Abstract
Here attention is focused on one of the fundamental problems in astrophysics—the formation of protoplanetary accretion disks around late-type stars whose special case is the origin of the Solar system. Particular attention is given to the development of a semiempirical approach to modeling heterogeneous turbulence in the accretion disk that surrounded the proto-Sun at the early stage of its existence with the goal of reducing the number of assumptions in the models used. We formulate a complete system of equations of two-phase multicomponent mechanics by taking into account the relative motion of the phases, coagulation processes, phase transitions, chemical reactions, and radiation. Basically, it is designed for schematized formulations and numerical solution of specific model problems on mutually consistent modeling of the structure, dynamics, thermal regime, and chemical composition of the circumsolar disk at various stages of its evolution. The processes in the disk medium in the presence of the developed turbulent motions of a coagulating gas suspension are addressed that eventually contribute to the formation of a dust subdisk near the equatorial plane of the proto-Sun within the model under consideration and the emergence of hydrodynamic and then gravitational instability in it followed by the formation of dust clusters.
For an adequate phenomenological description of turbulent flows in a gas–dust disk, we perform the probability-theoretic Favre averaging of the stochastic equations of heterogeneous mechanics and derive the defining gradient relations for the turbulent interphase diffusion and heat fluxes as well as for the “relative” and Reynolds stress tensors needed to close the hydrodynamic equations of mean motion. We investigate the influence of the inertial effects of dust particles on the characteristics of turbulence in the disk, in particular, on the additional generation of turbulent energy by large particles. We propose a semiempirical method of modeling the turbulent viscosity coefficient in a two-phase disk by taking into account the inverse effects of dispersed phase and heat transport on the development of turbulence with the goal of modeling the vertically inhomogeneous thermohydrodynamic structure of the dust subdisk and the ambient gas.
For a steady motion when solid particles settle down to the central plane of the disk under gravity, we investigate a parametric method of moments for solving the Smoluchowski integro-differential coagulation equation for the particle size distribution function that is based on the a priori belonging of the sought-for distribution function to a certain parametric class of distributions. In addition, we analyze the possible regime of limiting saturation of the subdisk atmosphere by fine dust particles that is responsible for the intensification of various coagulation mechanisms in a turbulized medium. The results of this chapter open new possibilities for constructing improved (and more realistic) models of stellar-planetary cosmogony, thereby providing a new approach to solving the fundamental problem of the origin and evolution of the Solar system and planetary systems around other stars.
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References
Cuzzi, J.N., Weidenschilling, S.J.: In: Lauretta, D., Leshin, L.A., McSween, H. (eds.) Particle-Gas Dynamics and Primary Accretion in Meteorites and the Early Solar System II, p. 353. University of Arizona, Tuscon (2006)
Russell, S.S., Hartmann, L.A., Cuzzi, J.N., et al.: Timescales of the solar protoplanetary disk. In: Lauretta, D., Leshin, L.A., McSween, H. (eds.) Meteorites and the Early Solar System II, p. 233. University of Arizona, Tucson (2006a)
