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Parameters of the turbulence of the interplanetary plasma derived from scintillation observations of the quasars 3C 48 and 3C 298 at the solar-activity maximum

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Abstract

An analysis of temporal spectra of interplanetary scintillations of the radio sources 3C 48 and 3C 298 observed at 111 MHz on the Big Scanning Antenna of the Lebedev Physical Institute at the maximum of the 24th solar-activity cycle is reported. The measured temporal spectra of the scintillations are used to estimate the velocity of the in homogeneities and the index of the spatial spectrum of the turbulence. The dependence of the spectral index of the turbulence on the solar-wind speed persists in periods of high solar activity, when the global spatial structure of the solar wind is strongly modulated by the activity cycle.

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References

  1. A. Hewish, P. E. Scott, and D. Wills, Nature 203, 1214 (1964).

    Article  ADS  Google Scholar 

  2. D. J. McComas, B. L. Barraclough, H. O. Funsten, J. T. Gosling, E. Santiago-Munoz, R. M. Skoug, B. E. Goldstein, M. Neugebauer, P. Riley, and A. Balogh, J. Geophys. Res.: Space Phys. 105, 10419 (2000).

    Article  ADS  Google Scholar 

  3. P. K. Manoharan, J. Geophys. Res.: Space Phys. 99, 23411 (1994).

    Article  ADS  Google Scholar 

  4. S. K. Glubokova, S. A. Tyul’bashev, I. V. Chashei, and V. I. Shishov, Astron. Rep. 57, 586 (2013).

    Article  ADS  Google Scholar 

  5. S. K. Glubokova, I. V. Chashei, S. A. Tyul’bashev, and V. I. Shishov, Adv. Astron. Space Phys. 3, 94 (2013).

    ADS  Google Scholar 

  6. S. M. Kutuzov, Yu. I. Azarenkov, I. A. Alekseev, V. V. Ivanova, V. A. Izvekova, V. M. Karpov, V. I. Kostromin, A. S. Kutuzov, and G. A. Latyshev, Tr. Fiz. Inst. Lebedeva RAN 229, 3 (2000).

    Google Scholar 

  7. Lockheed Martin Solar and Astrophysics Laboratory (LMSAL)-Science-Last Events-Solar Soft. http://www.lmsal.com/solarsoft/last_events/

  8. Real-time (Quicklook) Dst index. http://wdc.kugi.kyoto-u.ac.jp/dst_realtime/

  9. V. S. Artyukh and T. V. Smirnova, Sov. Astron. Lett. 15, 344 (1989).

    ADS  Google Scholar 

  10. A. Purvis, S. J. Tappin, W. G. Rees, A. Hewish, and P. J. Duffett-Smith, Mon. Not. R. Astron. Soc. 229, 589 (1987).

    Article  ADS  Google Scholar 

  11. V. S. Artyukh, S. A. Tyul’bashev, and P. A. Chernikov, Astron. Rep. 43, 1 (1999).

    ADS  Google Scholar 

  12. A. N. Kolmogorov, Dokl. Akad. Nauk SSSR 30, 9 (1941).

    Google Scholar 

  13. C. -Y. Tu and E. Marsch, Space Sci. Rev. 73, 1 (1995).

    Article  ADS  Google Scholar 

  14. S. Sridhar and P. Goldreich, Astrophys. J. 432, 612 (1994).

    Article  ADS  Google Scholar 

  15. P. Goldreich and S. Sridhar, Astrophys. J. 438, 763 (1995).

    Article  ADS  Google Scholar 

  16. A. A. Schekochichin, S. C. Cowley, W. Dorland, G. W. Hammett, G. G. Howes, E. Quataert, and T. Tatsuno, Astrophys. J. Suppl. Ser. 182, 310 (2009).

    Article  ADS  Google Scholar 

  17. R. S. Iroshnikov, Sov. Astron. 7, 566 (1963).

    ADS  MathSciNet  Google Scholar 

  18. D. H. Kraichnan, Phys. Fluids 8, 1385 (1965).

    Article  ADS  MathSciNet  Google Scholar 

  19. I. V. Chashei and V. I. Shishov, Geomagn. Aeron. 17, 984 (1977).

    ADS  Google Scholar 

  20. I. V. Chashei and V. I. Shishov, Geomagn. Aeron. 25, 1 (1985).

    ADS  Google Scholar 

  21. S. Boldyrev, Phys. Rev. Lett. 96, 5002 (2006).

    Article  Google Scholar 

  22. J. K. Perez and S. Boldyrev, Astrophys. J. Lett. 672, L61 (2008).

    Article  ADS  Google Scholar 

  23. A. A. Ruzmaikin, J. Feynman, B. E. Goldstein, E. J. Smith, and A. Balogh, J. Geophys. Res.: Space Phys. 100, 3395 (1995).

    Article  ADS  Google Scholar 

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Authors and Affiliations

  1. Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow oblast, 142290, Russia

    S. K. Glubokova, A. V. Glyantsev, S. A. Tyul’bashev, I. V. Chashei & V. I. Shishov

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  1. S. K. Glubokova
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  2. A. V. Glyantsev
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  3. S. A. Tyul’bashev
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  4. I. V. Chashei
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  5. V. I. Shishov
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Correspondence to S. A. Tyul’bashev.

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Original Russian Text © S.K. Glubokova, A.V. Glyantsev, S.A. Tyul’bashev, I.V. Chashei, V.I. Shishov, 2015, published in Astronomicheskii Zhurnal, 2015, Vol. 92, No. 1, pp. 38–45.

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Glubokova, S.K., Glyantsev, A.V., Tyul’bashev, S.A. et al. Parameters of the turbulence of the interplanetary plasma derived from scintillation observations of the quasars 3C 48 and 3C 298 at the solar-activity maximum. Astron. Rep. 59, 33–39 (2015). https://doi.org/10.1134/S1063772915010035

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  • DOI: https://doi.org/10.1134/S1063772915010035

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