Abstract
AbstractIonospheric outflow is driven by an ambipolar electric field induced due to the separation of electrons and ions in a gravitational field when equilibrium along a magnetic field line is lost. A model of ionospheric outflow at Saturn was developed using transport equations to estimate the number of charged particles that flow from the auroral regions into the magnetosphere. The model evaluates the outflow from 1,400 km in altitude above the 1 bar level, to 3 RS along the field line. The main ion constituents evaluated are R+ and . We consider the centrifugal force exerted on the particles due to a fast rotation rate, along with the effects of field‐aligned currents present in the auroral regions. The total number flux from both auroral regions is found to be 5.5–13.0×1027 s−1, which relates to a total mass source of 5.5–17.7 kg s−1. These values are on average an order of magnitude higher than expected without the additional effects of centrifugal force and field‐aligned currents. We find the ionospheric outflow rate to be comparable to the lower estimates of the mass loading rate from Enceladus and are in agreement with recent Cassini observations. This additional mass flux into the magnetosphere can substantially affect the dynamics and composition of the inner and middle magnetosphere of Saturn.
Highlights
Axford (1968) first theorised that the polar wind is a supersonic flow of charged particles from the ionosphere along open field lines at Earth
We find a range of total particle source rates, from 5.5×1027 to 1.3 × 1028 s−1 corresponding to a total mass source rate of 5.5 − 17.7 kg s−1
Using initial conditions appropriate for auroral and sub-auroral conditions, we find a range of total particle and mass source rates of the ionospheric outflow
Summary
Axford (1968) first theorised that the polar wind is a supersonic flow of charged particles from the ionosphere along open field lines at Earth. The polar wind at Earth is caused by an ambipolar electric field arising from the separation of ions and electrons due to gravity. This electric field accelerates the ions outward along the field lines to maintain quasi-neutrality. Hoffman (1970) used Explorer 31 satellite data to first observe H+. Earth’s polar wind is dominated by H+ and O+ ions, the lightest and dominant ionospheric constituents, respectively. The reader is directed to Yau et al (2007)
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