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- W32041181 abstract "Small meteor particles are considered, which produce meteors with magnitudes between +3 m and +10 m to +12 m , and for which the thermal conductivity may be assumed infinite. Fragmentation and air cap effects are neglected. The derivation is made taking into account radiation losses and temperature variation during the evaporation time. The temperature variation of the meteoroid is defined in this case by the equation:" @default.
- W32041181 created "2016-06-24" @default.
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- W32041181 date "1968-01-01" @default.
- W32041181 modified "2023-10-18" @default.
- W32041181 title "16. Some aspects of the creation of meteor trains and radio-wave scattering from them" @default.
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- W32041181 doi "https://doi.org/10.1017/s0074180900019732" @default.
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