PACS numbers

52.30.−q Plasma dynamics and flow 96.60.−j Solar physics 96.60.Hv Electric and magnetic fields, solar magnetism 96.60.P− Corona 96.60.Q− Solar activity
  1. B.P. Filippov “Mass ejections from the solar atmosphere62 (9) (2019)
    52.30.−q, 96.60.−j, 96.60.Hv, 96.60.P−, 96.60.Q− (all)
  2. D.A. Dolgolenko, Yu.A. Muromkin “On separation of mixtures of chemical elements in plasma60 994–1017 (2017)
    28.41.Kw, 52.25.Xz, 52.30.−q, 52.75.−d (all)
  3. V.V. Kocharovsky, V.V. Kocharovsky et alThe analytical theory of self-consistent current structures in a collisionless plasma59 1165–1210 (2016)
    52.30.−q, 52.35.−g, 94.30.−d (all)
  4. V.V. Zheleznyakov, E.Ya. Zlotnik et alDouble plasma resonance nd its manifestations in radio astronomy59 997–1020 (2016)
    96.60.P−, 96.60.Tf, 97.60.Gb, 52.35.−g, 52.35.Hr, 52.35.Qz (all)
  5. E.P. Popova “Current results on the asymptotics of dynamo models59 513–530 (2016)
    52.30.Cv, 96.60.Hv, 96.60.Q− (all)
  6. A.V. Nedospasov “Gas rotation in discharges in a longitudinal magnetic field58 574–578 (2015)
    52.27. Lw, 52.30.−q, 52.35. Mw
  7. D.D. Sokoloff “Problems of magnetic dynamo58 601–605 (2015)
    07.55.Db, 41.20.−q, 91.25.−r, 96.12.Hg, 96.60.Hv (all)
  8. V.D. Kuznetsov “Space solar research: achievements and prospects58 621–629 (2015)
    07.87.+v, 96.60.−j (all)
  9. A.V. Timofeev “On the theory of plasma processing of spent nuclear fuel57 990–1021 (2014)
    28.41.Kw, 52.30.−q, 52.35.Tc, 52.40.Fd, 52.50.−b (all)
  10. D.D. Sokoloff, R.A. Stepanov, P.G. Frick “Dynamo: from an astrophysical model to laboratory experiments57 292–311 (2014)
    07.55.Db, 41.20.−q, 91.25.−r, 96.12.Hg, 96.60.Hv (all)
  11. Challenges in astrophysics (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 25 January 2012)55 929–941 (2012)
    01.10.Fv, 26.60.−c, 52.35.−g, 67.10.−j, 96.60.−j, 97.10.Sj, 97.60.Jd (all)
  12. A.V. Stepanov, V.V. Zaitsev, V.M. Nakariakov “Coronal seismology55 929–935 (2012)
    52.35.−g, 96.60.−j, 97.10.Sj (all)
  13. Modern problems in the physical sciences (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 30 November 2011)55 808–837 (2012)
    01.10.Fv, 04.20.−q, 04.70.−s, 47.27.Gs, 47.35.Pq, 68.03.Kn, 72.25.Hg, 72.25.Pn, 72.25.Rb, 71.35.−y, 73.63.Hs, 78.47.−p, 78.67.−n, 96.50.−e, 96.60.−j, 95.75.−z, 98.80.−k (all)
  14. V.G. Kurt, E.N. Mironova “Motion of the Sun through the interstellar medium55 825–831 (2012)
    95.75.−z, 96.50.−e, 96.60.−j (all)
  15. V.D. Kuznetsov “Solar-terrestrial physics and its applications55 305–314 (2012)
    91.25.Mf, 94.30.−d, 96.60.−j (all)
  16. A.G. Zhilkin, D.V. Bisikalo, A.A. Boyarchuk “Flow structure in magnetic close binary stars55 115–136 (2012)
    52.30.−q, 97.10.Gz, 97.80.−d (all)
  17. A.G. Frank “Dynamics of current sheets underlying flare-type events in magnetized plasmas53 941–947 (2010)
    52.30.Cv, 52.35.Vd, 96.60.Q− (all)
  18. V.D. Kuznetsov “Space research of the Sun53 947–954 (2010)
    07.87.+v, 52.35.Vd, 96.60.−j (all)
  19. Yu.D. Kotov “High-energy solar flare processes and their investigation onboard Russian satellite missions CORONAS53 619–631 (2010)
    07.87.+v, 95.55.Ev, 96.60.−j (all)
  20. A.V. Masalov “Spectroscopy: from atoms to cosmic objects52 1147–1152 (2009)
    01.30.Bb, 42.62.Eh, 95.55.−n, 96.60.−j (all)
  21. V.S. Beskin “School of Modern Astrophysics — 200952 1185–1187 (2009)
