Properties of meteoroids from forward scatter radio observations

dc.contributor.author	Lamy, H.
dc.date	2019
dc.date.accessioned	2023-07-10T12:33:51Z
dc.date.available	2023-07-10T12:33:51Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/11031
dc.description	This chapter presents a brief overview of the properties of meteoroids entering the Earth's atmosphere that can be obtained with forward scatter radio observations. The first part is a general introduction about radio meteor observations, based mostly on the extension of the classical work of Mc Kinley (1961) to forward scatter radio observations. The most important part of this chapter is devoted to BRAMS (Belgian RAdio Meteor Stations) network, which is introduced as a recent example of a system using radio forward scatter observations to study trail meteor echoes. Comparisons of BRAMS radio data with meteor optical observations are briefly envisaged at the end.
dc.language	eng
dc.publisher	IOP Publishing, Bristol, United Kingdom
dc.title	Properties of meteoroids from forward scatter radio observations
dc.type	Book chapter
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Hypersonic Meteoroid Entry Physics
dc.source.page	3-1 - 3-22
Orfeo.peerreviewed	Yes
dc.identifier.doi	10.1088/2053-2563/aae894ch3
dc.identifier.scopus
dc.source.editor	Colonna, G.
dc.source.editor	Capitelli, M.
dc.source.editor	Laricchiuta, A.