| Literature DB >> 11538486 |
Abstract
The principal ion in the ionosphere of Triton is N+. Energetic electrons of magnetospheric origin are the primary source of ionization, with a smaller contribution due to photoionization. To explain the topside plasma scale height, we postulate that N+ ions escape from Triton. The loss rate is 3.4 x 10(7) cm-2 s-1 or 7.9 x 10(24) ions s-1. Dissociative recombination of N2+ produces neutral exothermic fragments that can escape from Triton. The rate is estimated to be 8.6 x 10(6) N cm-2 s-1 or 2.0 x 10(24) atoms s-1. Implications for the magnetosphere of Neptune and Triton's evolution are discussed.Entities:
Keywords: NASA Discipline Exobiology; NASA Discipline Number 52-20; NASA Program Exobiology; Non-NASA Center
Mesh:
Substances:
Year: 1990 PMID: 11538486 DOI: 10.1029/gl017i010p01717
Source DB: PubMed Journal: Geophys Res Lett ISSN: 0094-8276 Impact factor: 4.720