Schneider, G., Smith, B.A., Becklin, E.E., et al.: NICMOS imaging of the HR 4796A circumstellar disk. Astrophys. J. 513, L127 (1999)
Abramovich, G.N., Girshovich, T.A.: On the diffusion of heavy particles in turbulent gas flows. Dokl. Akad. Nauk USSR 212, 573 (1973)
Alfven, H., Arrhenius, G.: Evolution of the Solar System. Sci. & Techn. Inf. Office, NASA, Washington, D.C. (1976)
Armitage, P.J., Livio, M., Pringle, J.E.: Episodic accretion in magnetically layered protoplanetary disks. Mon. Not. R. Astron. Soc. 324, 705 (2001b)
Balbus, S.A., Hawley, J.F.: Instability, turbulence, and enhanced transport in accretion disks. Rev. Mod. Phys. 70, 1 (1998b)
Barenblatt, G.I., Golitsyn, G.S.: Local Structure of Developed Dust Storms. Moscow State University, Moscow (in Russian) (1973)
Barenblatt, G.I., Golitsyn, G.S.: Local structure of mature dust storms. J. Atmos. Sci. 31, 1917 (1974)
Barge, P., Sommeria, J.: Did planet formation begin inside persistent gaseous vortices? Astron. Astrophys 295, L1 (1995a)
Beckwith, S.V.W., Henning, T., Nakagawa Y. In: Mannings, V., Boss, A.P., Rassell, S.S. (eds.) Dust Properties and Assembly of Large Particles in Protoplanetary Disks in Protostars and Planets IV, Tucson Univ. Ariz. Press, 533 (2000)
Bisnovaty-Kogan, G.S., Lovelace, R.V.E.: Advective accretion disks and related problems including magnetic fields. New Astron. Rev 45, 663 (2001b)
Bryden, G., Chen, X., Lin, D., et al.: Tidally induced gap formation in protostellar disks: Gap clearing and suppression of protoplanetary growth. Astrophys. J. 514, 344 (1999b)
Busroyd, R.: Flow of Gas with Suspended Particles, Mir, Moscow (in Russian) (1975)
Cabot, W., Canuto, V.M., Hubickyj, O., Pollack, J.B.: The role of turbulent convection in the primitive solar nebula. Icarus 69, 423 (1987)
Cameron, A.G.W.: Accumulation processes in the primitive solar nebula. Icarus 18, 407–450 (1973)
Cameron, A.G.W.: Formation and evolution of the primitive solar nebula. In: Black, D.C., Matthews, M.S. (eds.) Protostars and Planets II, pp. 1073–1099. Univ. of Arizona Press, Tucson, AZ (1985)
Cameron, A.G.W.: The primitive solar accretion disc and formation of planets. In: Dermott, S.F. (ed.) The Origin of the Solar System. pp. 49–75. NY (1978)
Сhavanis, P.-H.: Trapping of Dust by Coherent Vortices in the Solar Nebula,//arXiv:astro-ph/9912087, 16, 1. (1999)
Cuzzi, J.N.: Blowing in the Wind: III. Accretion of dust rims by chondrule-sized particles in a turbulent protoplanetary nebula. Icarus 168, 484 (2004b)
Cuzzi, J.N., Dobrovolskis, A.R., Champney, J.M.: Particle-gas dynamics in the midplane of a protoplanetary nebula. Icarus 106, 102 (1993)
Cuzzi, J.N., Davis, S.S., Dobrovolskis, A.R.: Blowing in the Wind. II. Creation and Redistribution of Refractory Inclusions in a Turbulent Protoplanetary Nebula. Icarus 166, 385 (2003b)
Danon, H., Wolfshtein, M., Hetsroni, G.: Numerical calculation of two—phase turbulent round jet. Int. Multiphase Flow 3, 223 (1977)
Derevich, I.V.: Influence of an admixture of large particles on turbulent characteristics of a gas suspension in channels. PMTF 2, 70 (1994)
Dominik, C., Blum, J., Cuzzi, J., Wurm, G.: Growth of dust as the initial step toward planet formation in protostars and planets V. Arizona, AZ (2007b)
Dorofeeva, V.A., Makalkin, A.B..: Evolution of the Early Solar System. Cosmochemical and Physical Aspects. Editorial URSS, Moscow (in Russian) (2004b)
Dubrulle, B.: A turbulent closure model for thin accretion disks. Astron. Astrophys. 266, 592 (1992)
Dubrulle, B.: Differential rotation as a source of angular momentum transfer in the solar nebula. Icarus 106, 59 (1993b)
Dubrulle, B., Morfill, G., Sterzic, M.: The dust subdisk in the protoplanetary nebula. Icarus 114, 237 (1995)
Dullemond, C.P., Dominik, C.: Dust coagulation in protoplanetary disks: A rapid depletion of small grains. Astron. Astrophys. 434, 971 (2005b)
