Meteor Orbit Determinations with Multistatic Receivers Using the MU Radar

Details Meteor Orbit Determinations with Multistatic Receivers Using the MU Radar Meteor Orbit Determinations with Multistatic Receivers Using the MU Radar

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008em%26p..102..309f&link_type=abstract

Earth, Moon, and Planets, Volume 102, Issue 1-4, pp. 309-314

Physics

Meteor, Radar Observation

Scientific paper

The MU radar of RISH (Research Institute for Sustainable Humanosphere, Kyoto University), which is a MST radar (46.5 MHz, 1 MW peak power), has been successfully applied to meteor studies by using its very high versatility. The system has recently renewed with 25 channel digital receivers which significantly improved the sensitivity and precision of interferometer used in meteor observation. The transmission is now synchronized to GPS signals, and two external receiving sites with a ranging capability has additionally been operated in order to determine the trajectories and speeds of meteoroids.

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