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The detection of coronal mass ejections in the interplanetary medium using scintillation observations

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Abstract

Daily observations of scintillating radio sources obtained from July 2011 through June 2012 on the Big Scanning Antenna of the P.N. Lebedev Physical Institute at 111 MHz using a 16 beams system are analyzed. Variations in the observed scintillation indices are compared with data on solar X-ray flares and geomagnetic disturbances. Comparison of the observed scintillation indices on successive days enables the detection of most propagating disturbances associated with coronal events of class M5.0 and higher.

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Authors and Affiliations

  1. Pushchino Radio Astronomy Observatory, Astro Space Center, P.N. Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow region, Russia

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

Authors
  1. A. V. Glyantsev
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  2. S. A. Tyul’bashev
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  3. I. V. Chashei
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  4. V. I. Shishov
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Corresponding author

Correspondence to S. A. Tyul’bashev.

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Original Russian Text © A.V. Glyantsev, S.A. Tyul’bashev, I.V Chashei, V.I. Shishov, 2014, published in Astronomicheskii Zhurnal, 2014, Vol. 91, No. 9, pp. 713–719.

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Glyantsev, A.V., Tyul’bashev, S.A., Chashei, I.V. et al. The detection of coronal mass ejections in the interplanetary medium using scintillation observations. Astron. Rep. 58, 619–625 (2014). https://doi.org/10.1134/S1063772914090030

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  • DOI: https://doi.org/10.1134/S1063772914090030

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