Summary
Solution of the linear kinetic dispersion equation shows that cometary new-born ions with large perpendicular energies (large initial angles between the solar wind velocity and the IMF) can excite a wave mode with rest frame frequencies of the order of the heavy ion cyclotron frequency which exhibits maximum growth slightly away (6°–15°) from parallel propagation, together with high mass density compression ratios and almost linear polarization. The association of these properties is relevant to space observations of MHD-like waves at comets and in planetary foreshocks and has not been reported in the vast literature on possible instability mechanisms. Dilute drifting oxygen ion and photoelectron rings with finite thermal spreads model the free energy source in the solar wind frame. For parallel propagation, the mode of interest is left-hand circularly polarized, moves in the direction of the newborn particles, and is predominantly fed by the perpendicular energy of the heavy ions; as obliquity increases, its polarization and compression change rapidly. Modification of the free energy source parameters (ring density, drift velocity, perpendicular speed and thermal spread) determines their relative influence, defines the domain of existence of the mode, and shows that it might evolve into a nonoscillatory, purely growing structure distinct from the mirror wave. The results are also applicable to non-cometary environments.
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References
Anderson, R.R., C.C. Harvey, M.M. Hoppe, B.T. Tsurutani, T.E. Eastman, J. Etcheto: 1982, J. Geophys. Res. 87, 2082
Belcher, J.W., L. Davis, Jr.: 1971, J. Geophys. Res. 76, 3534
Burlaga, L.F.: 1971, J. Geophys. Res. 76, 4360
Coleman, P.J., Jr.: 1966, J. Geophys. Res. 71, 5509
Gary, S.P., C.W. Smith, M.A. Lee, M.L. Goldstein, D.W. Forslund: 1984, Phys. Fluids 27, 1852
Gary, S.P., C.D. Madland, B.T. Tsurutani.: 1985, Phys. Fluids 28, 3691
Goldstein, M., W. Wong, A. Vifias, C. Smith: 1985, J. Geophys. Res. 90, 302
Hada, T.: 1985, Ph.D. Thesis, UCLA
Hada, T., M. Ashour-Abdalla.: 1986, EOS 67, 1167
Hasegawa, A.: 1969, Phys. Fluids 12, 2642
Hoppe, M., C.T. Russel, L.A. Frank, T.E. Eastman, E.W. Greenstadt: 1981, J. Geophys. Res. 86, 4471
Ipavich, F.M., A.B. Galvin, G. Gloeckler, D. Hovestadt, B. Klecker, M. Scholer: 1986, Science 232, 366
Kaufmann, R.L., J.T. Horng, A. Wolfe: 1970, J. Geophys. Res. 75, 4666
Kennel, C.F., H.E. Petschek: 1966, J. Geophys. Res. 71, 1
Krall, N.A., and A.W. Trievelpiece: 1973, Principles of Plasma Physics, McGraw-Hill, New York, p. 405
Kraus, J.D.: 1966, Radio Astronomy, Chap. 4, McGraw-Hill, New York
Lanzerotti, L.J., A. Hasegawa, C.G. Maclennan: 1969, J. Geophys. Res. 74, 5565
Lee, J.C., F.W. Crawford.: 1970, J. Geophys. Res. 75, 85
Lepping, R.P., K.W. Behannon: 1986, J. Geophys. Res. 91, 8725
Neubauer, F., K. Glessmeier, M. Pohl, J. Raeder, M. Acufia, L. Burlaga, N. Ness, G. Musmann, F. Mariani, M. Wallis, E. Ungstrup, H. Schmidt: 1986, Nature 321, 352
Neugebauer, M., D.R. Clay, B.E. Goldstein, B.T. Tsurutani, R.D. Zwickl: 1984, J. Geophys. Res. 89, 5395
Neugebauer, M., C.J. Alexander, R. Schwenn, A.K. Richter: 1986, J. Geophys. Res. 91, 13694
Price, C.P., D.W. Swift, L.C. Lee: 1986, J. Geophys. Res. 91, 101
Riedler, W., K. Schwingenschuk, Ye. G. Yeroshenko, V.A. Styashkin, C. T. Russel: 1986, Nature 321, 288
Roberts, D.A., L.W. Klein, M.L. Goldstein: 1986, EOS 67, 1149
Rönnmark, K.: 1982, Kiruna Geophysical Institute Report No. 179
Rönnmark, K.: 1983, Plasma Phys. 25, 699
Sharma, O., V. Patel: 1986, J. Geophys. Res. 91, 1529
Smith, E.J.: 1973, J. Geophys. Res. 78, 2054
Smith, R.L., N. Brice: 1964, J. Geophys. Res. 69, 5029
Smith, C.W., M.A. Lee: 1986, J. Geophys. Res. 91, 81
Smith, E.J., B.T. Tsurutani, D.L. Chenette, T.F. Conlon, J.A. Simpson: 1976, J. Geophys. Res. 81, 65
Smith, C.W., M.L. Goldstein, S.P. Gary, C.T. Russel: 1985, J. Geophys. Res. 90, 1429
Southwood, D.J., W.J. Hughes: 1983, Space Sci. Rev. 35, 301
Southwood, D.J., W.J. Hughes: 1983, Space Sci. Rev. 35, 301
Tsurutani, B.T., E.J. Smith: 1979, J. Geophys. Res. 84, 2773
Tsurutani, B.T., E.J. Smith: 1984, Geophys. Res. Letters 11, 331
Tsurutani, B.T., E.J. Smith: 1986a, Geophys. Res. Letters 13, 263
Tsurutani, B.T., E.J. Smith: 1986b, Geophys. Res. Letters 13, 259
Tsurutani, B.T., E.J. Smith, R.R. Anderson, K.W. Ogilvie, J.D. Scudder, D.N. Baker, S.J. Bame: 1982, J. Geophys. Res. 87, 6060
Tsurutani, B.T., E.J. Smith, D.E. Jones: 1983, J. Geophys. Res. 88, 5645
Tsurutani, B.T., R.M. Thorne, E.J. Smith, J.T. Gosling, H. Matsumoto: 1987, J. Geophys. Res. (submitted)
Vinas, A.I., M.L. Goldstein, M.H. Acura: 1984, J. Geophys. Res. 89, 6813
Winske, D., C.S. Wu, Y.Y. Li, Z.Z. Mou, S.Y. Guo: 1985, J. Geophys. Res. 90, 2713
Wong, H.K., M.L. Goldstein: 1986, J. Geophys. Res. 91, 5617
Wu, C.S., R.E. Hartle: 1974, J. Geophys. Res. 79, 283
Young, D.T., S. Perrault, A. Roux, C. de Villedary, R. Gendrin, A. Korth, G. Kremser, D. Jones: 1981, J. Geophys. Res. 86, 6755
Yumoto, K., T. Saito, T. Nakagawa: 1986, Geophys. Res. Letters 13, 825
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Brinca, A.L., Tsurutani, B.T. (1988). Unusual characteristics of electromagnetic waves excited by cometary newborn ions with large perpendicular energies. In: Grewing, M., Praderie, F., Reinhard, R. (eds) Exploration of Halley’s Comet. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-82971-0_57
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