000003306 001__ 3306
000003306 005__ 20180118170608.0
000003306 037__ $$aCTALK-2017-0102
000003306 100__ $$aMartínez Picar, Antonio
000003306 245__ $$aUsing a small phased array for meteor observations
000003306 260__ $$c2017
000003306 269__ $$c2017-09-22
000003306 520__ $$aA prototype of a phased array of 8 elements is being built at the Humain Radio-Astronomy Station by the Royal Observatory of Belgium. The main goal of this instrument is monitoring the solar activity in the band of 20–80 MHz using Software De ned Radio receivers and employing beam- forming techniques to track the Sun. However, because the operation frequency of the BRAMS forward-scatter system lies within the frequency range of such an array, an appealing window of opportunity opens for meteor science as well. In this paper we explore the possibility of using the expected capabilities of the Small Phased Array Demonstrator to register radio meteor echoes.
000003306 536__ $$a2BRAIN_SPADE/$$c2BRAIN_SPADE/$$f2BRAIN_SPADE
000003306 594__ $$aNO
000003306 6531_ $$ameteors
000003306 6531_ $$aradio echo
000003306 6531_ $$aphase array
000003306 700__ $$aMarqué, Christophe
000003306 773__ $$tInternational Meteor Conference 2017 - Petnica, Serbia
000003306 8560_ $$fantonio.martinez@observatoire.be
000003306 85642 $$ahttp://imc2017.imo.net/
000003306 8564_ $$s7884234$$uhttp://publi2-as.oma.be/record/3306/files/IMC2017 martinez slides.pdf$$ySlides of IMC 2017 talk about SPADE and radio meteor observations
000003306 8564_ $$s7035$$uhttp://publi2-as.oma.be/record/3306/files/IMC2017 martinez slides.gif?subformat=icon$$xicon$$ySlides of IMC 2017 talk about SPADE and radio meteor observations
000003306 8564_ $$s9086$$uhttp://publi2-as.oma.be/record/3306/files/IMC2017 martinez slides.jpg?subformat=icon-180$$xicon-180$$ySlides of IMC 2017 talk about SPADE and radio meteor observations
000003306 906__ $$aContributed
000003306 980__ $$aCTALKCONT