Abstract:qi,qz,qi,qz = General quantities given by Equation (S), SM' = S M / d R = r = rt = a = rm = s = T = T = Ti = Tz = N T~ = -NTa* = .. v * A Part I ratio of cylinder speeds radius or coordinate radius of inner cylinder radius of outer cylinder mean radius shape function given by Equation (23), Part I temperature average temperature in annulus temperature of inner cylinder temperature of outer cylinder Taylor number Tavlor number ( \ i N~a " __-N T~~ = t = tl= u = u 1 = us = o = 0 1 = o = -. w = w1 = z = z = , . N… Show more
“…(2) shows the pressure temperature relations of Ar hydrate system accompanied with the literature values [3,18]. In the low-pressure region (up to 200 MPa), our data are in good agreement with Marshall's ones [18]. Moreover, except less than 20 MPa, the present data are in almost agreement with Dyadin's ones [3].…”
Section: Resultssupporting
confidence: 87%
“…The region A corresponds to the pressure range up to 281 MPa. The pressure range from 281 to 456 MPa is region B, and over 456 MPa defined as region C. Especially, in the region B, the present data show the large discrepancies with the literature [3,18]. The Raman spectrum of intermolecular O-O stretching vibration mode of water molecules was detected around 210 cm -1 in the structure-II gas hydrate systems; we have already reported about N 2 and SF 6 hydrate systems [19,20].…”
Section: Resultscontrasting
confidence: 78%
“…(2). Pressure -temperature relations of Ar hydrate stability boundaries: , three-phase coexisting curve of Ar hydrate (present study); , Marshall, Saito, and Kobayashi [18]; , Dyadin, Larionov, Mirinski, Mikina, and Starostina [3]. From our experimental data (up to 485 MPa), Ar hydrate has two structural transition points located at 281 MPa and 456 MPa.…”
Abstract:The three-phase coexisting curve of Ar hydrate + water + gas has been investigated in a pressure range up to 485 MPa and a temperature range of (279.57 to 305.32) K. The Raman spectrum of intermolecular O-O stretching vibration mode has been measured for Ar hydrate crystal along the stability boundary curve. Both the discontinuity of slope of the three-phase coexisting curve and the pressure dependence of the Raman shift reveal that two structural phase transition points exist at (281±1) MPa and (302.7±0.1) K, (456±1) MPa and (304.6±0.1) K in a pressure range up to 485 MPa for the Ar hydrate system.
“…(2) shows the pressure temperature relations of Ar hydrate system accompanied with the literature values [3,18]. In the low-pressure region (up to 200 MPa), our data are in good agreement with Marshall's ones [18]. Moreover, except less than 20 MPa, the present data are in almost agreement with Dyadin's ones [3].…”
Section: Resultssupporting
confidence: 87%
“…The region A corresponds to the pressure range up to 281 MPa. The pressure range from 281 to 456 MPa is region B, and over 456 MPa defined as region C. Especially, in the region B, the present data show the large discrepancies with the literature [3,18]. The Raman spectrum of intermolecular O-O stretching vibration mode of water molecules was detected around 210 cm -1 in the structure-II gas hydrate systems; we have already reported about N 2 and SF 6 hydrate systems [19,20].…”
Section: Resultscontrasting
confidence: 78%
“…(2). Pressure -temperature relations of Ar hydrate stability boundaries: , three-phase coexisting curve of Ar hydrate (present study); , Marshall, Saito, and Kobayashi [18]; , Dyadin, Larionov, Mirinski, Mikina, and Starostina [3]. From our experimental data (up to 485 MPa), Ar hydrate has two structural transition points located at 281 MPa and 456 MPa.…”
Abstract:The three-phase coexisting curve of Ar hydrate + water + gas has been investigated in a pressure range up to 485 MPa and a temperature range of (279.57 to 305.32) K. The Raman spectrum of intermolecular O-O stretching vibration mode has been measured for Ar hydrate crystal along the stability boundary curve. Both the discontinuity of slope of the three-phase coexisting curve and the pressure dependence of the Raman shift reveal that two structural phase transition points exist at (281±1) MPa and (302.7±0.1) K, (456±1) MPa and (304.6±0.1) K in a pressure range up to 485 MPa for the Ar hydrate system.
