Abstract
According to the data of the BMSW/SPEKTR-R instrument, which measured the density and velocity of solar wind plasma with a record time resolution, up to ~3 ×10–2 s, the structure of the front of interplanetary shocks has been investigated. The results of these first investigations were compared with the results of studying the structure of the bow shocks obtained in previous years. A comparison has shown that the quasi-stationary (averaged over the rapid oscillations) distribution of plasma behind the interplanetary shock front was significantly more inhomogeneous than that behind the bow-shock front, i.e., in the magnetosheath. It has also been shown that, to determine the size of internal structures of the fronts of quasi-perpendicular (θBN > 45°) shocks, one could use the magnetic field magnitude, the proton density, and the proton flux of the solar wind on almost equal terms. A comparison of low Mach (М А < 2), low beta (β1 < 1) fronts of interplanetary and bow shocks has shown that the dispersion of oblique magnetosonic waves plays an essential role in their formation.
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References
Sagdeev, R.Z., Collective processes and shock waves in low-density plasma, in Voprosy teorii plazmy (Problems in the Theory of Plasma), Moscow: Atomizdat, 1964, vol. 4, pp. 20–80.
Galeev, A.A. and Sagdeev, R.Z., Lectures on the Non-Linear Theory of Plasma, Trieste, Italy, 1966, p. 35.
Tidman, D.A., Turbulent shock waves in plasma, Phys. Fluids, 1967, vol. 10, pp. 547–568.
Iskol’dskii, A.M., Kurtmullaev, R.Kh., Nesterikhin, Yu.E., et al., Experimental investigation of collisionless shock waves in a plasma, Sov. Phys. JETP, 1965, vol. 20, no. 2, pp. 517–519.
Zagorodnikov, S.P., Rudakov, L.I., Smolkin, G.E., et al., Observation of shock waves in a collisionless plasma, Sov. Phys. JETP, 1965, vol. 20, no. 5, pp. 1154–1156.
Paul, J.W.H., Holmes, L.S., Parkinson, M.J., et al., Experimental observations on the structure of collisionless shock waves in a magnetized plasma, Nature, 1965, vol. 208, pp. 133–135.
Alikhanov, S.G., Belan, V.G., and Sagdeev, R.Z., Nonlinear ion-acoustic waves in a plasma, JETP Lett., 1968, vol. 7, no. 11, pp. 405–408.
Wong, A.Y. and Means, R.W., Evolution of turbulent electrostatic shock, Phys. Rev. Lett., 1971, vol. 27, no. 15, pp. 973–976.
Volkov, O.L., Eselevich, V.G., Kichigin, G.N., et al., Turbulent shock wave in a low-density unmagnetized plasma, Sov. Phys. JETP, 1975, vol. 40, no. 5, pp. 841–842.
Moreno, G., Olbert, S., and Pai, L., Risultati di IMP-1 sul vento solare, Quad. Ric. Sci., 1966, vol. 45, pp. 119–135.
Bame, S.J., Asbridge, J.R., Gosling, J.T., et al., High temporal resolution observations of electron heating at the bow shock, Space Sci. Rev., 1979, vol. 23, no. 1, pp. 75–92.
Vaisberg, O.L., Galeev, A.A., Klimov, S.I., et al., Energy dissipation mechanisms in high-M collisionless shock waves: A study based on measurements by the Prognoz 8 satellite, JETP Lett., 1982, vol. 35, no. 1, pp. 30–33.
Eselevich, V.G., Bow shock structure from laboratory and satellite experimental results, Planet. Space Sci., 1983, vol. 31, no. 6, pp. 615–631.
Šafránková, J., Němeček, Z., Přech, L., et al., Fast solar wind monitor (BMSW): Description and first results, Space Sci. Rev., 2013, vol. 175, no. 1, pp. 165–182.
Zastenker, G.N., Šafránková, J., Němeček, Z., et al., Fast measurements of parameters of the Solar Wind using the BMSW instrument, Cosmic Res., 2013, vol. 51, no. 2, pp. 78–89.
Němeček, Z., Šafránková, J., Goncharov, O., et al., Ion scales of quasi-perpendicular low-Mach-number interplanetary shocks, Geophys. Res. Lett., 2013, vol. 40, pp. 4133–4137.
