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Автор Haerendel, Gerhard
Дата выпуска 1986
dc.description The plasma flow in the cometary coma is described by a simple relation which results from the balance of magnetic stresses and drag forces, the latter being mainly due to ion mass loading. Inertial and pressure effects are not explicitly considered, but lumped into a correcting factor of order unity. The relation is used to infer the ionization rate due to the critical velocity effect. The limits, r<sub>crit</sub> and r<sub>lim</sub>, between which the effect dominates over photoionization are evaluated. Critical velocity ionization stabilizes the plasma flow speed at η<sup>−1/2</sup> v<sub>crit</sub>, where η is the overall efficiency of energy transfer to the ionizing electrons. This speed is estimated to be close to 20 km/s. At the outer limit, r<sub>lim</sub>, there is a strong rise of plasma density as seen from outside. Inside r<sub>crit</sub>, recombination and ion‐neutral friction come into play. The contact surface is found to be largely determined by ion‐neutral collisions. A second neutral component of the order of 10² cm<sup>−3</sup> is predicted to originate from recombination inside r<sub>lim</sub>. It is characterized by an antisunward flow with ∼ 20 km/s. Numerical values for the radial profile of n<sub>i</sub> and of the critical boundaries (except the bow shock) are given. The high plasma density found by ICE at the closest approach to comet Giacobini‐Zinner is interpreted as a result of the critical velocity effect.
Формат application.pdf
Копирайт Copyright 1986 by the American Geophysical Union.
Тема Comets
Тема Comets
Тема Comets
Тема Comets
Тема Comets I
Тема Planetary Sciences: Comets and Small Bodies
Тема Planetology: Comets and Small Bodies: Interactions with solar wind plasma and fields
Тема Space Plasma Physics
Тема Space Plasma Physics: Ionization processes
Название Plasma flow and critical velocity ionization in cometary comae
Тип article
DOI 10.1029/GL013i003p00255
Electronic ISSN 1944-8007
Print ISSN 0094-8276
Журнал Geophysical Research Letters
Том 13
Первая страница 255
Последняя страница 258
Аффилиация Haerendel, Gerhard; Max‐Planck‐Institut für Physik und Astrophysik, Institut für extraterrestrische Physik
Выпуск 3
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