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Mapping the depth to magnetic basement using inversion of pseudogravity: Application to the Bishop model and the Stord Basin, northern North Sea

机译:使用伪重力反演将深度映射到磁性基底:在Bishop模型和北海北部Stord盆地中的应用

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Magnetic depth estimation methods are routinely used to map the depth of sedimentary basins by assuming that the sediments are nonmagnetic and underlain by magnetic basement rocks. Most of these methods generate basement depth estimates at discrete points. Converting these depth estimates into a grid or map form often requires the application of qualitative methods. The reason for this is twofold: first, in deeper parts of basins, there is generally a scarcity of depth estimates and those that have been determined tend to be biased toward the shallower basement structures close to the basin edge; and second, depth estimates intrinsically relate to magnetic anomalies that emanate from the top edges of basement faults/contacts resulting in a shallow depth bias. Thus, simple grid interpolation of these depth estimates often forms a shallower and structurally unrepresentative map when evaluated in detail. To overcome these problems of qualitative and/or simple grid interpolation of these point-depth estimates into a regular grid, we use the pseudogravity field transform response of the magnetic field to constrain this interpolation using inversion methods together with the relationship between the point-depth estimates and their pseudogravity values. The pseudogravity transformation converts a grid of magnetic data such that the resulting grid has the same simple relationship to magnetic susceptibility that a gravity grid has to density. The pseudogravity map is thus straightforward to visualize in terms of basement structure, but it only maps the magnetic properties of the subsurface and is not related to the gravity anomaly or the density. We describe a practical approach to invert pseudogravity grids using gravity inversion software to produce a 3D basin model assuming a constant susceptibility basement. The approach is initially tested on the Bishop 3D model and then applied to an example from the northern North Sea. This approach can be considered complementary to 3D gravity inversion and has the advantage that the pseudogravity response is not affected by structure within the sediments or effects such as sediment compaction, inversion, or isostatic compensation, all of which often complicate the gravity response of sedimentary basins.
机译:通常采用磁性深度估算方法来绘制沉积盆地的深度图,方法是假设沉积物是非磁性的,并被磁性基底岩层覆盖。这些方法大多数都在离散点生成地下室深度估计。将这些深度估计值转换为网格或地图形式通常需要应用定性方法。原因是双重的:首先,在盆地的较深部分,通常缺乏深度估算,已经确定的深度估算往往偏向靠近盆地边缘的较浅的基底结构。第二,深度估算从本质上与地下室断层/接触的顶部边缘产生的磁异常有关,从而导致浅的深度偏差。因此,在进行详细评估时,这些深度估算值的简单网格插值通常会形成较浅且在结构上不具代表性的地图。为了克服将这些点深度估计值定性和/或简单网格插值到规则网格中的问题,我们使用磁场的伪重力场变换响应,使用反演方法以及点深度之间的关系来约束该插值估计及其伪重力值。伪重力变换转换磁数据的网格,以使所得的网格与磁化率具有与重力网格必须具有的密度相同的简单关系。因此,伪重力图可以根据地下室结构直接直观地看到,但是它仅映射地下的磁性,与重力异常或密度无关。我们描述了一种使用重力反演软件来对伪重力网格进行反演的实用方法,以假定恒定的磁化率基础来生成3D盆地模型。该方法最初在Bishop 3D模型上进行了测试,然后应用于北海北部的示例。这种方法可以被认为是3D重力反演的补充,其优点是假重力响应不受沉积物内部结构或沉积物压实,反演或等静压补偿等影响,所有这些因素通常会使沉积盆地的重力响应复杂化。

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