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. Author manuscript; available in PMC: 2016 Sep 14.
Published in final edited form as: Astrophys J. 2014 Nov 4;796(1):41. doi: 10.1088/0004-637X/796/1/41

Fig. 18.

Fig. 18

Top panel: Comparison between the distribution of absolute velocities of meteors traveling through the radar beam predicted by ZoDy and those predicted to be detected by the radar using our approach. Bottom panel: Comparison between the distribution of meteors masses input by ZoDy and those predicted to be detected by the radar using our approach.