PACS numbers

47.27.−i Turbulent flows 47.32.−y Vortex dynamics; rotating fluids 97.10.−q Stellar characteristics and properties
  1. M.V. Kalashnik, M.V. Kurgansky, O.G. Chkhetiani “Baroclinic instability in geophysical fluid dynamics65 1039–1070 (2022)
    05.45.−a, 47.10.−g, 47.20.Ft, 47.20.Ky, 47.27.Cn, 47.32.−y, 47.32.Ef, 47.32.cd, 47.85.Dh, 92.10.Lq, 92.60.−e, 92.60.hk (all)
  2. D.S. Agafontsev, E.A. Kuznetsov et alCompressible vortex structures and their role in the onset of hydrodynamic turbulence65 189–208 (2022)
    47.10.−g, 47.27.−i, 47.32.−y (all)
  3. V.P. Lukin “Outer scale of turbulence and its influence on fluctuations of optical waves64 280–303 (2021)
    42.68.Bz, 47.27.−i, 92.60.hn (all)
  4. V.E. Panchuk, Yu.Yu. Balega et alStudy of exoplanets by spectroscopic methods63 562–582 (2020)
    95.75.Fg, 97.10.−q, 97.82.−j (all)
  5. V.I. Klyatskin “Stochastic structure formation in random media59 67–95 (2016)
    05.40.−a, 05.45.−a, 46.65.+g, 47.27.−i (all)
  6. O.G. Bakunin “Stochastic instability and turbulent transport. Characteristic scales, increments, diffusion coefficients58 252–285 (2015)
    05.40.−a, 47.27.−i, 47.53.+n (all)
  7. I.I. Vigdorovich “Does the power formula describe turbulent velocity profiles in tubes? (comment on "Turbulent flows at very large Reynolds numbers: new lessons learned" [Phys. Usp. 57 250 (2014); 58 196–198 (2015)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  8. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “On the problem of turbulent flows in pipes at very large Reynolds numbers (reply to comment by I I Vigdorovich [Phys. Usp. 58 (2015); Usp. Fiz. Nauk 185 213 (2015)] on "Turbulent flows at very large Reynolds numbers: new lessons learned" [Phys. Usp. 57 250 (2014); Usp. Fiz. Nauk184 265 (2014)])58 199–201 (2015)
    47.27.−i, 47.27.Ak, 47.27.N− (all)
  9. N.S. Kardashev, I.D. Novikov et alReview of scientific topics for Millimetron space observatory57 1199–1228 (2014)
    07.87.+v, 95.55.−n, 97.10.−q, 98.62.−g, 98.80.−k (all)
  10. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “Corrigenda to the paper by G I Barenblatt, A J Chorin, V M Prostokishin "Turbulent flows at very large Reynolds numbers: new lessons learned" (Usp. Fiz. Nauk, March 2014, Vol. 184, No. 3, pp. 265—272)57 1248–1248 (2014)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  11. E.P. Kurbatov, D.V. Bisikalo, P.V. Kaygorodov “On the possible turbulence mechanism in accretion disks in nonmagnetic binary stars57 787–798 (2014)
    47.20.−k, 47.27.−i, 95.30.Lz (all)
  12. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “Turbulent flows at very large Reynolds numbers: new lessons learned57 250–256 (2014)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  13. O.G. Bakunin “The role of B.B. Kadomtsev’s ideas in shaping the current understanding of turbulent transport56 1132–1149 (2013)
    05.40.−a, 47.27.−i, 47.53.+n (all)
  14. V.E. Zakharov, V.I. Karas’ “Nonequilibrium Kolmogorov-type particle distributions and their applications56 49–78 (2013)
    47.11.−j, 47.27.−i, 47.27.ek, 52.25.Dg (all)
  15. V.P. Budaev, S.P. Savin, L.M. Zelenyi “Investigation of intermittency and generalized self-similarity of turbulent boundary layers in laboratory and magnetospheric plasmas: towards a quantitative definition of plasma transport features54 875–918 (2011)
    05.45.−a, 47.27.−i, 52.35.Ra (all)
  16. V.I. Klyatskin “Integral characteristics: a key to understanding structure formation in stochastic dynamic systems54 441–464 (2011)
    05.40.−a, 05.45.−a, 46.65.+g, 47.27.−i (all)
  17. P.S. Landa, D.I. Trubetskov, V.A. Gusev “Delusions versus reality in some physics problems: theory and experiment52 235–255 (2009)
    01.65.+g, 47.27.−i, 84.40.Fe (all)
