Skip to main content

Monitoring the near-space meteoroid population using the AMOR Radar Facility

Baggaley, Jack 1, Galligan, David1
Affiliation data not available1

Document details

Publishing year2001 PublisherESA Publishing typeConference Name of conference3rd European Conference on Space Debris
Pagesn/a Volume
3
Issue
1
Editors
H. Lacoste

Abstract

The heliocentric orbital distribution of Earth-impacting meteoroids is provided via routine surveillance using the radar monitoring system Advanced Meteor Orbit Radar (AMOR). This orbital description of the Solar System dust population provides the speed and directional characteristics of the influx of this external dust into the Earth's environment. Details of this high-speed background dust component are important inputs for assessing the multiple contributions to the space debris population.

Preview