Burlaga, L., Sitteler, E., Mariani, F., and Schwenn, R., Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP8 observations, J. Geophys. Res., 1981, vol. 86, no. A8, pp. 6673–6684.
Burlaga, L., Klein, L., Sheeley, N.R., Jr., et al., A magnetic cloud and a coronal mass ejection, Geophys. Res. Lett., 1982, vol. 9, no. 12, pp. 1317–1320.
Burlaga, L., Micro-scale structure in the interplanetary medium, Sol. Phys., 1968, no. 4, pp. 67–92.
Eselevich, M.V. and Eselevich, V.G., Fractal structure of the heliospheric plasma sheet in the Earth’s orbit, Geomagn Aeron. (Engl. Transl.), 2005, vol. 45, no. 3, pp. 326–336.
Eselevich, V.G., Shock wave structure in collisionless plasmas from results of laboratory experiments, Space Sci. Rev., 1982, vol. 32, no. 1, pp. 65–81.
Greensdadt, E.W., Russell, C.T., Scarf, F.L., et al., Structure of the quasi-perpendicular laminar bow shock, J. Geophys. Res., 1975, vol. 80, no. 4, pp. 502–514.
Paschmann, G., Sckopke, N., Bame, S.J., and Gosling, J.T., Observations of gyrating ions in the foot of the nearly perpendicular bow shock, Geophys. Res. Lett., 1982, vol. 9, no. 8, pp. 881–884.
Newbury, J.A., Russell, C.T., and Gedalin, M., The ramp width of high-Mach-number, quasi-perpendicular collisionless shocks, J. Geophys. Res., 1998, vol. 103, no. A12, pp. 29581–29593.
Farris, M.H., Russell, C.T., and Thomsen, M.F., Magnetic structure of the low beta, quasi-perpendicular shock, J. Geophys. Res., 1993, vol. 98, no. A9, pp. 15285–15294.
Eselevich, V.G., Es’kov, A.G., Kurtmullaev, R.Kh., et al., Isomagnetic discontinuity in a collisionless shock wave, Sov. Phys. JETP, 1971, vol. 33, no. 6, pp. 1120–1126.
Balikhin, M.A., Nozdrachev, M., Dunlop, M., et al., Observation of the terrestrial bow shock in quasi-electrostatic subshock regime, J. Geophys. Res., 2002, vol. 107, no. A8, pp. SSH 1-1–SSH 1-9.
Kennel, C.F., Edmiston, J.P., and Hada, T., A quarter century of collisionless shock research, in Collisionless Shocks in the Heliosphere: A Tutorial Review, Stone, R.G. and Tsurutani, B.T., Eds., Washington, D.C.: Am. Geophys. Union, 1985, vol. 34, pp. 1–36.
Song, P. and Russell, C.T., Time series data analyses in space physics, Space Sci. Rev., 1999, vol. 87, no. 3, pp. 387–463.
Fairfield, D.H. and Feldman, W.C., Standing waves at low Mach number laminar bow shocks, J. Geophys. Res., 1975, vol. 80, pp. 515–522.
Fredricks, R.W., Crook, Q.M., Kennel, C.F., et al., OGO 5 observation of electrostatic turbulence in bow shock magnetic structure, J. Geophys. Res., 1970, vol. 75, pp. 3751–3768.
Formisano, V., Hedgecock, P.C., Moreno, G., et al., Observations of Earth’s bow shock for low Mach numbers, Planet. Space Sci., 1971, vol. 19, no. 11, pp. 1519–1531.
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Original Russian Text © V.G. Eselevich, N.L. Borodkova, M.V. Eselevich, G.N. Zastenker, Y. Šafránkova, Z. Němeček, L. Přech, 2017, published in Kosmicheskie Issledovaniya, 2017, Vol. 55, No. 1, pp. 32–47.
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Eselevich, V.G., Borodkova, N.L., Eselevich, M.V. et al. Fine structure of the interplanetary shock front according to measurements of the ion flux of the solar wind with high time resolution. Cosmic Res 55, 30–45 (2017). https://doi.org/10.1134/S0010952517010038
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DOI: https://doi.org/10.1134/S0010952517010038