A new perspective concerning the influence of the solar wind on the Jovian magnetosphere

By D. Southwood, M. Kivelson. 2001

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In Astronomy and Astrophysics

Citations in the corpus

Dynamical consequences of two modes of centrifugal instability in Jupiter's outer magnetosphere (2004, background): “Finally, as the outer portion of the plasmasheet moves inward, its rotation should speed up and it should become easier for the ionospheric torque to maintain rotation on a shortened flux tube [ Southwood and Kivelson, 2001; Cowley and Bunce, 2001].”
Space Weather: Terrestrial Perspective (2007, background): “In the terrestrial case, the interaction is dominated by the strong intrinsic quasidipolar magnetic field; this is also the case of the outer giant planets Jupiter, Saturn, Uranus and Neptune (Southwood and Kivelson, 2001).”
Jupiter's polar auroral emissions (2003, methodology): “We relate them to the theoretical frame described by Cowley et al. [2003] which was originally based on the observation of H3 + auroral infrared emissions [Stallard et al., 2001, 2003] in Jupiter’s northern hemisphere.”
Simultaneous Chandra X ray, Hubble Space Telescope Ultraviolet, and Ulysses Radio Observations of Jupiter's Aurora (2005, background): “This Birkeland current connects to radially outward currents in the middle magnetosphere where the plasma begins to depart from corotation [cf. Hill, 2001; Bunce and Cowley, 2001; Southwood and Kivelson, 2001; Cowley et al., 2003a, 2003b].”
Jupiter's polar ionospheric flows: Theoretical interpretation (2003, background): “…currents are then joined by field-aligned currents which flow outward from the ionosphere into the current sheet throughout this region, which have been suggested to be associated with the main oval auroras [Bunce and Cowley, 2001b; Cowley and Bunce, 2001; Hill, 2001; Southwood and Kivelson, 2001].”
Response of Jupiter's and Saturn's auroral activity to the solar wind (2009, background): “At Jupiter, the dense outward drifting plasma reaches a distance where corotation with the magnetic field can no longer be enforced, leading to strong currents in and out of the polar ionosphere and bright auroral emissions [Hill, 2001; Cowley and Bunce, 2001; Southwood and Kivelson, 2001].”
Jupiter's main auroral oval observed with HST-STIS (2003, background): “These measurements directly test the theoretical predictions [Cowley and Bunce, 2001, 2003a, 2003b; Southwood and Kivelson, 2001; Waite et al., 2001; Khurana, 2001] of the changes in auroral activity which are expected to accompany changes in the angular velocity of the equatorial plasma.”
Saturn's polar ionospheric flows and their relation to the main auroral oval (2003, unknown): “It has recently been proposed that Jupiter’s main auroral oval is formed in this way (Bunce and Cowley, 2001; Cowley and Bunce, 2001; Hill, 2001; Southwood and Kivelson, 2001), the angular momentum transfer being required by the equatorial radial outflow of sulphur and oxygen plasma from the Io…”