Diffuse structure of some meteors at the beginning of their trajectories at classic heights

Author:

Kozak P.M.,

Publisher

National Academy of Sciences of Ukraine (Co. LTD Ukrinformnauka)

Subject

General Medicine

Reference37 articles.

1. 1.Kozak P. M., Kozak L. V. (2015) Method for photometry of low light level meteors and earth artificial satellites from observations of superisocon TV systems. Space Science and Technology. 21(1). 38-47. (In Ukrainian).

2. 2.Kozak P., Rozhilo O., Taranukha Ju. (2012) Kinematical parameters of the meteors from the results of the basic television observations during the period of the Autumn Equinox 2001. Bulletin of Taras Shevchenko National University of Kyiv. Astronomy. 49. 20-25. (In Ukrainian).

3. 3.Kozak P., Rozhilo O., Taranukha Ju., Kruchynenko V. G. (2011) Kinematical characteristics of September meteors from double-station TV observations in 2003. Space Science and Technology. 17(4). 53-64. (In Ukrainian).

4. 4.Levin B. Y. (1956) Physical Theory of Meteors and Meteor Matter in the Solar System, USSR Academy of Sciences, Moscow. (In Russian).

5. 5.Abe S., Borovička J., Spurný P., Koten P., Ceplecha Z., Tamagawa T., and Meteor Network Team in Japan. (2006) Earth-grazing fireball on March 29, 2006. European Planet. Sc. Cong. 2006, Berlin, Germany. 486.

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