Challenges and Solutions for Accurate Wellbore Placement in the Barents Sea

Alexander M. Mitkus, S. Maus, Marc E. Willerth, Andrew Reetz, R. Oskarsen, Morten H. Emilsen, Amir Gergerechi
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引用次数: 2

Abstract

As development of the Barents Sea continues with new plays such as the Castberg, accurate specification of the local magnetic field is important to reliably infer the orientation of the bottomhole assembly (BHA) in horizontal drilling. Since magnetic fields at high latitudes vary spatially and temporally, one requires both spatial models and a way to capture temporal changes. Large temporal changes in the magnetic field can severly distort measured azimuths and therefore must be corrected for. This study, based on a report written for Petroleumstilsynet (Maus et al., 2017), shows that in regions of the Barents Sea within 50 km of a magnetic observatory, either the nearest observatory, interpolated infield referencing (IIFR), or the disturbance function (DF) method may be used for corrections in wellbore surveying to meet accuracy requirements. IIFR and DF will give better error reduction but are slightly more complicated to implement. At distances between 50 km and 250 km, the disturbance field (DF) method best meets accuracy requirements. In remote regions beyond 250 km, a local observatory must be deployed to meet the highest accuracy specifications, but the DF will still far outperform the other interpolated methods at such large distances from an existing observatory. Despite having focused on the Barents Sea region, this comparison of the accuracy of different spatial and temporal magnetic field mitigation methods for wellbore surveying is applicable to high latitude northern and southern regions across the globe.
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巴伦支海精确井筒定位的挑战与解决方案
随着巴伦支海(Barents Sea)新区块的不断开发,例如Castberg,在水平钻井中,精确的局部磁场规格对于可靠地推断底部钻具组合(BHA)的方向非常重要。由于高纬度地区的磁场在空间和时间上都有变化,因此既需要空间模型,也需要一种捕捉时间变化的方法。磁场的大时间变化会严重扭曲测量的方位角,因此必须加以校正。该研究基于为Petroleumstilsynet编写的一份报告(Maus等人,2017),表明在巴伦支海地区,在距磁观测站50公里范围内,可以使用最近的观测站,内插值参考(IIFR)或干扰函数(DF)方法进行井筒测量校正,以满足精度要求。IIFR和DF可以更好地减少错误,但实现起来稍微复杂一些。在50 ~ 250 km的距离上,扰动场(DF)法最能满足精度要求。在超过250公里的偏远地区,必须部署一个当地的天文台来满足最高的精度要求,但是在距离现有天文台如此远的距离上,DF仍然远远优于其他插值方法。尽管研究的重点是巴伦支海地区,但这种对不同时空磁场减缓方法的井眼测量精度的比较适用于全球北部和南部高纬度地区。
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