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Dayside/nightside asymmetry of ion densities and velocities in Saturn's inner magnetosphere
Author(s) -
Holmberg M. K. G.,
Wahlund J.E.,
Morooka M. W.
Publication year - 2014
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2014gl060229
Subject(s) - saturn , magnetosphere , asymmetry , physics , magnetosphere of saturn , ion , astrobiology , geophysics , astronomy , magnetopause , magnetic field , planet , quantum mechanics
We present Radio and Plasma Wave Science Langmuir probe measurements from 129 Cassini orbits, which show a day/night asymmetry in both ion density and ion velocity in the radial region 4–6 R S (1 R S = 60,268 km) from the center of Saturn. The ion densities n i vary from an average of ∼35 cm −3 around noon up to ∼70 cm −3 around midnight. The ion velocities v i , θ vary from ∼28–32 km/s at the lowest dayside values to ∼36–40 km/s at the highest nightside values. The day/night asymmetry is suggested to be due to the radiation pressure force acting on negatively charged nanometer‐sized dust of the E ring. This force will introduce an extra grain and ion drift component equivalent to the force of an additional electric field of 0.1–2 mV/m for 10–50 nm sized grains.