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AGU: Geophysical Research Letters

 

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  • Planetology: Comets and Small Bodies: Plasma and MHD instabilities

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 14, NO. 2, PP. 107-110, 1987
doi:10.1029/GL014i002p00107

Stochastic acceleration of cometary ions by lower hybrid waves

B. Buti

Physical Research Laboratory, Ahmedabad‐380009, India

G. S. Lakhina

Indian Institute of Geomagnetism, Colaba, Bombay‐400005, India

The turbulence produced by lower hybrid waves, during interaction of solar wind with the cometary pick‐up ions, leads to stochastic acceleration of these ions. The resulting energies of the cometary ions, calculated on the assumption that the entire turbulent electric field is used up for accelerating particles, are much larger compared to the recently observed energies of water‐group ions in the vicinity of comets Halley as well as Giacobini‐Zinner. Accounting for the fact that only a fraction of the field would lead to acceleration and the rest to heating, lower hybrid waves seem to be a potential source for the observed energetic cometary ions.

Received 12 December 1986; accepted 15 January 1987; .

Citation: Buti, B., and G. S. Lakhina (1987), Stochastic acceleration of cometary ions by lower hybrid waves, Geophys. Res. Lett., 14(2), 107–110, doi:10.1029/GL014i002p00107.

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