Eardley, D.M., Lightman, A.P., Payne, D.G., Shapiro, S.L.: Accretion disks around massive black holes: Persistent emission spectra. Astrophys. J. 234, 53 (1978b)
Elghobashi, S.E., Abou-Arab, T.W.: A second-order turbulence model for two-phase flows. Heat Transfer 5, 219 (1982)
Elghobashi, S.E., Abou-Arab, T.W.: A two-equation turbulence model for two-phase flows. Phys. Fluids 26, 931 (1983)
Epstein, P.S.: On the resistance experienced by spheres in their motion through gases. Phys. Rev. 23, 710 (1924)
Favre, A.: Statistical equations of turbulent gases in problems of hydrodynamics and continuum mechanics. SIAM, Philadelphia (1969b). 231
Fridman, F.M.: To the dynamics of a viscous differentially rotating gravitating medium. Pis’ma Astron. Zh. 15, 1122 (1989b)
Fridman, A.M., Boyarchuck, F.F., Bisikalo, D.V., et al.: The collective mode and turbulent viscosity in accretion disks. Phys. Lett. A 317, 181 (2003b)
Fuks, N.A.: Mechanics of Aerosols. Akad. Nauk USSR, Moscow (in Russian) (1955)
Garaud, P., Barriere-Fouchet, L., Lin, D.N.C.: Individual and collective behavior of dust particles in a protoplanetary nebula. Astroph. J. 603, 292 (2005)
Gavin, L.B., Naumov, V.A., Shor, V.V.: Numerical analysis of a gas jet with heavy particles based on a two-parameter turbulence model. PMTF 1, 62 (1984)
Goldrich, P., Ward, W.R.: The formation of planetesimals. Astrophys. J. 183, 1051 (1973b)
Goodmann, J., Pindor, B.: Secular instability and planetesimal formation in the dust layer. Icarus 148, 537 (2000)
Gor’kavyi, N.N., Fridman, A.M.: Physics of Planetary Rings. Nauka, Moscow (in Russian) (1994b)
Gorbis, Z.R.: Heat Exchange and Hydromechanics of Disperse Through Flows. Energiya, Moscow (in Russian) (1970)
Gore, R.A., Crowe, C.T.: Effect of particle size on modulating turbulent intensity. Int. J. Multiphase Flow 15, 279 (1989)
Grad, H.: On the kinetic theory of rarefied gases. Commun. Pure Appl. Math. 2, 331 (1949)
Hayashi, C., Nakazawa, K., Nakagawa, Y.: In: Black, D.C., Matthews, M.S. (eds.) Formation of the Solar System In Protostars and Planets II, University of Arizona, Tucson, 1100. (1985)
Hazlehurst, J., Sargent, W.L.W.: Astrophys J. 130, 276 (1959)
Hersant, F., Dudrulle, B., Hure, J.-M.: Turbulence in Circumstellar Disks, Astron. Astrophys. (2004) Manuscript No. 3549, 1
Hirschfelder, D., Curtiss, C., Bird, R.: Molecular Theory of Gases and Liquids. John Wiley and Sons, New York and London (1954b)
Hunter, S.C., Cherry, S.S., Kliegel, J.R., Waldman, C.H.: Gas-particle nozzle flow with reaction and particle size change. AIAA Paper 37, 14 (1981)
Ievlev, V.M.: Approximate equations of turbulent motion for an incompressible fluid. Izv. Akad. Nauk USSR Ser MZhG 1, 91 (1970)
Ievlev, V.M.: Turbulent Motion of High-Temperature Continuous Media. Nauka, Moscow (in Russian) (1975c)
Kartushinskii, A.I.: Transport of an inertial admixture in a two-phase turbulent jet. Izv. Akad. Nauk USSR Ser MZhG 1, 36 (1984)
Kolesnichenko, A.V.: To the theory of turbulence in planetary atmospheres: numerical simulation of structural parameters. Astron. Vestn. 29, 133 (1995a)
Kolesnichenko, A.V.: Stefan-Maxwell Relations and Heat Flow for Turbulent Multicomponent Continuous Media in Problems of Modern Mechanics. Moscow State University, Moscow (in Russian) (1998b). 52
Kolesnichenko, A.V.: Modeling turbulent transport coefficients in a gas-dust accretion disk. Astron. Vestn. 34, 516 (2000a)
Kolesnichenko, A.V.: Hydrodynamics aspects of modeling mass transfer and coagulation in a turbulent accretion disk. Astron. Vestn. 35, 139 (2001a)
Kolesnichenko, A.V.: Synergetic Approach to Describing Stationary-Nonequilibrium Turbulence of Astrophysical Systems in Modern Problems of Mechanics and Space Physics. Fizmatlit, Moscow (in Russian) (2003a). 123
