediments from eastern Greenland, the Faeroe Islands, the Isle of Mull, and Antrim (Northern Ireland), and above basalt at the Rockall Plateau. The assemblage is also present in sediments around the Paleocene/Eocene boundary in Spitsbergen. This pollen and spore flora is also associated with dinoflagellate cysts of the Apectodinium hyperacanthum Zone in the deposits from eastern Greenland, the Rockall Plateau, and Spitsbergen, suggesting that these are correlative. Assemblages of the same age from the North Sea, Denmark, and the London and Paris Basins are different. Paleobotanical evidence suggests a short survival of the intrabasaltic flora, and that all the deposits considered here are of about the same age. We propose that at around the Paleocene/Eocene boundary a distinct flora, named here as the Brito-Arctic Igneous Province (BIP) flora, occurred on the line of volcanicity stretching from Rockall to the Greenland Sea, and even to Spitsbergen. Geophysical evidence supports our view that the Rockall to East Greenland intrabasaltics are more or less contemporaneous, at about the Paleocene/Eocene boundary. However, the comparable pollen and spore assemblage in the Hebridean province, at Mull and Antrim, is from pyroclastics that may be a little older.