Probabilistic models of the Jovian magnetopause and bow shock locations

By S. Joy, M. Kivelson, R. Walker, K. Khurana, C. Russell, T. Ogino. 2002

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View Paper: https://www.semanticscholar.org/paper/20135d7dac093a4e16b365486ca6e0243d937cd7

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In Astronomy and Astrophysics

Citations in the corpus

Mercury's magnetopause and bow shock from MESSENGER Magnetometer observations (2013, methodology): “[24] We also examined the magnetopause and bow shock positions in a probabilistic manner, by means of a method employed at Jupiter by Joy et al. [2002]. As described in section 2, for each crossing we identified an extended region in space within which the magnetopause or bow shock crossings occurre”
Flow of mass and energy in the magnetospheres of Jupiter and Saturn (2011, background): “[1993], Jurac and Richardson [2005], and Cassidy and Johnson [2010] for Saturn).”
Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure (2006, background): “observed in theoretical [Joy et al., 2002] and empirical [Huddleston et al.”
The Jovian Auroral Distributions Experiment (JADE) on the Juno Mission to Jupiter (2017, methodology): “Using measurements of the solar wind dynamic pressure measured by the Ulysses SWOOPS instrument (e.g., Bame et al. 1992) and the Joy et al. (2002) empirical functions, it is estimated that Juno will likely cross the bow shock and magnetopause 64 and 42 times (±9), respectively (Bagenal et al. 2013).”
MESSENGER observations of magnetopause structure and dynamics at Mercury (2013, background): “By comparison, the combination of solar wind dynamic pressure falling off as 1/r(2) with increasing Heliocentric distance r and stronger planetary dipole moments results in average magnetopause standoff distances of 75RJ (whereRJ is Jupiter’s radius) and 24 RS (where RS is Saturn’s radius) at Jupite”
Dynamical consequences of two modes of centrifugal instability in Jupiter's outer magnetosphere (2004, background): “The background of the figure represents the equatorial magnetosphere with the magnetopause and bow shock locations shown as broad curves to reflect typical ranges of their positions [Joy et al., 2002].”
Solar wind interaction with Jupiter's magnetosphere (2009, methodology): “The magnetopause boundary is determined by the Joy et al. [2002] magnetopause model for rarefied solar wind conditions.”
JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system (2013, background): “Depending on the solar wind dynamic pressure, the dayside magnetopause can be found anywhere from a distance of 45 RJ to 100 RJ (Joy et al., 2002).”