Вісник Астрономічної школи (Dec 2004)
Installation for radio observations of meteors
Abstract
Installation for radio observations of meteors assembled in astronomical study group of Kiev school number 59 is described. Its action is based on use of a method of registration of far (located on distance about 500–2000 km from the observer) FM-radio stations signals reflected by meteors’ ion trace. Results of radio observations on this installation of meteoric stream Geminids in 2003 are represented.