Hostname: page-component-76fb5796d-r6qrq Total loading time: 0 Render date: 2024-04-25T11:50:22.271Z Has data issue: false hasContentIssue false
  • English
  • Français

Physical Driving Forces and Models of Coronal Responses (Invited Paper)

Published online by Cambridge University Press:  14 August 2015

S. I. Syrovatskii  and
B. V. Somov
S. I. Syrovatskii
Affiliation:
Lebedev Physical Institute, Academy of Sciences of the USSR, Moscow
B. V. Somov
Affiliation:
Lebedev Physical Institute, Academy of Sciences of the USSR, Moscow

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The reasons for nonstationary hydrodynamic flows in solar atmospere are reviewed. It is emphasized that a rapid local heating of corona or upper chromosphere can scarcely provide a very large mass of solar plasma ejections observed in corona and interplanetary space. We suggest that coronal transients and interplanetary ejections are produced by magnetic field evolving in solar atmosphere. Magnetic reconnection in current sheets can play essential role in this process. The suitable approximation of strong magnetic field is formulated. Some solutions of MHD equations in this approximation are demonstrated. Their applications to coronal conditions are discussed.

Type
Part VI. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Theoretical Considerations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 425 - 441
Copyright
Copyright © Reidel 1980 

References

Baum, P.J., Bratenahl, A., and Kamin, G.: 1978, Astrophys. J. 226, pp. 286–300.Google Scholar
Bobrova, N.A. and Syrovatskii, S.I.: 1979, Solar Phys. 61, pp. 379–387.Google Scholar
Brown, J.C.: 1973, Solar Phys. 31, pp. I43–I69.Google Scholar
Bulanov, S.V., Sasorov, P.V., and Syrovatskii, S.I.: 1977, Soviet Phys. (Letters) JETP 26, pp. 565–568.Google Scholar
Bulanov, S.V. and Sasorov, P.V.: I978, Fizika Plasmy 4, pp. 746–757.Google Scholar
Burnes, C.W. and Sturrock, P.A.: I972, Astrophys. J. I74, pp. 629–638.Google Scholar
Dryer, M.: I979, Invited Rev. Paper, Solar Wind 4 Conf. (Rosenbauer, H., Ed.), Springer-Verlag, Berlin, in press.Google Scholar
Dryer, M. and Maxwell, A.: I979, Astrophys. J., 23I, pp. 945–959.Google Scholar
Dryer, M., Smith, Z.K., Steinolfson, R.S., Mihalov, J.D., Wolfe, J.H., and Chao, J.K.: 1976a, Geophys. Res. 8I, pp. 465I–4660.Google Scholar
Dryer, M., Steinolfson, R. S., and Wu, S. T.: 1976b, Space Research XVI (Rycroft, M. J., Ed.), Akademie-Verlag, Berlin, pp. 685–691.Google Scholar
Dryer, M., Wu, S.T., Steinolfson, R.S., and Wilson, R.M.: I979, Astrophys. J. 227, pp. I059–I07I.Google Scholar
Heyvaerts, J., Priest, E.R., and Rust, D.M.: 1977, Astrophys. J. 2I6, pp. I23–I37.Google Scholar
Ivanov, L.N. and Platov, Yu.V.: I977, Solar Phys. 54, pp. 35–44.CrossRefGoogle Scholar
Jockers, K.: 1978, Solar Phys. 56, pp. 37–53.Google Scholar
Kirii, N.P., Markov, V.S., Syrovatskii, S.I., Frank, A.G., and Hodzgaev, A.Z.: I979, in ‘Flare processes in plasmas’, Lebedev Phys. Inst. Proc. 110, pp. I2I–I6I (in Russian).Google Scholar
Low, R.P. and Nakagawa, Y.: I972, Astrophys. J. I99, pp. 237–246.Google Scholar
Mahmudov, M.O., Nikolskii, G.M., and Zhugzhda, Yu.D.: I979, Solar Phys., in press.Google Scholar
Nakagawa, Y., Steinolfson, R.S., and Wu, S.T.: I976, Solar Phys. 47, pp. I93–203.Google Scholar
Nakagawa, Y., Wu, S.T., and Tandberg-Hanssen, E.: I975, Solar Phys. 4I, pp. 387–396.Google Scholar
Ostapenko, V.A.: I979, Soviet Astron. AJ, in press.Google Scholar
