Clathrate Hydrates. Группа авторов

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style="font-size:15px;">      91 91 von Stackelberg, M. and Müller, H.R. (1951). On the structure of gas hydrates. J. Chem. Phys. 19: 1319; (1951). Zur Struktur der Gashydrate. Naturwissenschaften 38 : 456.

      92 92 Claussen, W.F. (1951). A second water structure for inert gas hydrates. J. Chem. Phys. 19: 1425.

      93 93 Müller, H.R. and von Stackelberg, M. (1952). Zur Struktur der Gashydrate. Naturwissenschaften 39: 20.

      94 94 Jeffrey, G.A. (1984). Clathrate hydrates. In: Inclusion Compounds, vol. 1 (ed. J.L. Atwood, D. JED and M.N. DD), 135–190. London: Academic.

      95 95 Van der Waals, J.H. and Platteeuw, J.C. (1958). Clathrate solutions. Adv. Chem. Phys. 2: 1–57.

      96 96 Hammerschmidt, E.G. (1934). Formation of gas hydrates in natural gas transmission lines. Ind. Eng. Chem. 26: 851–855.

      97 97 Deaton, W.M. and Frost, E.M. Jr. (1946). Gas Hydrates and their Relation to the Operation of Natural‐Gas Pipe Lines. United States Bureau of Mines.

      98 98 Sloan, E.D. and Koh, C.A. (2008). Clathrate Hydrates of Natural Gases, 3e. Boca Raton, FL: CRC Press.

      99 99 Katz, D.L., Cornell, D., Vary, J.A. et al. (1959). Handbook of Natural Gas Engineering. New York: McGraw‐Hill.

      100 100 McKoy, V. and Sinanoğlu, O. (1963). Theory of dissociation pressures of some gas hydrates. J. Chem. Phys. 38: 2946–2956.

      101 101 Parrish, W.R. and Prausnitz, J.M. (1972). Dissociation pressures of gas hydrates formed by gas mixtures. Ind. Eng. Chem. Process. Des. Dev. 11: 26–35.

      102 102 Tester, J.W., Bivins, R.L., and Herrick, C.C. (1972). Use of Monte Carlo in calculating the thermodynamic properties of water clathrates. AIChE J. 18: 1220–1230.

      103 103 Tse, J.S. and Davidson, D.W. (1982). Intermolecular potentials in gas hydrates. 4th Canadian Permafrost Conference, pp. 329–334.

      104 104 Tse, J.S., Klein, M.L., and McDonald, I.R. (1983). Molecular dynamics studies of ice Ic and the structure I clathrate hydrate of methane. J. Phys. Chem. 87: 4198–4203.

      105 105 Strizhov, I.N. and Khodanovich, I.E. (1946). Gas Production. Gostoplekhiz dat. Moscow.

      106 106 Makogon, Y.F. (1965). Hydrate formation in gas‐bearing layers under permafrost conditions. Gazov. Promyshlennost (Gas Industry) 5: 14–15.

      107 107 Bily, C. and Dick, J.W.L. (1974). Naturally occurring gas hydrates in the Mackenzie Delta. NWT. Bull. Can. Pet. Geol. 32: 340–352.

      108 108 Stoll, R.D., Ewing, J.I., and Bryan, G.M. (1971). Anomalous wave velocities in sediments containing gas hydrates. J. Geophys. Res. 76: 4539–4555.

      109 109 Miller, S.L. (1969). Clathrate hydrates of air in Antarctic ice. Science 165: 489–490.

      110 110 Miller, S.L. (1961). The occurrence of gas hydrates in the solar system. Proc. Natl. Acad. Sci. U.S.A. 47: 1798–1808.

      111 111 Miller, S.L. (1970). Carbon dioxide clathrate in the Martian ice cap. Science 170: 531–533.

      112 112 Delsemme, A.H. and Swings, P. (1952). Hydrates de gaz dans les noyaux cométaires et les grains interstellaires. Annal. Astrophys. 15: 1–6.

      1 1 Due to the same circumstance, these bodies are well suited for examining the changes that occur in physical properties of the two elements of a compound that forms by the mere fact of their contact. Indeed, the two components retain their identity within the compound; they preserve there a molecular state as close as possible to that which they possess in the state of freedom.

      2 2 When a rapid flow of SO2 is passed through a solution, whereas elevation of the temperature up to 8° or 9° makes all of the (hydrate) crystals disappear, a slight lowering of temperature is sometimes enough to make them reappear. In this way I have seen them form at 3°, 4°, 5°.Messrs. Cailletet and Wroblewski mention a similar fact. According to these scientists, a simple compression is enough to re‐form the hydrates (which they were working with) shortly after they had disappeared. Mr. Cailletet assumed that in this case an infinitely small crystal remained in the tube. In the case of SO2 hydrate, however, it seems to me that this supposition is inadmissible because a hydrate crystal, however small it may be, will have already caused crystallization at 7°.Can one not assume: that shortly after dissociation of the solid hydrate, some aggregates of liquid molecules still have a favorable arrangement for the reformation, but which they lose later?

      3 3 … for each new hydrate, the remaining task, therefore, is to determine numerical values corresponding to equilibrium; but the general laws are no longer unknown.

      4 4 The experiments carried out by de Forcrand were not exhaustive. Today we know that boiling points (or melting points for solids) do not determine the suitability of materials to be hydrate guests. For instance, double hydrates with cyclooctane (b.p. 149 °C), iso‐amyl alcohol (b.p. 131.2 °C), hexachloroethane (m.p. 183–5 °C), and adamantane (m.p. 270 °C) as guests are known.

      5 5 “In some cases I have noticed almost perfect octahedra. Moreover, examination with a polarized light microscope can leave no doubt as to the cubic form of these crystals, which do not act on polarized light.”

      6 6 “… the resulting numbers show that the amount of heat generated is considerable, but it is mainly due to the change of state of the water that is in the compound.”

      7 7 “... the presence of ice causes disturbances which are difficult to take into account, and which have prevented us here from obtaining consistent results.”

      8 8 The dissociable compounds, which are stable only in the solid state, are formed of water with various gases, are all isomorphous to each other, crystallize in the cubic system, and have a constitution expressed by the general formula M + 6H2O where M designates a molecule of the gas under consideration.

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