    01.10.Fv, 96.30.−t, 96.60.−j (all)
  22. V.V. Zaitsev, A.V. Stepanov “Coronal magnetic loops51 1123–1160 (2008)
    52.35.−g, 96.60.−j, 97.10.Sj (all)
  23. V.D. Kuznetsov “Heliophysics: from observations to models49 305–311 (2006)
    01.10.Fv, 95.55.Ev, 95.75.−z, 96.60.−j (all)
  24. V.V. Zaitsev, A.V. Stepanov “Problems of solar activity physics49 311–319 (2006)
    01.10.Fv, 96.60.−j, 96.60.Pb, 97.10.Jb (all)
  25. V.N. Oraevskii, I.I. Sobel’man et alComprehensive solar studies by CORONAS-F satellite: new results45 886–896 (2002)
    96.60.−j
  26. K.A. Razumova “Transport barrier formation in a tokamak plasma44 311–315 (2001)
    52.30.−q, 52.35.−g, 52.55.Fa (all)
  27. K.A. Razumova, A.V. Marchenko “Scientific session of the Division of General Physics and Astronomy of the Russian Academy of Sciences (October 25, 2000)44 311–315 (2001)
    01.10.Fv, 52.30.−q, 52.35.−g, 52.55.Fa, 83.10.Dd, 83.80.Nb, 92.10.Rw (all)
  28. G.D. Fleishman, V.F. Mel’nikov “Millisecond solar radio spikes41 1157–1189 (1998)
    96.60.−j
  29. V.E. Zakharov, E.A. Kuznetsov “Hamiltonian formalism for nonlinear waves40 1087–1116 (1997)
    52.30.−q, 52.35.Ra, 52.55.Fa (all)
  30. V.V. Yan’kov “Attractors and frozen-in invariants in turbulent plasma40 477–493 (1997)
    52.30.−q, 52.35.Ra, 52.55.Fa (all)
  31. R.A. Gulyaev “Erratum: Outer Solar corona as an optical manifestation of a heliospheric current layer [Sov. Phys. Usp. 35, 1083-1085 (December 1992)]36 (5) 454–454 (1993)
    96.60.pf, 96.60.Mz, 96.60.Hv, 96.50.Bh (all)
  32. G.Ya. Smol’kov “New results on microwave emission from active regions of the sun36 (1) 26–28 (1993)
    96.90.+c, 96.60.Q−, 95.55.Ev, 95.55.Jz (all)
  33. R.A. Gulyaev “Outer solar corona as an optical manifestation of the heliospheric current sheet35 (12) 1083–1085 (1992)
    96.60.pf, 96.60.Mz, 96.60.Hv, 96.50.Bh (all)
  34. I.V. Sokolov “Hydrodynamic cumulative processes in plasma physics33 (11) 960–973 (1990)
    52.35.Tc, 52.30.−q (all)
  35. A.I. Morozov “Development of the principles of a quasi-steady-state plasma accelerator with an intrinsic magnetic field with a power of 109-1011 W33 (7) 576–577 (1990)
    52.59.−f, 52.65.Kj, 52.25.Xz, 52.55.Fa, 52.30.−q (all)
  36. Yu.S. Protasov “First All-Union Symposium on Radiation Plasmodynamics33 (7) 583–584 (1990)
    52.35.Tc, 52.25.Kn, 52.70.Kz, 52.50.Dg, 52.30.−q, 01.30.Cc (all)
  37. A.Z. Dolginov “Origin of the magnetic fields of the earth and celestial bodies30 475–493 (1987)
    97.30.Fi, 91.25.−r, 96.60.Hv, 97.20.Ec, 91.35.Ed (all)
  38. Ya.B. Zeldovich, A.A. Ruzmaikin “The hydromagnetic dynamo as the source of planetary, solar, and galactic magnetism30 494–506 (1987)
    91.25.Mf, 96.12.Hg, 96.15.Gh, 96.60.Hv, 98.35.Eg (all)
  39. A.A. Ruzmaikin “Magnetic fields on the sun29 1069–1070 (1986)
    96.60.Hv, 96.60.Bn, 96.60.Q− (all)
  40. B.E. Meierovich “Toward the realization of electromagnetic collapse29 506–529 (1986)
    52.58.Lq, 52.35.Py, 52.30.−q (all)
  41. G.Ya. Smol’kov, T.A. Treskov, A.A. Pistol’kors “Commissioning of the Siberian Solar Radiotelescope and the results of first observations28 1052–1054 (1985)
    96.60.Q−, 95.55.Ev, 95.55.Jz, 95.75.Kk (all)
  42. E.R. Mustel’, V.E. Chertoprud, N.B. Mulyukova “Energy sources for atmospheric cyclones28 526–526 (1985)
    92.60.Qx, 92.60.hv, 96.60.Q−, 94.30.Lr, 94.30.Xy (all)
