Voids size distribution in gelled waxy crude oil under dynamic and static cooling

Q1 Earth and Planetary Sciences
Girma T. Chala , Shaharin A. Sulaiman
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Abstract

Waxy crude oil is known for its high wax contents that can potentially result in gelling following sufficient cooling of the transportation line in the subsea bed at offshore fields. The gelling over the entire lines requires an accurately predicted restart pressure to restart the clogged and idle system. However, the common way of predicting the restart pressure has been reported to result in over-designed and predicted piping parameters. Recent research findings evidenced the formation of voids which would reduce the restart pressure significantly. The study conducted in this paper is aimed at investigating the voids size distribution in gelled crude oil across and along transportation pipelines. Sets of experiments simulating crude oil transportation during both static and dynamic cooling were conducted. The gelled crude oil below the pour point temperature was then scanned using a Magnetic Resonance Imaging (MRI) system to detect the voids formed. The resulting voids at each scanning cross-section were quantified, and their distributions were investigated. It was observed that dynamic cooling had minimal impacts on the voids size difference along the pipeline with the difference in voids areas within 10 mm2 to be twice and uniform for the entire flow rates tested. However, voids size in statically cooled waxy crude oil was found to be highly distributed with a maximum of 6 voids size distribution in 10 mm2 ranges. The low-end temperature had the highest size difference while the difference was decreasing with higher end temperatures. This study shows that the voids amount in dynamically cooled waxy crude oil could also be estimated with lower numbers of cross-sectional voids areas. However, the higher cross-sectional voids detection is recommended while estimating voids in statically cooled waxy crude oil.

动、静态冷却条件下胶凝含蜡原油孔隙尺寸分布
众所周知,含蜡原油的含蜡量很高,在近海油田的海底油层中,当运输管道充分冷却后,可能会出现胶凝现象。整个管线的胶化需要一个准确预测的重启压力,以重启堵塞和闲置的系统。然而,据报道,预测重启压力的常见方法会导致过度设计和预测管道参数。最近的研究结果表明,空隙的形成会大大降低重新启动压力。本文的研究旨在调查胶凝原油在运输管道上和管道沿线的空隙大小分布。实验模拟了原油在静态和动态冷却过程中的运输情况。然后使用磁共振成像(MRI)系统对低于倾点温度的胶凝原油进行扫描,以检测形成的空隙。对每个扫描截面上形成的空隙进行量化,并研究其分布情况。结果表明,动态冷却对管道沿线空隙大小差异的影响极小,在整个测试流速范围内,10 平方毫米以内的空隙面积差异为两倍且均匀。然而,静态冷却的含蜡原油中的空隙大小分布很广,在 10 平方毫米范围内最多有 6 个空隙大小分布。低端温度下的尺寸差异最大,而随着温度的升高,差异逐渐减小。这项研究表明,动态冷却含蜡原油中的空隙量也可以用较少的横截面空隙面积来估算。不过,在估算静态冷却含蜡原油的空隙时,建议采用较高的横截面空隙检测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Petroleum Research
Petroleum Research Earth and Planetary Sciences-Geology
CiteScore
7.10
自引率
0.00%
发文量
90
审稿时长
35 weeks
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