Kolesnichenko, A.V.: On the synergetic formation mechanism of coherent structures in the continuum theory of developed turbulence. Astron. Vestn. 38, 405 (2004c)
Kolesnichenko, A.V., Maksimov, V.M.: Generalized darcy filtering law as a corollary of the Stefan-Maxwell relations for a heterogeneous medium. Mat. Mod. 13, 3 (2001)
Kolesnichenko, A.V., Marov, M.Y.: Turbulence of Multicomponent Media. MAIK-Nauka, Moscow (in Russian) (1999g)
Kolesnichenko, A.V., Marov, M.Y.: Fundamentals of mechanics of heterogenic media with application to circumsolar protoplanetary cloud: Influence of solid paticles on the disc turbulence. Solar System Res. 40(1), 2–62 (2006b)
Kolmogorov, A.N.: Equations of turbulent motion for an incompressible fluid. Izv. Akad. Nauk. USSR Ser. fiz. 6, 56 (1942c)
Kolmogorov, A.N.: On a new version of the gravitational theory of motion of suspended sediments, vestn. MGU 3, 41 (1954b)
Kusaka, T., Nakano, N., Hayashi, C.: Growth of Solid Particles in the Primordial Solar Nebula. Progr. Theor. Phys 44, 1580 (1970)
Laikhtman, G.L.: Physics of the Atmospheric Boundary Layer. Gidrometeoizdat, Leningrad (in Russian) (1970b)
Landau, L.D., Lifshitz, V.M.: Hydrodynamics. Nauka, Moscow (in Russian) (1988d)
Lee, K.W.: Change of particle size distribution during brownian coagulation. J. Colloid Interface Sci. 92, 38 (1983)
Leonard, A.: Energy cascade in large eddy simulations of turbulent fluid flows. Adv. Geophys. A18, 237 (1974)
Lin, D.N.C., Papaloizou, J.: On the structure and evolution of the primordial solar nebula. Mon. Not. Roy. Astron. Soc. 191, 37–48 (1980)
Lissauer, J.J., Stewart, G.R.: In: Levy, E.H., Lunine, I.J. (eds.) Growth of Planets from Planetesimals in Protostars and Planets III, Univ. Arizona Press, Tucson, 1061 (1993)
Loginov, V.I.: Dehydration and Desalinization of Oil. Khimiya, Moscow (in Russian) (1979)
Lynden-Bell, D., Pringle, J.E.: The evolution of viscous discsand the origin of the nebular variables. Mon. Not. Roy. Astron. Soc. 168, 603–637 (1974a)
Makalkin, A.B..: Radial compaction of the dust subdisk in a protoplanetary disk as possible way to gravitational instability. Lunar Planet. Sci. 25, 827 (1994b)
Makalkin, A.B..: Problems of the Evolution of Protoplanetary Disks in Modern Problems of Mechanics and Space Physics. Fizmatlit, Moscow (in Russian) (2003a). 402
Makalkin, A.B..: Peculiarities of the evolution of a viscous circumsolar protoplanetary disk. Astron. Vestn. 38, 559 (2004a)
Makalkin, A.B.., Dorofeeva, V.A.: Structure of the protoplanetary accretion disk around the sun at the T tauri phase. I Initial data, equations, and modeling methods. Astron. Vestn. 29, 99 (1995a)
Makalkin, A.B.., Dorofeeva, V.A.: Structure of the protoplanetary accretion disk around the sun at the T tauri phase. II. Results of model calculations. Astron. Vestn. 30, 496 (1996)
Marov, M.Y., Kolesnichenko, A.V.: Introduction to Planetary Aeronomy. Nauka, Moscow (in Russian) (1987e)
Marov, M.Y., Kolesnichenko, A.V.: Mechanics of Turbulence of Multicomponent Gases. Kluwer Academic Publishers, Dordrecht–Boston–London (2002b)
Mazin, I.P.: Theoretical estimation of the coagulation coefficient of droplets in clouds. Trudy TsAO 95, 12 (1971)
Mednikov, E.P.: Turbulent Transport and Sedimentation of Aerosols. Nauka, Moscow (in Russian) (1981)
Melville, W.K., Bray, K.N.C.: A Model of the Two-Phase Turbulent Jet. Int. J. Heat Mass Transfer 22, 647 (1979)
Monin, A.S., Yaglom, A.M.: Statistical Hydrodynamics, vol. I. Gidrometeoizdat, St. Petersburg (in Russian) (1992e)
Morkovin, M.V.: Effects of Compressibility on Turbulent Flow in Mechanics of Turbulence. Gordon and Breach, New York (1961b). 367
