Kexin Chen , Pengfei Liu , Wenyuan Wang , Linhan Wang , Yan Wang , Hao Liu , Zizhuang Yan , Yu Zhao , Kaichen Song , Yunmin Chen , Bate Bate
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Seven sets of water–oil displacement experiments were conducted on two chips (channel depths of 160 μm and 30 μm) under 0 g, 1 g, and 50 g conditions, with capillary numbers (<em>Ca</em>) ranging from <em>9.55 × 10<sup>-6</sup></em> to <em>9.05 × 10<sup>-5</sup></em> (typical of the viscous fingering regime) and Bond numbers (<em>Bo</em>) ranging from <em>−0.69</em> to <em>0</em>. The results demonstrate that hypergravity (50 g) dragged down the bulk of the dense defending phase, reducing the local pressure gradient at the fluid–fluid interface, and thereby inhibited the upward advancement of the invading phase. In a wide flow channel (576 μm in Chip 1, <em>Bo</em> = -0.69), hypergravity overwhelmed viscous forces, accelerated the dense defending phase downward, even pinched off the invading phase (snap-off), and thus reduced displacement efficiency (<em>S<sub>nw</sub></em>) to 26.9 % (compared to 55.5 % at 1 g); while in a narrow flow channel (80 μm in Chip 2, <em>Bo</em> = -0.0133), the effects of hypergravity and viscous forces were comparable, resulting in enhanced lateral spreading of the invading phase, and thus drastically improved <em>S<sub>nw</sub></em> up to 60.9 % (compared to 29.6 % at 1 g). Meanwhile, hypergravity has a secondary influence on the displacement morphology, as evidenced by the fact that the slope of fluid–fluid interface length (<em>l<sub>nw</sub></em>) to invading phase saturation (<em>S<sub>nw</sub></em>) were constricted to narrow ranges (23.04 ∼ 29.12 for Chip 1, and 50.46 ∼ 64.96 for Chip 2). These findings shed lights on the immiscible fluid–fluid displacement efficiency and morphology under hypergravity, providing insights on applying hypergravity field on meter level models to simulate large-scale and long-duration physical phenomena encountered in deep-earth oil recovery.</div></div>","PeriodicalId":325,"journal":{"name":"Fuel","volume":"391 ","pages":"Article 134776"},"PeriodicalIF":7.5000,"publicationDate":"2025-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Hypergravity experimental study on immiscible fluid–fluid displacement in micromodels\",\"authors\":\"Kexin Chen , Pengfei Liu , Wenyuan Wang , Linhan Wang , Yan Wang , Hao Liu , Zizhuang Yan , Yu Zhao , Kaichen Song , Yunmin Chen , Bate Bate\",\"doi\":\"10.1016/j.fuel.2025.134776\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Hypergravity offers transformative potential for enhanced oil recovery (EOR) and CO<sub>2</sub> sequestration by mimicking subsurface geostress and pressure conditions, facilitating the study of large-scale physical phenomena like fluid migration and sediment compaction within reduced experimental timeframes and scales. In CO<sub>2</sub> sequestration, hypergravity shortens Ostwald ripening, facilitates bubble coalescence, and intensifies gas–solid mass transfer. While the dynamic process of two-phase flow under hypergravity remains insufficiently explored. Hence, a hypergravity microfluidic observation system (HMOS) was developed to investigate the aforementioned process. Seven sets of water–oil displacement experiments were conducted on two chips (channel depths of 160 μm and 30 μm) under 0 g, 1 g, and 50 g conditions, with capillary numbers (<em>Ca</em>) ranging from <em>9.55 × 10<sup>-6</sup></em> to <em>9.05 × 10<sup>-5</sup></em> (typical of the viscous fingering regime) and Bond numbers (<em>Bo</em>) ranging from <em>−0.69</em> to <em>0</em>. The results demonstrate that hypergravity (50 g) dragged down the bulk of the dense defending phase, reducing the local pressure gradient at the fluid–fluid interface, and thereby inhibited the upward advancement of the invading phase. In a wide flow channel (576 μm in Chip 1, <em>Bo</em> = -0.69), hypergravity overwhelmed viscous forces, accelerated the dense defending phase downward, even pinched off the invading phase (snap-off), and thus reduced displacement efficiency (<em>S<sub>nw</sub></em>) to 26.9 % (compared to 55.5 % at 1 g); while in a narrow flow channel (80 μm in Chip 2, <em>Bo</em> = -0.0133), the effects of hypergravity and viscous forces were comparable, resulting in enhanced lateral spreading of the invading phase, and thus drastically improved <em>S<sub>nw</sub></em> up to 60.9 % (compared to 29.6 % at 1 g). Meanwhile, hypergravity has a secondary influence on the displacement morphology, as evidenced by the fact that the slope of fluid–fluid interface length (<em>l<sub>nw</sub></em>) to invading phase saturation (<em>S<sub>nw</sub></em>) were constricted to narrow ranges (23.04 ∼ 29.12 for Chip 1, and 50.46 ∼ 64.96 for Chip 2). 