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Small-Scale Heat Localization with Blowup in the Magnetic-Tube Cross Section During a Solar Flare

  • I. Mathematical Modeling
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We investigate the solutions of the nonlinear heat equation with a volume heat source and thermal conductivity dependent on a negative power of temperature. Properties of self-similar solutions are examined. Structures with contracting half-width evolve in the LS-regime with blowup. Self-similar analysis shows that the system attains a self-similar regime. The nonlinear heat equation is applied to model fast heating of the plasma in flares forming in a magnetic tube cross section, when heat is propagated by plasma ions across the magnetic field. Microflares are described by localized structures evolving in LS-regime with blowup. They may form thin hot filaments stretched in the direction of the magnetic field. The modeling results are consistent with experimental observations.

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References

  1. B. S. Somov, Cosmic Plasma Physics, Kluwer, Dordrecht (2000).

    Book  Google Scholar 

  2. H. Alfven, Cosmic Plasma [Russian translation], Mir, Moscow (1983).

  3. V. V. Zaitsev and A. V. Stepanov, “Issues in the physics of solar activity,” UFN, 176, No. 3, 325–333 (2006).

    Article  Google Scholar 

  4. V. A. Kovalev and I. V. Kovalev, “Differential method for diagnosis of nonlinear regimes,” Nelineinyi Mir, 7, No. 12, 918–921 (2009).V. A. Kovalev and I. V. Kovalev, “Differential method for diagnosis of nonlinear regimes,” Nelineinyi Mir, 7, No. 12, 918–921 (2009).

  5. I. A. Bilenko and V. A. Kovalev, “Heating regimes during solar flares,” Pis’ma v AZh, 35, No. 11, 873–880 (2009).

    Google Scholar 

  6. V. A. Kovalev, I. G. Kostyuchenko, M. I. Savchenko, and Yu. E. Charikov, “Fast and slow regimes in the solar flare of 5 July 2009,” Dinamika Slozhnykh Sred, XXI Century, No. 3 (2015).

  7. A. A. Samarskii, V. A. Galaktionov, S. P. Kurdyumov, and A. P. Mikhailov, Blowup Regimes in Problems for Quasilinear Parabolic Equations [in Russian], Nauka, Moscow (1987).

    Google Scholar 

  8. V. A. Kovalev and B. V. Somov, “The role of collisions for particle acceleration in solar-flare magnetic traps,” Pis’ma v AZh, 29, No. 5, 465–472 (2003).

    Google Scholar 

  9. V. A. Kovalev, “A nonlinear heating source during a solar flare,” Nelineinyi Mir, 8, No. 11, 717–723 (2010).

    Google Scholar 

  10. M. V. Livshits, “Solar flares: observation results and gas-dynamic processes,” in: L. V. Zelenyi and I. S. Veselovskii (editors), Plasma Heliophysics [in Russian], Vol. I (2008), p. 60.

  11. V. A. Galaktinov, V. A. Dorodnitsyn, G. G. Elenin, S. P. Kurdyumov, and A. A. Samarskii, “Quasi-linear heat equation with a source: blowup, localization, symmetry, exact solutions, asymptotics, structures,” Itogi Nauki i Tkhniki, series: Current Issues in Mathematics [in Russian], VINITI, Moscow (1987), pp. 95-205.

  12. G. G. Malinetskii (editor), Blowup Regimes. The Evolution of an Idea [in Russian], Nauka, Moscow (1998).

  13. E. S. Kurkina, E. D. Kuretova, and V. A. Kovalev, “Formation of thermal structures with blowup during solar flares,” Computational Mathematics and Modeling, 26, No. 2, 144–155 (2015).

    Article  MathSciNet  Google Scholar 

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Correspondence to E. S. Kurkina.

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Translated from Prikladnaya Matematika i Informatika, No. 50, 2015, pp. 5–30.

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Kurkina, E.S., Troshchiev, Y.V., Kovalev, V.A. et al. Small-Scale Heat Localization with Blowup in the Magnetic-Tube Cross Section During a Solar Flare. Comput Math Model 27, 395–416 (2016). https://doi.org/10.1007/s10598-016-9330-5

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  • DOI: https://doi.org/10.1007/s10598-016-9330-5

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