“…A CO 2 -methane-water hydrate is stable at higher temperatures or lower pressures than a pure methane-water hydrate and thus could not account for an upward translation of the hydrate stability field. Likewise, at constant temperature, a natural gas-water hydrate is stable at much shallower depths than a methane-water hydrate (Marshall et al, 1964). For example, a 10% addition of ethane to a pure methane hydrate at 15°C would shift the phase boundary from 140 bar to 75 bar (Katz et al, 1959).…”
The drilling during Ocean Drilling Program Leg 146 at the accretionary margin complexes off Vancouver Island, Canada (VIM), and Oregon, U.S.A (COM), addressed specific geochemical relationships and phenomena associated with fluid, gas, and heat fluxes generated by the compressive forces. Of particular importance were the occurrence of hydrates and formation of thermogenic hydrocarbons. In most cases, the geochemistry of the hemipelagic sediments is dominated by steady-and nonsteady-state diagenetic reactions, including sulfate reduction (Sites 888 and 891), and methanogenesis and methanotrophy (Sites 888-892). However, these shallow (<600 mbsf) sediments are also clearly and extensively influenced by pervasive and active fracture COM migration of deeper seated thermogenic hydrocarbons at the VIM and COM, respectively. The origin of bacterial and thermogenic gases is confirmed by their molecular and stable carbon isotope signatures. In many cases, the occurrence of C 2 + hydrocarbons delineates the fault zones.Only disseminated macrocrystalline hydrate, not massive hydrate, was encountered during Leg 146. Based on the carbon isotope signature, the hydrate is of bacterial origin and identical to that of the surrounding sediment free gas. Thermogenic gas hydrates were not encountered. The discrepancy between the location of the bottom-simulating reflector (BSR) and the base of hydrate stability may be caused by the presence of other gases or fluid constituents in the hydrate lattice. The amount of free gas inferred by the vertical seismic profiler (VSP) below the BSR may be due to the incomplete upward cryo-distillation of gases. This vertical shift could be created by (1) the change in bottom-water temperatures between glacial and interglacial, and (2) a pressure drop caused by sea-level change and accretionary uplift. The presence of hydrogen sulfide in the methane hydrates at Site 892 was unexpected and results from the rapid incorporation of H 2 S into hydrates, protecting them from reaction, (e.g., formation of iron monosulfides.)
“…Sarupria compared the MD simulations result with experimental data, and found that the difference in the melting points (T m (hydrate)-T m (ice)) that was obtained from MD simulations is in good agreement with the experimental value. Under the experimental conditions, the hydrate melting point at 30 MPa is 295 K [61], 22 K higher than the melting point of Ice Ih. The melting point of SPC model is 190 K at 30 MPa, the corresponding hydrate melting point is about 212 K. In our simulation work, the temperature range of 243 K-263 K is higher than the melting point of both Ice Ih and hydrate at 30 MPa.…”
Almost 98% of methane hydrate is stored in the seawater environment, the study of microscopic mechanism for methane hydrate dissociation on the sea floor is of great significance to the development of hydrate production, involving a three-phase coexistence system of seawater (3.5% NaCl) + hydrate + methane gas. The molecular dynamics method is used to simulate the hydrate dissociation process. The dissociation of hydrate system depends on diffusion of methane molecules from partially open cages and a layer by layer breakdown of the closed cages. The presence of liquid or gas phases adjacent to the hydrate has an effect on the rate of hydrate dissociation. At the beginning of dissociation process, hydrate layers that are in contact with liquid phase dissociated faster than layers adjacent to the gas phase. As the dissociation continues, the thickness of water film near the hydrate-liquid interface became larger than the hydrate-gas interface giving more resistance to the hydrate dissociation. Dissociation rate of hydrate layers adjacent to gas phase gradually exceeds the dissociation rate of layers adjacent to the liquid phase. The difficulty of methane diffusion in the hydrate-liquid side also brings about change in dissociation rate.
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