Portal de Periódicos da CAPES

Saturn's Dusty Ionosphere

2019; Wiley; Volume: 124; Issue: 3 Linguagem: Inglês

10.1029/2018ja026154

2169-9402

M. Morooka, Jan‐Erik Wahlund, Lina Hadid, A. I. Eriksson, N. J. T. Edberg, E. Vigren, D. J. Andrews, A. M. Persoon, W. S. Kŭrth, D. A. Gurnett, W. M. Farrell, J. H. Waite, R. Perryman, M. E. Perry,

Laser-induced spectroscopy and plasma

Abstract Measurements of electrons and ions in Saturn's ionosphere down to 1,500‐km altitudes as well as the ring crossing region above the ionosphere obtained by the Langmuir probe onboard the Cassini spacecraft are presented. Five nearly identical deep ionosphere flybys during the Grand Finale orbits and the Final plunge orbit revealed a rapid increase in the plasma densities and discrepancies between the electrons and ions densities (N e and N i ) near the closest approach. The small N e / N i ratio indicates the presence of a dusty plasma, a plasma which charge carrier is dominated by negatively charged heavy particles. Comparison of the Langmuir probe obtained density with the light ion density obtained by the Ion and Neutral Mass Spectrometer confirmed the presence of heavy ions. An unexpected positive floating potential of the probe was also observed when N e / N i ≪ 1. This suggests that Saturn's ionosphere near the density peak is in a dusty plasma state consisting of negatively and positively charged heavy cluster ions. The electron temperature ( T e ) characteristics in the ionosphere are also investigated and unexpectedly high electron temperature value, up to 5000 K, has been observed below 2,500‐km altitude in a region where electron‐neutral collisions should be prominent. A well‐defined relationship between T e and N e /N i ratio was found, implying that the electron heating at low altitudes is related to the dusty plasma state of the ionosphere.