Fig. 1

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Beginning (blue symbols) and end (red symbols) heights of the photographic meteors as a function of the length of the atmospheric trajectory. Solid lines show linear dependencies of heights Hbeg and Hend on observed length of atmospheric trajectory, L, dashed lines show linear dependencies of heights HbegS and HendS observed by spectral photographic camera at station Churáňov (CS in Table 1) on the length observed by the CS camera. Our three video meteors are plotted by diamonds for comparison. Values of beginning and terminal heights of AMO meteors observed by CAMS (triangles) and terminal heights of Perseid meteors (green stars) are also shown for easy comparison.
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