  43. S.I. Gopasyuk “Dynamics of the magnetic field, electric currents, and flares in active regions on the sun28 269–270 (1985)
    01.30.Cc, 96.60.qe, 96.60.Hv, 96.60.qd, 96.60.Mz (all)
  44. S.A. Kazantsev “Astrophysical and laboratory applications of self-alignment26 328–351 (1983)
    31.50.+w, 95.30.Es, 96.60.−j, 52.20.Hv (all)
  45. V.A. Krat “Prospects for Development of Solar Physics at the Main Astronomical Observatory of the USSR Academy of Sciences18 799–799 (1975)
    95.55.Ev, 95.75.−z, 96.60.Q− (all)
  46. É.R. Mustel’ “Action of Solar Particle Fluxes on the Lower Layers of the Earth’s Atmosphere16 739–740 (1974)
    96.60.Q−, 92.60.hv, 94.30.Lr, 92.60.Ry, 92.60.Qx (all)
  47. S.M. Osovets “Dynamic methods of confinement and stabilization of hot plasma17 239–262 (1974)
    52.58.Lq, 52.25.−b, 52.35.Py, 52.30.−q, 52.65.Kj (all)
  48. V.A. Krat “First Results from the Third Flight of the Soviet Solar Stratospheric Observatory14 804–804 (1972)
    96.60.Mz, 96.60.Hv, 96.60.qd, 95.55.Ev, 95.55.Qf (all)
  49. V.N. Kuril’chik “Relativistic Electrons in Extragalactic Radio Sources14 804–805 (1972)
    01.10.Fv, 96.60.qd, 96.60.Mz, 96.60.Hv, 96.60.Na (all)
  50. S.I. Vainshtein, Ya.B. Zel’dovich “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)15 159–172 (1972)
    95.85.Sz, 95.30.Qd, 96.60.Hv, 97.10.Ld (all)
  51. A.V. Timofeev “Oscillations of inhomogeneous flows of plasma and liquids13 632–646 (1971)
    52.30.−q, 52.35.Py, 47.20.−k, 47.10.ab, 52.65.Vv (all)
  52. A.B. Severnyi “Certain New Results of Measurements of the Total Magnetic Field of the Sun and of the Stars13 663–663 (1971)
    96.60.Hv, 96.60.Bn, 96.60.qd, 97.10.Ld, 97.20.Pm, 95.55.Ev, 95.55.Qf (all)
  53. A.A. Mikhailov “Motion of the Earth’s Poles13 663–664 (1971)
    96.60.Hv, 96.60.Bn, 96.60.qd, 97.10.Ld, 97.20.Pm, 97.10.Cv, 97.10.Kc, 95.55.Fw, 95.55.Qf (all)
  54. S.A. Kaplan, V.N. Tsytovich “Plasma radiation mechanisms in astrophysics12 42–63 (1969)
    96.50.Tf, 98.54.Aj, 96.60.P− (all)
  55. N.A. Lotova “Radioastronomical investigations of the inhomogeneous structure of the near-solar plasma11 424–434 (1968)
    96.60.P−, 96.60.Vg, 95.30.Qd, 96.50.Ci, 98.70.Dk (all)
  56. M.N. Gnevyshev “The eleven year cycle of solar activity9 752–758 (1967)
    96.60.qd, 96.60.P− (all)
  57. S.B. Pikel’ner “Dynamics of the solar atmosphere9 236–250 (1966)
    96.60.Ly, 96.60.qd, 96.60.Na, 97.10.Ex, 96.60.Bn, 96.60.Hv (all)
  58. A.B. Severnyi “Magnetic fields of the Sun and stars9 1–30 (1966)
    96.60.Hv, 96.60.qd, 97.10.Ld, 97.10.Tk (all)
  59. N.B. Divari “Zodiacal light7 681–695 (1965)
    96.50.Dj, 96.60.Ub, 96.60.P− (all)
  60. V.I. Krasovskii “Some results of igy and igc research on the aurora and night glow4 904–918 (1962)
    92.60.hw, 96.60.Q−, 94.20.Ac, 94.30.Xy (all)
  61. I.S. Shklovskii “The ultraviolet radiation and soft X-rays of the Sun4 812–834 (1962)
    92.60.Vb, 94.20.de, 94.20.dg, 94.20.dj, 94.20.wq, 96.60.Q− (all)
  62. V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic rays3 504–541 (1961)
    96.50.sb, 96.50.Dj, 97.60.Bw, 96.60.Q−, 98.70.Sa (all)
  63. A.A. Vedenov, E.P. Velikhov, R.Z. Sagdeev “STABILITY OF PLASMA4 332–369 (1961)
    52.35.Qz, 52.30.−q (all)
  64. L.A. Artsimovich “Research on controlled thermonuclear reactions in the U.S.S.R.1 191–207 (1958)
    52.55.Lf, 25.60.Pj, 52.30.−q, 28.52.−s, 52.50.Dg (all)
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