Implementation of the radar, lidar and passive optical remote sensing concepts for measuring space debris from an Earth orbiting platform was investigated. Each system was compared for their requirements on the host platform, their performance relative to the space debris measurement program and the estimated cost of developing each concept into a flight instrument. It is found that the radar and lidar systems offer the greatest versatility and accuracy since they control the direction, intensity and duration of the energy incident on the target object. The performance of the passive optical system is determined by the capability of the detector and by the baseline separation of the telescopes, which requires the use of an on-orbit deployment mechanism. The passive optical concept provides the largest total event rae, and includes significant detections of particle sizes greater than 10 cm to allow correlation with ground based observations of the larger particles. The event rate for the radar system is relatively constant with particle while the lidar system is slightly biased toward the smaller sizes. These event rate differences result from a combination of the debris flux size distribution and the variation of sensitive detection area with particle size for the three concepts.
In situ orbital debris experiment concepts
1985-03-01
Conference paper
No indication
English
In-Situ Detection of Micrometeoroids and Orbital Debris: The PIE Experiment on MIR
British Library Conference Proceedings | 2000
|In-Situ Detection of Micrometeoroids and Orbital Debris: The PIE Experiment on MIR
Online Contents | 2000
|Meteoroid and Orbital Debris Flight Experiment DTO 1118
British Library Conference Proceedings | 1998
|Meteoroid and orbital debris flight experiment DTO 1118
AIAA | 1998
|Online Contents | 1993