Approximations for the Electron Density in Meteor Trails
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Herlofsen (1947) has shown that an exact solution of the equations governing the evaporation of a meteor particle during its flight in the upper atmosphere can be obtained in the special case of a spherical meteor in an isothermal atmosphere. In terms of the number n of meteor atoms evaporated in unit length of trail, the electron density a is . (1)
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1968 ◽
Vol 34
(1)
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pp. 145-158
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1955 ◽
Vol 6
(1-6)
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pp. 133-140
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