Pneuman, G.W.: I979, On reconnection driven coronal transients, (these priceedings).Google Scholar
Podgornii, A.I. and Syrovatskii, S.I.: I979, in ‘Flare processes in plasmas’, Lebedev Phys. Inst. Proc. 110, pp. 33–56 (in Russian).Google Scholar
Rust, D.M.: I978, Transient coronal holes and magnetic reconnection. Preprint AS&E-43I8.Google Scholar
Rust, D.M. and Hildner, E.: I976, Solar Phys. 48, pp. 38I–388.Google Scholar
Sermulina, B.Ja., Somov, B.V., Spektor, A.R., and Syrovatskii, S.I.: I979, Gasodynamics of impulsive heated solar plasma, (these proc.).Google Scholar
Shmeleva, O.P. and Syrovatskii, S.I.: I973, Solar Phys. 33, pp. 34I–362.Google Scholar
Somov, B.V.: I978, in ‘Solar cosmic rays’, Proc IX Leningrad Seminar on Space Phys., pp. I85–2I0 (in Russian).Google Scholar
Somov, B.V.: I979a, Bull. Acad. Sci. USSR, Phys. Series 43, No. 4 (Allerton press Inc., New York).Google Scholar
Somov, B.V., Spektor, A.R., and Syrovatskii, S.I.: I977, Bull. Acad. Sci. USSR, Phys. Series 4I, pp. 32–43.Google Scholar
Somov, B.V., Spektor, A.R., and Syrovatskii, S.I.: I979, in ‘Flare processes in plasmas’, Lebedev Phys. Inst. Proc. 110, pp. 73–94.Google Scholar
Somov, B.V.: I979b, in ‘Flare processes in plasmas’, Lebedev Phys. Inst. Proc. 110, pp. 57–72 (in Russian).Google Scholar
Somov, B.V. and Syrovatskii, S.I.: I972, Soviet Phys. JETP 34, pp. 992–997.Google Scholar
Somov, B.V. and Syrovatskii, S.I.: I974, in ‘Neutral current sheets in plasmas’, Lebedev Phys. Inst. Proc. 74, pp. I4–72 (in Russian).Google Scholar
Somov, B.V. and Syrovatskii, S.I.: I975, Bull. Acad. Sci. USSR, Phys. Series 39, pp. I09–III (Allerton Press Inc., New York).Google Scholar
Somov, B.V. and Syrovatskii, S.I.: I976, Soviet Phys. Uspekhi 19, pp. 813–835 (American Inst. Phys.).Google Scholar
Somov, B.V. and Syrovatskii, S.I.: I979, Magnetically driven motions in solar corona, (these proceedings).Google Scholar
Steinolfson, R.S., Wu, S.T., Dryer, M., and Tandberg-Hanssen, E.: I978, Astrophys. J. 225, pp. 259–274.Google Scholar
Steinolfson, R.S., Wu, S.T., Dryer, M., and Tandberg-Hanssen, E.: I979, Solar Wind 4 Conf. (Rosenbauer, H., Ed.), Springer-Verlag, Berlin, in press.Google Scholar
Svestka, Z.: I976, Solar Flares. D.Reidel Publ. Co., Dordrecht, Boston.Google Scholar
Sweet, P.A.: I958, in ‘Electromagnetic Phenomena in Cosmic Physics’, Proc. IAU Symp. No. 6, pp. I23–I32.Google Scholar
Syrovatskii, S.I.: I966, Soviet Astron. AJ I0, pp. 270–279.Google Scholar
Syrovatskii, S.I.: I969, Astrophys. Space Sci. 4, pp. 246–250.Google Scholar
Syrovatskii, S.I.: I971, Soviet Phys. JETP 60, pp. I727–I736.Google Scholar
Syrovatskii, S.I.: I976, Soviet Astron. (Letters) AJ 2.Google Scholar
Syrovatskii, S.I.: I977, Solar Phys. 53, p. 247.Google Scholar
Syrovatskii, S.I.: I978, Astrophys. Space Sci. 56, pp. 3–I2.CrossRefGoogle Scholar
Syrovatskii, S.I.: I979, Lebedev Phys. Inst. Preprint, in press.Google Scholar
Webb, D.F., Cheng, C.C., Dulk, G.A., Edberg, S.J., Matrin, S.F., McKenna-Lawlor, S., and McLean, D.J.: I978a, Preprint AS&E-4364.Google Scholar
Webb, D.F., McIntosh, P.S., Nolte, J.T., and Solodyna, C.V.: I978b, Solar Phys. 58, pp. 389–396.Google Scholar
Wu, S.T., Dryer, M., and Han, S.M.: I976, Solar Phys. 49, pp. I87–204.Google Scholar
Wu, S.T., Dryer, M., Nakagawa, Y., and Han, S.M.: I978, Astrophys. J. 2I9, pp. 324–335.Google Scholar
Zirin, H. and Tanaka, K.: I973, Solar Phys. 32, pp. I73–207.Google Scholar