Sunrise and range distribution of meteors

作者: V. Porubčan , A. Hajduk , G. Cevolani

DOI: 10.1007/BF02508591

关键词: Range (statistics)IonizationSunriseAntenna (radio)AstronomyEcho (computing)MeteoroidMeteor (satellite)Meteor showerPhysics

摘要: The influence of the sunrise effect on ionization meteor zone has been found from comparison echo range distributions obtained by radars at Springhill (120 000 echoes) and Budrio (7000 during activity Geminids shower. position maximum distribution corresponding to motion shower radiant was be shifted larger distances, as expected effect, independently different antenna systems two equipments.

参考文章(4)
Marsha R. Torr, D.G. Torr, R.A. Hoffman, W.B. Hanson, J.H. Hoffman, W.K. Peterson, J.C.G. Walker, An auroral F-region study using in situ measurements by the Atmosphere Explorer-C satellite Planetary and Space Science. ,vol. 23, pp. 1669- 1679 ,(1975) , 10.1016/0032-0633(75)90094-X
M. J. Neale, RADAR EQUIPMENT FOR CONTINUOUS METEOR OBSERVATIONS Canadian Journal of Physics. ,vol. 44, pp. 1021- 1028 ,(1966) , 10.1139/P66-085
DAVID W. HUGHES, W. J. BAGGALEY, Physical Sciences: Effect of Sunrise on the Meteor Region Nature. ,vol. 237, pp. 224- 226 ,(1972) , 10.1038/237224A0
T.F. Nicholson, L.M.G. Poole, The observed characteristics of radio-echoes from overdense meteor trains Planetary and Space Science. ,vol. 22, pp. 1669- 1689 ,(1974) , 10.1016/0032-0633(74)90109-3