  18. V.I. Balykin, A.N. Ryabtsev et alOn the 40th anniversary of the Institute of Spectroscopy of the Russian Academy of Sciences (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 8 October 2008)52 275–309 (2009)
    03.75.−b, 03.75.Hh, 05.30.Jp, 07.07.−a, 32.30.−r, 32.30.Jc, 33.20.−t, 36.40.−c, 37.20.+j, 42.82.Cr, 61.43.−j, 63.20.−e, 63.50.−x, 67.25.dw, 71.35.Lk, 71.36.+c, 78.30.−j, 78.47.−p, 78.55.−m, 81.07.−b, 87.85.fk, 87.64.−t, 95.30.Ky, 97.10.−q (all)
  19. A.N. Ryabtsev, S.S. Churilov “Spectroscopy of ionized atoms for astrophysics and nanotechnology52 282–286 (2009)
    32.30.−r, 32.30.Jc, 42.82.Cr, 95.30.Ky, 97.10.−q (all)
  20. A.M. Fridman, D.V. Bisikalo “The nature of accretion disks of close binary stars: overreflection instability and developed turbulence51 551–576 (2008)
    47.27.−i, 97.10.Gz, 97.80.−d (all)
  21. O.G. Onishchenko, O.A. Pokhotelov, N.M. Astaf’eva “Generation of large-scale eddies and zonal winds in planetary atmospheres51 577–589 (2008)
    47.27.−i, 92.10.hf, 92.60.−e (all)
  22. S.B. Popov, M.E. Prokhorov “Population synthesis in astrophysics50 1123–1146 (2007)
    97.10.−q, 97.60.Jd, 97.80.−d (all)
  23. L.L. Kichatinov “The differential rotation of stars48 449–467 (2005)
    47.27.−i, 47.32.−y, 97.10.−q (all)
  24. Yu.N. Efremov, A.D. Chernin “Large-scale star formation in galaxies46 1–20 (2003)
    97.10.−q, 98.20.Bg, 98.58.Db (all)
  25. V.F. Kop’ev, S.A. Chernyshev “Vortex ring oscillations, the development of turbulence in vortex rings and generation of sound43 663–690 (2000)
    43.30.−k, 47.27.−i, 47.27.Sd, 47.32.−y (all)
  26. P.K. Volkov “Similarity in problems related to zero-gravity hydromechanics41 1211–1217 (1998)
    03.40.Gc, 47.27.−i
  27. R.E. Gershberg “Flaring red dwarf stars: news from Crimea41 807–814 (1998)
    96.60.Qc, 97.10.−q, 97.20.−w, 97.30.−b (all)
  28. A.F. Gutsol “The Ranque effect40 639–658 (1997)
    47.32.−y
  29. S.K. Betyaev “Hydrodynamics: problems and paradoxes38 287–316 (1995)
    42.11.+j, 47.27.−i, 47.32.−y (all)
  30. A.G. Bershadskii “Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean33 (12) 1073–1075 (1990)
    47.53.+n, 92.10.Lq, 47.27.−i, 95.30.Lz, 05.45.Df (all)
  31. S.G. Chefranov “Advances in investigating turbulence33 (11) 994–995 (1990)
    47.27.−i, 01.30.Cc (all)
  32. B.S. Kerner, V.V. Osipov “Self-organization in active distributed media: scenarios for the spontaneous formation and evolution of dissipative structures33 (9) 679–719 (1990)
    47.27.−i, 72.30.+q (all)
  33. V.A. Dogel’ “Differential rotation and stellar convection33 (5) 392–392 (1990)
    96.60.Bn, 96.60.qd, 47.27.−i, 95.30.Lz (all)
  34. M.I. Rabinovich, M.M. Sushchik “The regular and chaotic dynamics of structures in fluid flows33 (1) 1–35 (1990)
    47.52.+j, 47.27.ed, 47.27.Jv, 47.32.−y (all)
  35. Yu.A. Stepanyants, A.L. Fabrikant “Propagation of waves in hydrodynamic shear flows32 783–805 (1989)
    47.35.De, 47.35.Rs, 47.35.Bb, 47.32.−y (all)
  36. V.I. Tatarskii “Criteria for the degree of chaos32 450–451 (1989)
    47.52.+j, 47.15.−x, 47.27.−i (all)
  37. A.V. Gaponov-Grekhov, M.I. Rabinovich “Nonlinear dynamics of nonequilibrium media: structures and turbulence30 433–434 (1987)
    01.10.Fv, 05.45.−a, 47.27.−i, 47.52.+j (all)
  38. B.S. Rinkevicius “The Doppler method of measuring local velocities using lasers16 712–725 (1974)
    47.80.Cb, 47.15.−x, 41.20.Jb, 47.85.Dh, 85.60.Gz, 47.27.−i (all)
  39. V.N. Tsytovich “Development of the concepts of plasma turbulence15 632–650 (1973)
    52.35.Ra, 52.25.Fi, 47.27.−i (all)
  40. D.A. Frank-Kamenetskii “Kirill Ivanovich Shchelkin (obituary)12 305–306 (1969)
    01.60.+q, 47.40.Rs, 47.27.−i (all)
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