2006
DOI: 10.1007/s11038-006-9098-2
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Study of a Bistatic Radar System Using VLBI Technologies for Detecting Space Debris and the Experimental Verification of its Validity

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Cited by 3 publications
(2 citation statements)
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“…In these operations, a large antenna transmits a tone to the target of interest, while the receiver antenna(s) observes the bounced echo. The technique has been successfully applied to determine the spin states of asteroids Busch et al (2010) and surveying the space debris with VLBI technology Yajima et al (2007); Montebugnoli et al (2010). In 2021, we have demonstrated the capability of the Hobart and Katherine 12-metre antennas for tracking the echo reflected by a large space vehicle.…”
Section: Bistatic Radarmentioning
confidence: 99%
“…In these operations, a large antenna transmits a tone to the target of interest, while the receiver antenna(s) observes the bounced echo. The technique has been successfully applied to determine the spin states of asteroids Busch et al (2010) and surveying the space debris with VLBI technology Yajima et al (2007); Montebugnoli et al (2010). In 2021, we have demonstrated the capability of the Hobart and Katherine 12-metre antennas for tracking the echo reflected by a large space vehicle.…”
Section: Bistatic Radarmentioning
confidence: 99%
“…Usually, the ground radar astronomical observations employ state-of-the-art ground large radio astronomical antennas, powerful radar transmitters, low-noise receivers, and high-speed data-acquisition computers [3]. Progressive updates of the NASA Goldstone and NSF (National Science Foundation) Arecibo systems, primarily by moving to higher frequencies and more powerful transmitters, have made these two compounds the dominant instruments for current radar studies of the solar system [4][5][6][7][8].…”
Section: Introductionmentioning
confidence: 99%