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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. 4.

Fig. 4

Distribution of measured meteor head-echo SNR (in percent of total) for all the meteors detected by the Arecibo Observatory during the 2002 campaign. The dash lines indicate that over 0.1 % of the detected meteors will have SNR above −10 dB and approximately 1 and 2 orders of magnitude lower percentages for SNR values of −20 and −30 respectively.