Abstract
A new model for solar spike bursts is considered based on the interaction of Langmuir waves with ion-sound waves: l+s→t. Such a mechanism can operate in shock fronts, propagating from a magnetic reconnection region. New observations of microwave millisecond spikes are discussed. They have been observed in two events: 4 November 1997 between 05:52–06:10 UT and 28 November 1997 between 05:00–05:10 UT using the multichannel spectrograph in the range 2.6–3.8 GHz of Beijing AO. Yohkoh/SXT images in the AR and SOHO EIT images testify to a reconstruction of bright loops after the escape of a CME. A fast shock front might be manifested as a very bright line in T e SXT maps (up to 20 MK) above dense structures in emission measure (EM) maps. Moreover one can see at the moment of spike emission (for the 28 November 1997 event) an additional maximum at the loop top on the HXR map in the AR as principal evidence of fast shock propagation. The model gives the ordinary mode of spike emission. Sometimes we observed a different polarization of microwave spikes that might be connected with the depolarization of the emission in the transverse magnetic field and rather in the vanishing magnetic field in the middle of the QT region. Duration and frequency band of isolated spikes are connected with parameters of fast particle beams and shock front. Millisecond microwave spikes are probably a unique manifestation of flare fast shocks in the radio emission.
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References
Allaart, M. A. F. et al.: 1990, Atlas of Fine Structure in Solar Microwave Bursts, Sterrenkundig Instituut, Utrecht.
Altyntsev, A. T., Grechnev, V. V., Konovalov, S. K. et al.: 1996, Astrophys. J. 469, 976.
Altyntsev, A. T., Grechnev, V. V., and Hanaoka, Y.: 1998, Solar Phys. 178, 575.
Aschwanden, M. J.: 1990, Astron. Astrophys. 237, 512.
Aschwanden, M. J. and Güdel, M.: 1992, Astrophys. J. 401, 736.
Benz, A. O.: 1986, Solar Phys. 104, 99.
Benz, A. O.: 1993, Plasma Astrophysics, Kluwer Academic Publishers, Dordrecht, Holland.
Benz, A. O. and Güdel, M.: Solar Phys. 111, 175.
Benz, A. O. and Wentzel, D.: 1981, Astron. Astrophys. 94, 100.
Chernov, G. P.: 1990, Solar Phys. 130, 234.
Chernov, G. P. and Fomichev, V. V.: 1989, Soviet Astron. Lett. 15, 410.
Chernov, G. P. and Zlobec, P.: 1995, Solar Phys. 160, 79.
Fleishman, G. D. and Mel'nikov, V. F.: 1998, Uspehi Fizicheskih Nauk 168, 1265.
Fomichev, V. V. and Fainstein, S. M.: 1988, Soviet Astron. 65, 1058 (in Russian).
Fu, Q. J., Gong, Y. F., Jin, S. Z., and Zhao, R. Y.: 1990, Solar Phys. 130, 161.
Güdel, M.: 1990, Astron. Astrophys. 239,L1.
Güdel, M. and Benz, A. O.: 1990, Astron. Astrophys. 231, 202.
Güdel, M. and Zlobec, P.: 1991, Astron. Astrophys. 245, 299.
Gurnett, D. A. et al.: 1979, J. Geophys. Res. 84, 2029.
Karlický, M., Sobotka, M., and Jiřička, K.: 1996, Solar Phys. 168, 375.
Krucker, S., Benz, A. O., and Aschwanden, M. J.: 1997, Astron. Astrophys. 317, 569.
Krucker, S., Aschwanden, M. J., Bastian, T. S., and Benz, A. O.: 1995a, Astron. Astrophys. 302, 551.
Krucker, S., Benz, A. O., Aschwanden, M. J., and Bastian, T. S.: 1995b, Solar Phys. 160, 151.
Li, C. S., Fu, Q. J., and Li, H. W.: 1991, Solar Phys. 131, 337.
Melrose, D. B.: 1980, Plasma Astrophysics, Gordon and Breach Publishers, New York.
Melrose, D. B.: 1989, Solar Phys. 119. 143.
Melrose, D. B. and Dulk, G. A.: 1982, Astrophys. J. 259, 844.
Melrose, D. B. and Robinson, P. A.: 1994, Proc. Astron. Soc. Austr. 11, 16.
Rabin, D.: 1997, Solar Phys. 174, 281.
Sakai, J.-I. and Ohsava, Y.: 1987, Space Sci. Rev. 46, 113.
Tsuneta, S.: 1996, Astrophys. J. 456, 840.
Tsytovich, V. N.: 1971, Nonlinear Effects in Plasma, Plenum, New York.
Tsytovich, V. N.: 1977, Theory of Turbulent Plasma, Consultant Bureau, New York.
Wang, D. Y. and Li, D. Y.: 1991, Solar Phys. 135, 393.
Wang, D. Y., Li, D. Y., Fu, Q. J., and Xia, Z. G.: 1997, Solar Phys. 246, 129.
Wentzel, D. and Aschwanden, M. J.: 1991, Astrophys. J. 372, 688.
Wu, C. S.: 1985, Space Sci. Rev. 41, 215.
Yokoyama, T. and Shibata, K.: 1996, Publ. Astron. Soc. Japan 48, 353.
Zheleznyakov, V. V.: 1970 Radio emission of the Sun and Planets, Nauka, Moscow.
Zheleznyakov, V. V. and Zaitsev, V. V.: 1975, Astron. Astrophys. 39, 107.
Zheleznyakov, V. V. and Zlotnik, E. Ya.: 1988, Sov. Astron. Lett. 14, 195.
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Chernov, G., Fu, Q., Lao, D. et al. Ion-Sound Model of Microwave Spikes with Fast Shocks in the Reconnection Region. Solar Physics 201, 153–180 (2001). https://doi.org/10.1023/A:1010310210707
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DOI: https://doi.org/10.1023/A:1010310210707