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

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 energi...

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Détails bibliographiques
Publié dans:Geophysical research letters. - 1984. - 42(2015), 13 vom: 16. Juli, Seite 5125-5131
Auteur principal: Burch, J L (Auteur)
Autres auteurs: Cravens, T E, Llera, K, Goldstein, R, Mokashi, P, Tzou, C-Y, Broiles, T
Format: Article
Langue:English
Publié: 2015
Accès à la collection:Geophysical research letters
Sujets:Journal Article charge exchange comet solar wind
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Résumé: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
Description:Date Revised 25.03.2024
published: Print-Electronic
Citation Status PubMed-not-MEDLINE
ISSN:0094-8276