PACS numbers

95.55.Ka X- and γ-ray telescopes and instrumentation 96.60.−j Solar physics 96.60.qe Flares
  1. S.A. Bogachev, A.S. Ulyanov et alMicroflares and nanoflares in the solar coron63 783–800 (2020)
    95.55.Ka, 96.60.−j, 96.60.Q−, 96.60.qe (all)
  2. A.A. Petrukovich, H.V. Malova et alModern view of the solar wind from micro to macro scales63 801–811 (2020)
    96.50.Ci, 96.60.−j (all)
  3. A.L. Lysenko, D.D. Frederiks et alX-ray and gamma-ray emission from solar flares63 818–832 (2020)
    95.55.Ka, 96.60.−j, 96.60.qe (all)
  4. V.V. Lider “Multilayer X-ray interference structures62 1063–1095 (2019)
    07.85.−m, 41.50.+h, 42.79.Dj, 42.88.+h, 61.05.cp, 78.20.Bh, 78.67.Pt, 95.55.Ka (all)
  5. B.P. Filippov “Mass ejections from the solar atmosphere62 847–864 (2019)
    52.30.−q, 96.60.−j, 96.60.Hv, 96.60.P−, 96.60.Q− (all)
  6. R.L. Aptekar, A.M. Bykov et alCosmic gamma-ray bursts and soft gamma-repeaters — observations and modeling of extreme astrophysical phenomena (100th anniversary of the Ioffe Institute)62 739–753 (2019)
    95.55.Ka, 97.80.Gm, 98.70.Rz (all)
  7. A.S. Lidvansky “G.T. Zatsepin and birth of gamma-ray astronomy61 921–925 (2018)
    07.85.−m, 29.40Ka, 95.55.Ka, 95.85.Pw (all)
  8. V.D. Kuznetsov “Space solar research: achievements and prospects58 621–629 (2015)
    07.87.+v, 96.60.−j (all)
  9. 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)
  10. A.V. Stepanov, V.V. Zaitsev, V.M. Nakariakov “Coronal seismology55 929–935 (2012)
    52.35.−g, 96.60.−j, 97.10.Sj (all)
  11. 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)
  12. 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)
  13. M.M. Barysheva, A.E. Pestov et alPrecision imaging multilayer optics for soft X-rays and extreme ultraviolet bands55 681–699 (2012)
    41.50.+h, 42.79.−e, 95.55.Ka (all)
  14. V.D. Kuznetsov “Solar-terrestrial physics and its applications55 305–314 (2012)
    91.25.Mf, 94.30.−d, 96.60.−j (all)
  15. V.D. Kuznetsov “Space research of the Sun53 947–954 (2010)
    07.87.+v, 52.35.Vd, 96.60.−j (all)
  16. B.V. Somov “Magnetic reconnection in solar flares53 954–958 (2010)
    52.30.Cv, 52.35.Vd, 96.60.qe (all)
  17. 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)
  18. R.L. Aptekar, S.V. Golenetskii et alCosmic gamma-ray bursts and gamma repeaters studies with Ioffe Institute Konus experiments53 401–406 (2010)
    95.55.Ka, 95.85.Pw, 98.70.Rz (all)
  19. G.M. Beskin, S.V. Karpov et alDiscovery of the fast optical variability of GRB 080319B and the prospects for wide-field optical monitoring with high time resolution53 406–414 (2010)
    95.55.Ka, 95.85.Pw, 98.70.Rz (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)
  26. G.D. Fleishman, V.F. Mel’nikov “Millisecond solar radio spikes41 1157–1189 (1998)
  27. M.I. Pudovkin, O.M. Raspopov “Physical mechanism of the action of solar activity and other geophysical factors on the state of the lower atmosphere, meteorological parameters, and climate36 (7) 644–647 (1993)
    96.60.qe, 96.60.Vg, 92.60.Ry, 94.30.Lr (all)
  28. V.G. Ryasnyĭ “Supernova shells33 (5) 393–395 (1990)
    97.60.Bw, 96.10.+i, 97.60.Gb, 97.60.Jd, 96.60.qe (all)
  29. G.S. Ivanov-Kholodnyi “Problems of solar-terrestrial physics and research on the ionosphere31 477–478 (1988)
    96.60.qe, 96.60.Ub, 96.60.Vg, 94.20.wq, 90.00.-x (all)
  30. 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)
  31. I.A. Zhitnik, S.L. Mandel’shtam et alNew observational data on x-ray flares and active regions on the sun28 270–271 (1985)
    96.60.qe, 96.60.Tf (all)
  32. B.V. Somov “New theoretical models of solar flares28 271–272 (1985)
    96.60.qe, 96.60.Iv, 96.60.Mz, 96.60.qd (all)
  33. 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)
  34. K.G. Ivanov “Structure of the Typical Nonstationary Stream of Interplanetary Plasma from Direct Measurements18 807–809 (1975)
    96.50.Ci, 96.50.Qx, 96.50.Fm, 96.50.Tf, 96.50.Ek, 96.60.qe (all)
  35. M.M. Kobrin, A.I. Korshunov, V.V. Pakhomov “Quasiperiodic Components in the Fluctuations of the Solar Radio-frequency Radiation16 287–288 (1973)
    96.60.Tf, 95.55.Jz, 95.55.Ev, 96.60.qe, 96.60.Vg (all)
  36. S.I. Syrovatskii “Current Sheets in Cosmic and Laboratory Plasmas14 533–534 (1972)
    94.30.Kq, 94.30.cq, 94.30.Va, 96.60.qe (all)
  37. S.L. Mandel’shtam “Polarization of the Emission of X-ray Flares on the Sun and their Spectra15 351–352 (1972)
    96.60.qd, 96.60.qe, 96.60.Tf (all)
  38. A.N. Charakhch’yan “Investigation of stratosphere cosmic ray intensity fluctuations induced by processes on the Sun7 358–374 (1964)
    92.60.hd, 96.50.sf, 96.60.qe (all)
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