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  3. Charge exchange in cometary coma: Discovery of H- ions in the solar wind close to comet 67P/Churyumov-Gerasimenko

Charge exchange in cometary coma: Discovery of H- ions in the solar wind close to comet 67P/Churyumov-Gerasimenko

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DOI
10.7892/boris.81645
Publisher DOI
10.1002/2015gl064504
Abstract
As Rosetta was orbiting comet 67P/Churyumov-Gerasimenko, the Ion and Electron Sensor detected negative particles with angular distributions like those of the concurrently measured solar wind protons but with fluxes of only about 10% of the proton fluxes and energies of about 90% of the proton energies. Using well-known cross sections and energy-loss data, it is determined that the fluxes and energies of the negative particles are consistent with the production of H- ions in the solar wind by double charge exchange with molecules in the coma.
Date Issued
2015
Publication Type
Article
Subject(s)
500 Science > 530 Physics
Language(s)
en
Author(s)
Burch, J. L.
Cravens, T. E.
Llera, K.
Goldstein, R.
Mokashi, P.
Tzou, Chia-Yu  
Physikalisches Institut, Weltraumforschung und Planetologie (WP)  
Broiles, T.
Additional Credits
Physikalisches Institut, Weltraumforschung und Planetologie (WP)  
Journal
Geophysical Research Letters
Publisher
American Geophysical Union
ISSN
0094-8276
Access(Rights)
open.access
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