岩石磁化过程中磁化率的各向异性(AF、IRM)和磁性载体的畴态信息

IF 2.4 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Physics of the Earth and Planetary Interiors Pub Date : 2023-09-01 DOI:10.1016/j.pepi.2023.107076
Pierrick Roperch , Catherine Kissel , France Lagroix , Guillaume Dupont-Nivet , Annick Chauvin , Fernando Poblete , Jovid Aminov
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引用次数: 1

摘要

我们提出并解释了各种岩石磁化率(AMS)结构的各向异性,重点研究了交变磁场(AF)退磁和等温剩余磁化(IRM)的影响。我们的研究结果表明,具有大多畴磁铁矿颗粒的侵入岩样品中的AMS受IRM或静态AF退磁的影响最小。在具有钛磁铁矿伪单畴(PSD)载体的近各向同性火山岩中,静态AF退磁引起的AMS织物很容易识别,最显著的影响是在AF退磁方向上形成明确的AMS线理(高达1.04)。相反,在具有较小磁性粒度的钛磁铁矿的快速冷却火山岩样品中,观察到与施加AF场方向正交的AMS片理(~ 1.02),而不是线理。在这样的样品中,IRM产生更大的AMS叶理,与IRM正交达1.3。在绿片岩相中,具有钛赤铁矿或磁黄铁矿磁性载体的变质岩中,irm印记的AMS也特别强。具有最大irm印迹织物的样品具有非常高的Mrs/Ms比(> ~ 0.4)。Mrs/Ms比值大于0.5可能表明SD磁性颗粒的贡献具有多轴各向异性。由于明显的多轴各向异性在具有微米级钛磁铁矿枝晶的火山岩中尤其明显,因此磁颗粒的复杂形状及其化学成分可能在irm -印象AMS中起关键作用。静态AF退磁后,不应测量火山岩中的AMS结构。翻滚AF退磁不会显著改变初始磁性结构,可以安全地用于与闪电相关的强磁化岩石,可能记录IRM印象的AMS。
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Anisotropy of magnetic susceptibility impressed during rock magnetic procedures (AF, IRM) and information on the domain state of the magnetic carriers

We present and interpret anisotropy of magnetic susceptibility (AMS) fabrics in various rocks, focusing on the effects of Alternating Field (AF) demagnetization and Isothermal Remanent Magnetization (IRM). Our findings reveal that AMS in samples from intrusive rocks with large multidomain magnetite grains is minimally affected by IRM or static AF demagnetization. In nearly isotropic volcanic rocks with titanomagnetite pseudo single domain (PSD) carriers, AMS fabrics caused by static AF demagnetization are easily identifiable, with the most prominent effect being a well-defined AMS lineation (up to 1.04) in the direction of the applied AF demagnetization. Conversely, in samples from rapidly cooled volcanic rocks with titanomagnetite of smaller magnetic grain size, an AMS foliation (∼1.02) is observed orthogonal to the direction of the applied AF field, instead of a lineation. In such samples, an IRM produces a much larger AMS foliation up to 1.3 orthogonal to the IRM. The IRM-impressed AMS is also particularly strong in metamorphic rocks in the greenschist facies with either titano-hematite or pyrrhotite magnetic carriers. Samples with the largest IRM-impressed fabric have very high Mrs/Ms ratio (>∼0.4). Mrs/Ms ratios above 0.5 may indicate the contribution of SD magnetic grains with multiaxial anisotropy. As the apparent multiaxial anisotropy is especially observed in volcanic rocks with micron size dendrites of titanomagnetites, the complex shape of the magnetic particles and their chemical composition likely play a key role in IRM-impressed AMS. AMS fabric in volcanic rocks should not be measured after static AF demagnetization. Tumbling AF demagnetization does not alter significantly the initial magnetic fabric and could be safely used in rocks with strong magnetization related to lightning possibly recording an IRM impressed AMS.

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来源期刊
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors 地学天文-地球化学与地球物理
CiteScore
5.00
自引率
4.30%
发文量
78
审稿时长
18.5 weeks
期刊介绍: Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.
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