Nakagawa, Y., Nakagawa, K., Hayashi, C.: Growth and sedimentation of dust grains in the primordial solar nebula. Icarus 45, 517 (1981b)
Nakagawa, Y., Sekiya, M., Hayashi, C.: Settling and growth of dust particles in a laminar phase of a low-mass solar nebula. Icarus 67, 375 (1986a)
Natta, A., Testi, L., Calvet, N., et al.: Dust in Protoplanetary Disks: Properties and Evolution in Protostars and Planets V. Arizona, AZ (2007b)
Nigmatulin, R.I.: Foundations of Mechanics of Heterogeneous Media. Nauka, Moscow (in Russian) (1978)
Nomura, H.: Structure and instabilities of an irradiated viscous protoplanetary disks. Astrophys. J. 567, 587 (2002)
Pollack, J.B., McKay, C.P., Cristofferson, B.M.: A calculation of a rosseland mean opacity of dust grains in primordial solar system nebulae. Icarus 64, 473 (1985)
Prigogine, I., Defay, R.: Chemical Thermodynamics. Longmans Green and Co., London–New York–Toronto (1954d)
Prigogine, I., Stengers, I.: Time. Chaos. Quantum. Toward Solving the Paradox of Time. Progress Publishing House, Moscow (in Russian) (1994c)
Richard, D., Zahn, J.-P.: Turbulence in differentially rotating flow. What can be learned from the Couette-Taylor experiment. Astron. Astrophys. 347, 734 (1999b)
Ruden, S.P., Pollack, J.B.: The dynamical evolution of the protosolar nebula. Asrophys. J. 375, 740 (1991)
Safronov, V.S.: Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets. Nauka, Moscow (in Russian) (1969b)
Safronov, V.S.: Current status of the theory of the Earth’s origin. Dokl. Akad. Nauk USSR, Phys. Earth 6, 5 (1982b)
Safronov, V.S.: Evolution of the dust component of the circumsolar protoplanetary disk. Astron. Vestn. 21, 216 (1987b)
Safronov, V.S., Guseinov, K.M.: On the possibility of in situ comet formation. Astron. Vestn. 1990(24), 248 (1990)
Schmidt, O.Y.: Four Lectures on the Earth’s Origin, 3rd edn. USSR Academy of Sciences, Moscow (in Russian) (1957b)
Schmitt, W., Henning, T., Mucha, R.: Dust evolution in protoplanetary accretion disks. Astron. Astrophys. 325, 569 (1997)
Sekiya, M., Nakagawa, Y.: Settling of dust particles and formation of planetesimals. Prog. Theor. Phys. Suppl. 96, 141 (1988)
Shakura, N.I., Sunyaev, R.A.: Black holes in binary systems. Observational appearance. Astron. Astrophys. 24, 337 (1973b)
Shakura, N.I., Sunyaev, R.A., Zilitinkevich, S.S.: On the turbulent energy transport in accretion disk. Astron. Astrophys. 62, 179 (1978a)
Shapiro, S., Teukolsky, S.: Black Holes, White Dwarfs, and Neutron Stars. John Wiley & Sons, New York (1983a)
Shraiber, A.A., Gavin, L.B., Naumov, V.A., Yatsenko, V.P.: Hydromechanics of Two-Component Flows with Polydisperse Material. Naukova Dumka, Kiev (in Russian) (1980)
Shraiber, A.A., Milyutin, V.N., Yatsenko, V.P.: Turbulent Flows of a Gas Suspension. Naukova Dumka, Kiev (in Russian) (1987)
Smoluchowski, M.: Three Lectures on Diffusion, Brownian Molecular Motion, and Coagulation of Colloidal Particles. Brownian Motion in Colloid Coagulation. ONTI, Moscow (in Russian) (1936)
Soo, S.L., Ihrig, H.K., Kouh, A.F.: Experimental determination of statistical properties of two-phase turbulent motion. Trans. ASME J. Basic Engng. 82, 609 (1960)
Stepinski, T.F., Valageas, P.: Global evolution of solid matter in turbulent protoplanetary disks. I. Aerodynamics of solid particles. Astron. Astrophys. 309, 301 (1996)
Stepinski, T.F., Valageas, P.: Global evolution of solid matter in turbulent protoplanetary disks. II. Development of icy planetesimals. Astron. Astrophys. 319, 1007 (1997)
Sternin, L.E., Shraiber, A.A.: Multiphase Flows of Gas with Particles. Мashinostroenie, Moscow (in Russian) (1994)
Sternin, L.E., Maslov, B.N., Shraiber, A.A., Podvysotskii, A.M.: Two-Phase Mono- and Polydisperse Flows of Gas with Particles. Mashinostroenie, Moscow (in Russian) (1980)
