Abstract
Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects.
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References
Dryer, M., Andrews M. D., Aurass, H. and 21 coauthors: 1998, ‘The Solar Minimum Active Region 7978, its X2.6/1B Flare, CME, and Interplanetary Shock Propagation of 9 July 1996’, Solar Physics 181, 159–183.
Hori, K.: 1999, Study of Solar Decimetric Bursts with a Pair of Cutoff Frequencies, in Proceedings of the Nobeyama Symposium, NRO Report, 479, 267–271.
Hudson, H. S., Kosugi, T., Nitta, N. and Shimojo, M.: 2001, ‘Hard X-Radiation from a Fast Coronal Ejection’, Astrophys. J. 561, L211–L214.
Karlický, M.: 1992, Radio Emission of Eruptive Flares, in Z. Švestka, B. V. Jackson, and M. E. Machado (eds), Eruptive Solar Flares, Lecture Notes in Physics 399, pp. 171–176.
Karlický, M.: 1998, ‘Chromospheric Evaporation Shock and Reduced Optical Thickness Drifting in the 1-4.5 GHz Range’, Astron. Astrophysics 338, 1084–1088.
Karlický, M. and Odstrčil, D.: 1994, ‘The Generation of MHD Shock Waves during the Impulsive Phase of the February 27, 1992 Flare’, Solar Physics 155, 171–184.
Karlický, M., Yan, Y., Fu, Q. et al.: 2001, ‘Drifting Radio Bursts and Fine Structures in the 0.8-7.6 GHz Frequency Range observed in the NOAA 9077 AR (July 10-14, 2000) Solar Flares’, Astron. Astrophysics 369, 1104–1111.
Khan, J. I., Vilmer, N., Saint-Hilaire, P. and Benz, A. O.: 2002, ‘The Solar Coronal Origin of a Slowly Drifting Decimetric-Metric Pulsation Structure’, Astron. Astrophysics 388, 363–372.
Klassen, A., Aurass, H., Klein, K. L. et al.: 1999, ‘Radio Evidence of Shock Wave Formation in the Solar Corona’, Astron. Astrophysics 343, 287–296.
Kliem, B., Karlický, M. and Benz, A. O.: 2000, Solar Flare Radio Pulsations as a Signature of Dynamic Magnetic Reconnection. Astron. Astrophysics 360, 715–728.
Reiner, M. J. and Kaiser, M. L.: 1999, ‘High-frequency type II Radio Emissions Associated with Shocks driven by Coronal Mass Ejection’, JGR 104, 16979–16992.
Ohyama, M. and Shibata, K.: 1998, ‘X-ray Plasma Ejection Associated with an Impulsive Flare on 1992 October 5; Physical Conditions of X-ray Plasma Ejection’, Astrophys. J. 499, 934–944.
Švestka, Z., Jackson, B. V. and Machado, M. E.: 1992, Eruptive Solar Flares. Lecture Notes in Physics 399. Springer-Verlag, Berlin, Heidelberg.
Yokoyama, T. and Shibata, K.: 2001, ‘Magnetohydrodynamic Simulation of a Solar Flare with Chro-mospheric Evaporation Effect based on the Magnetic Reconnection Model’, Astrophys. J. 549, 1160–1174.
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© 2003 Springer Science+Business Media Dordrecht
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Karlický, M. (2003). High-Frequency Radio Signatures of Solar Eruptive Flares. In: Chian, A.CL., et al. Advances in Space Environment Research. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-1069-6_8
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DOI: https://doi.org/10.1007/978-94-007-1069-6_8
Publisher Name: Springer, Dordrecht
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