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Observations of the dust radial velocity field in the F-corona on March 29, 2006

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Abstract

The results of interferometer observations of the dust radial velocity field in the F-corona during the total solar eclipse of March 29, 2006, are presented. The observations were performed in the Mugalzhar settlement, Aqtobe region, Kazakhstan. The observation results indicated that the dust orbital motion is opposite to the planetary motion and is inclined at an angle of about 105° with respect to the ecliptic plane. It is assumed that the observed dust is genetically related to Kreutz comets falling on the Sun and registered with the SOHO spacecraft on March 28 and 31, 2006.

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Authors and Affiliations

  1. DTOO Fesenkov Astrophysical Institute, Observatory 23, Almaty, Kazakhstan

    L. I. Shestakova, B. I. Demchenko & F. K. Rspaev

  2. Laboratoire d’Astrophysique de Grenoble, UMR 5571, CNRS, Université Joseph-Fourier, BP 53X, Grenoble, CEDEX 09, France

    A. Chalabaev

Authors
  1. L. I. Shestakova
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  2. B. I. Demchenko
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  3. F. K. Rspaev
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  4. A. Chalabaev
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Original Russian Text © L.I. Shestakova, B.I. Demchenko, F.K. Rspaev, A. Chalabaev, 2011, published in Solnechno-Zemnaya Fizika, 2011, Vol. 17, pp. 46–48.

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Shestakova, L.I., Demchenko, B.I., Rspaev, F.K. et al. Observations of the dust radial velocity field in the F-corona on March 29, 2006. Geomagn. Aeron. 51, 1054–1057 (2011). https://doi.org/10.1134/S0016793211080287

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  • DOI: https://doi.org/10.1134/S0016793211080287

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