|
|||||
|
|
Possibility of investigation of the microstreams and associations by the radiotomographic method |
|
| Authors: | O. I. Evdokimov T. K. Filimonova V. V. Sidorov Rasim Amer Ali |
| Affiliation: | (1) Engelhardt Astronomical Observatory, 422526 Kazan, Tatarstan, Russia;(2) Kazan State University, 420008 Kazan, Tatarstan, Russia;(3) University of Sebha, P.O.BOX 19758, Sebha, Libyan Arab Jamahiriya |
| Abstract: | This article contains the tomographic problem's solution of the radiants distribution study by the meteor radar data. It was received the distribution of meteors velocities for the parts of celestial sphere with angular dimensions 10° × 10° and 1° × 1°. Was shown that the angular dimensions of most of radiants are equal 1° – 3° and larger part of the sporadic background looks like a totality of microstreams. |
| Keywords: | meteor radiant meteor velocity radar goniometer |
| 本文献已被 SpringerLink 等数据库收录！ | |