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引用次数: 0
摘要
通过模拟地下地应力和压力条件,超重力为提高采收率(EOR)和二氧化碳封存提供了革命性的潜力,有助于在更短的实验时间和尺度内研究流体迁移和沉积物压实等大规模物理现象。在CO2固存中,超重力缩短了奥斯特瓦尔德成熟,促进了气泡的聚并,加强了气固传质。而两相流在超重力作用下的动力学过程尚未得到充分的研究。为此,研制了超重力微流控观测系统(HMOS)来研究上述过程。在0 g、1 g和50 g条件下,对两种芯片(通道深度分别为160 μm和30 μm)进行了7组水-油驱替实验,毛细管数(Ca)范围为9.55 × 10-6 ~ 9.05 × 10-5(典型的粘性指法),键数(Bo)范围为−0.69 ~ 0。结果表明:超重力(50 g)作用下,致密防御相的大部分被拉下,降低了流体-流体界面处的局部压力梯度,从而抑制了入侵相的向上推进。在宽流道(576 μm In Chip 1, Bo = -0.69)中,超重力压过了粘性力,加速了致密防御相向下,甚至挤压了入侵相(snap-off),从而将驱替效率(Snw)降低到26.9% (1 g时为55.5%);而在窄流道(80 μm in Chip 2, Bo = -0.0133)中,超重力和粘性力的影响相当,导致入侵相的横向扩展增强,从而使雪度大幅提高60.9% (1 g时为29.6%)。同时,超重力对位移形态的影响是次要的。流体-流体界面长度(lnw)与侵入相饱和度(Snw)的斜率在较窄的范围内(Chip 1为23.04 ~ 29.12,Chip 2为50.46 ~ 64.96)。这些发现揭示了超重力条件下的非混相流体-流体驱替效率和形态,为应用超重力场在米级模型上模拟深地采油过程中遇到的大规模、长时间物理现象提供了见解。
Hypergravity experimental study on immiscible fluid–fluid displacement in micromodels
Hypergravity offers transformative potential for enhanced oil recovery (EOR) and CO2 sequestration by mimicking subsurface geostress and pressure conditions, facilitating the study of large-scale physical phenomena like fluid migration and sediment compaction within reduced experimental timeframes and scales. In CO2 sequestration, hypergravity shortens Ostwald ripening, facilitates bubble coalescence, and intensifies gas–solid mass transfer. While the dynamic process of two-phase flow under hypergravity remains insufficiently explored. Hence, a hypergravity microfluidic observation system (HMOS) was developed to investigate the aforementioned process. Seven sets of water–oil displacement experiments were conducted on two chips (channel depths of 160 μm and 30 μm) under 0 g, 1 g, and 50 g conditions, with capillary numbers (Ca) ranging from 9.55 × 10-6 to 9.05 × 10-5 (typical of the viscous fingering regime) and Bond numbers (Bo) ranging from −0.69 to 0. The results demonstrate that hypergravity (50 g) dragged down the bulk of the dense defending phase, reducing the local pressure gradient at the fluid–fluid interface, and thereby inhibited the upward advancement of the invading phase. In a wide flow channel (576 μm in Chip 1, Bo = -0.69), hypergravity overwhelmed viscous forces, accelerated the dense defending phase downward, even pinched off the invading phase (snap-off), and thus reduced displacement efficiency (Snw) to 26.9 % (compared to 55.5 % at 1 g); while in a narrow flow channel (80 μm in Chip 2, Bo = -0.0133), the effects of hypergravity and viscous forces were comparable, resulting in enhanced lateral spreading of the invading phase, and thus drastically improved Snw up to 60.9 % (compared to 29.6 % at 1 g). Meanwhile, hypergravity has a secondary influence on the displacement morphology, as evidenced by the fact that the slope of fluid–fluid interface length (lnw) to invading phase saturation (Snw) were constricted to narrow ranges (23.04 ∼ 29.12 for Chip 1, and 50.46 ∼ 64.96 for Chip 2). These findings shed lights on the immiscible fluid–fluid displacement efficiency and morphology under hypergravity, providing insights on applying hypergravity field on meter level models to simulate large-scale and long-duration physical phenomena encountered in deep-earth oil recovery.
期刊介绍:
The exploration of energy sources remains a critical matter of study. For the past nine decades, fuel has consistently held the forefront in primary research efforts within the field of energy science. This area of investigation encompasses a wide range of subjects, with a particular emphasis on emerging concerns like environmental factors and pollution.