Stokes, G.G.: On the effect of the internal friction of fluids on the motion of pendulums. Trans. Camb. Phil. Soc. 9, 8 (1851)
Takeuchi, T., Lin, D.N.C.: Radial flow of dust particles in accretion disks. Astrophys. J. 581, 1344 (2002)
Takeuchi, T., Lin, D.N.C.: Surface out in optically thick dust disks by the radiation pressure. Astrophys. J. 593, 524 (2003)
Tanga, P., Babiano, A., Dubrulle, B.: Forming planetesimals in vortices. Icarus 121, 158 (1996a)
Tassoul, J.-L.: Theory of Rotating Stars. Princeton University, Princeton (1979a)
Toomre, A.: On the gravitational stability of a disk of stars. Astrophys. J. 139, 1217 (1964b)
Townsend, A.A.: The Structure of Turbulent Shear Flow. Cambridge University, Cambridge (1956c)
Varaksin, A.Y.: Turbulent Flows of Gas with Solid Particles. Fizmatlit, Moscow (in Russian) (2003)
Vereshchagin, I.P., Levitov, V.I., Mirzobekyan, G.Z., Pashin, M.M.: Foundations of Electrogasdynamics of Disperse Systems. Energiya, Moscow (in Russian) (1974)
Voloshchuk, V.M.: Kinetic Theory of Coagulation. Gidrometeoizdat, Moscow (in Russian) (1984)
Voloshchuk, V.M., Sedunov, Y.S.: Coagulation Processes in Disperse Systems. Gidrometeoizdat, Leningrad (in Russian) (1975)
Wadhwa, M., Amelin, Y., Davis, A.M., et al.: From Dust to Planetesimals: Implications for the Solar Protoplanetary Disk from Short-Lived Radionuclides in Protostars and Planets V. Arizona, AZ (2007b)
Wasson, J.T.: Meteorites: Their Record of Early Solar-System History. Freeman, New York (1985)
Watanabe, S., Nakagawa, Y., Nakazawa, K.: Cooling and quasi-static contraction of the primitive solar nebula after gas accretion. Astrophys. J. 358, 282 (1990)
Weidenschilling, S.J.: Aerodynamics of solid bodies in the solar nebula. Mon. Not. R. Astron. Soc. 180, 57 (1977)
Weidenschilling, S.J.: Dust to planetesimals: Settling and coagulation in the solar nebula. Icarus 44, 172 (1980)
Weidenschilling, S.J.: Evolution of grains in a turbulent solar nebula. Icarus 60, 553 (1984)
Whipple, F.L.: From Plasma to Planet, London (1972)
Willacy, K., Klahr, H.H., Millar, T.J., Henning, T.: Gas and Grain Chemistry in a Protoplanetary Disk. Astron. Astrophys. 338, 995 (1998)
Woods, J.D., Drake, J.C., Goldsmith, P.: Coalescence in a turbulent cloud. Quart. J. Roy. Met. Soc. 98, 135 (1972)
Yarin, L.P., Hetsroni, G.: Turbulence intensity in dilute two-phase flow -3. The particles-turbulence interaction in dilute two-phase flow. Int. J. Multiphase Flow 20, 27 (1994)
Youdin, A.N., Goodman, J.: Streaming Instabilities in Protoplanetary Disks, arXiv: Astro-ph/0409263, 1, 1 (2004)
Youdin, A.N., Shu, F.: Planetesimal formation by gravitational instability. Astrophys. J. 580, 494 (2002b)
Zaichik, L.I., Varaksin, A.Y.: Influence of the wake behind large particles on the intensity of carrier-flow turbulence. TVT 37, 1004 (1999)
Zel’dovich, Y.B.: On the friction of fluids between rotating cylinders. Proc. Roy. Soc. London A374, 299 (1981b)
Zuev, Y.V., Lepeshinskii, I.F.: Mathematical model of a two-phase turbulent jet. Izv. Akad. Nauk USSR Ser. MZhG 6, 69 (1981)
Khlopkov, Y.I., Zharov, V.A., Gorelov, S.L.: Coherent Structures in a Turbulent Boundary Layer. Moscow Physicotechnical Institute, Moscow (in Russian) (2002d)
Marov, M.Y., Kolesnichenko, A.V.: Chaotic and ordered structures in the developed turbulence. In: Fridman, A.M., Marov, M.Y. (eds.) Astrophysical Disks: Collective and Stochastic Phenomena, p. 23. Springer, The Netherlands (2006)
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Marov, M.Y., Kolesnichenko, A.V. (2013). Foundations of Mechanics of Heterogeneous Media for Accretion Disks. In: Turbulence and Self-Organization. Astrophysics and Space Science Library, vol 389. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-5155-6_7
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