Literature DB >> 11538486

Triton: topside ionosphere and nitrogen escape.

Y L Yung1, J R Lyons.   

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:

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Year:  1990        PMID: 11538486     DOI: 10.1029/gl017i010p01717

Source DB:  PubMed          Journal:  Geophys Res Lett        ISSN: 0094-8276            Impact factor:   4.720


  1 in total

1.  Atmospheric implications of the lack of H3+ detection at Neptune.

Authors:  L Moore; J I Moses; H Melin; T S Stallard; J O'Donoghue
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2020-11-09       Impact factor: 4.226

  1 in total

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