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- W2084312919 abstract "Conventional meteor radars, operating at wavelengths of around 5–15 m, are unable to detect high-altitude meteors due to the wavelength-dependent echo ceiling. It is suggested that the ‘missing mass’ in the 10−6–10−2 g range of interplanetary material is in fact a high-velocity component which is normally undetected since it ablates at high altitude. This contention is supported by previous work. In this paper we describe measurements of the heights of radio meteors (limiting magnitude about +7) at a wavelength of 150 m (frequency 2 MHz), for which the echo ceiling is above 140 km. The resultant true height distribution is found to peak at ~ 104 km, about 10 km above the peak found by conventional meteor radars. The majority of meteors are detected at or above this peak, and substantial numbers are seen right up to 140 km. It is therefore concluded that the ‘missing mass’, comprising the vast majority of the meteoric input to the atmosphere, ablates well above 100 km." @default.
- W2084312919 created "2016-06-24" @default.
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- W2084312919 date "1987-03-01" @default.
- W2084312919 modified "2023-10-02" @default.
- W2084312919 title "The height distribution of radio meteors: observations at 2 MHz" @default.
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- W2084312919 doi "https://doi.org/10.1016/0021-9169(87)90060-2" @default.
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