Next Generation High-Definition Geomagnetic Model for Wellbore Positioning, Incorporating New Crustal Magnetic Data

M. Nair, A. Chulliat, A. Woods, P. Alken, B. Meyer, B. Poedjono, Nicholas Zachman, J. Hernandez
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引用次数: 4

Abstract

Magnetic wellbore positioning depends on an accurate representation of the Earth's magnetic field,where the borehole azimuth is inferred by comparing the magnetic field measured-whiledrilling (MWD) with a geomagnetic reference model. Therefore, model accuracy improvements reduce the position uncertainties. An improved high-resolution model describing the core, crustal and external components of the magnetic field is presented, and it is validated with anindependent set of measurements. Additionally, we benchmark it against other high-resolution geomagnetic models. The crustal part of the improved high-definition model is based on NOAA/NCEI's latest magnetic survey compilation "EMAG2v3" which includes over 50 millionnew observations in several parts of the world, including the Gulf of Mexico and Antarctica, and does not rely on any prior information from sea-floor geology, unlike earlier versions. The core field part of the model covers years 1900 through 2020 andis inferred from polar-orbiting satellite data as well as ground magnetic observatory data. The external field part is modelled to degree and order 1 for years 2000 through 2020. The new model has internal coefficients to spherical harmonic degree and order 790, resolving magnetic anomalies to approximately 51 km wavelength at the equator. In order to quantitatively assess its accuracy, the model was compared with independent shipborne, airborne and ground magnetic measurements. We find that the newmodel has comparable or smaller errors than the other models benchmarkedagainst it over the regions of comparisons. Additionally, we compare theimproved model against magnetic datacollected from MWD; the residual error lies well within the accepted industry error model, which may lead tofuture error model improvements.
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结合新地磁数据的新一代高清晰地磁模型
磁井定位依赖于地球磁场的精确表示,通过比较随钻测量的磁场(MWD)和地磁参考模型来推断井眼方位角。因此,模型精度的提高降低了位置的不确定性。提出了一种改进的高分辨率模型,描述了地核、地壳和磁场的外部分量,并用一组独立的测量结果对其进行了验证。此外,我们将其与其他高分辨率地磁模型进行比较。改进后的高清模型的地壳部分是基于NOAA/NCEI最新的磁调查汇编“EMAG2v3”,其中包括在世界几个地区的5000多万次新观测,包括墨西哥湾和南极洲,不依赖于任何海底地质的先前信息,不像早期的版本。该模型的核心磁场部分涵盖1900年至2020年,是根据极轨卫星数据和地面磁观测数据推断出来的。从2000年到2020年,外场部分按1度和1阶建模。新模型的内系数为球谐度和790阶,可分辨赤道约51 km波长的磁异常。为了定量评估其准确性,将该模型与独立的船载、机载和地面磁测量结果进行了比较。我们发现,在比较区域内,新模型与其他模型相比具有相当或更小的误差。此外,我们将改进的模型与随钻测井采集的磁性数据进行了比较;剩余误差完全在公认的行业误差模型内,这可能导致未来误差模型的改进。
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