TY - JOUR
T1 - Electron Physics in 3-D Two-Fluid 10-Moment Modeling of Ganymede's Magnetosphere
AU - Wang, Liang
AU - Germaschewski, Kai
AU - Hakim, Ammar
AU - Dong, Chuanfei
AU - Raeder, Joachim
AU - Bhattacharjee, Amitava
N1 - Funding Information:
L. Wang, K. Germaschewski, and J. Raeder are supported by the NASA grant NNX13AK31G. L. Wang and K. Germaschewski are also supported by the DOE grant DESC0006670. A. Hakim and A. Bhattacharjee are supported by the NSF grant AGS-1338944. C. F. Dong is supported by the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by the University Corporation for Atmospheric Research. Computations were performed on Trillian, a Cray XE6m-200 supercomputer at UNH supported by the NSF MRI program under grant PHY-1229408. We thank J. C. Dorelli for providing the magnetic field data from Galileo observation shown in Figure and A. Glocer for useful discussion on implementation of inner boundary conditions. The simulation configuration file and output data can be obtained from (Wang et al.,).
Funding Information:
L. Wang, K. Germaschewski, and J. Raeder are supported by the NASA grant NNX13AK31G. L. Wang and K. Germaschewski are also supported by the DOE grant DESC0006670. A. Hakim and A. Bhattacharjee are supported by the NSF grant AGS-1338944. C. F. Dong is supported by the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by the University Corporation for Atmospheric Research. Computations were performed on Trillian, a Cray XE6m-200 supercomputer at UNH supported by the NSF MRI program under grant PHY-1229408. We thank J. C. Dorelli for providing the magnetic field data from Galileo observation shown in Figure 3 and A. Glocer for useful discussion on implementation of inner boundary conditions. The simulation configuration file and output data can be obtained from (Wang et al., 2016).
Publisher Copyright:
©2018. American Geophysical Union. All Rights Reserved.
PY - 2018/4
Y1 - 2018/4
N2 - We studied the role of electron physics in 3-D two-fluid 10-moment simulation of Ganymede's magnetosphere. The model captures nonideal physics like the Hall effect, electron inertia, and anisotropic, nongyrotropic pressure effects. A series of analyses were carried out: (1) The resulting magnetic field topology and electron and ion convection patterns were investigated. The magnetic fields were shown to agree reasonably well with in situ measurements by the Galileo satellite. (2) The physics of collisionless magnetic reconnection were carefully examined in terms of the current sheet formation and decomposition of generalized Ohm's law. The importance of pressure anisotropy and nongyrotropy in supporting the reconnection electric field is confirmed. (3) We compared surface “brightness” morphology, represented by surface electron and ion pressure contours, with oxygen emission observed by the Hubble Space Telescope. The correlation between the observed emission morphology and spatial variability in electron/ion pressure was demonstrated. Potential extension to multi-ion species in the context of Ganymede and other magnetospheric systems is also discussed.
AB - We studied the role of electron physics in 3-D two-fluid 10-moment simulation of Ganymede's magnetosphere. The model captures nonideal physics like the Hall effect, electron inertia, and anisotropic, nongyrotropic pressure effects. A series of analyses were carried out: (1) The resulting magnetic field topology and electron and ion convection patterns were investigated. The magnetic fields were shown to agree reasonably well with in situ measurements by the Galileo satellite. (2) The physics of collisionless magnetic reconnection were carefully examined in terms of the current sheet formation and decomposition of generalized Ohm's law. The importance of pressure anisotropy and nongyrotropy in supporting the reconnection electric field is confirmed. (3) We compared surface “brightness” morphology, represented by surface electron and ion pressure contours, with oxygen emission observed by the Hubble Space Telescope. The correlation between the observed emission morphology and spatial variability in electron/ion pressure was demonstrated. Potential extension to multi-ion species in the context of Ganymede and other magnetospheric systems is also discussed.
KW - Galileo
KW - Ganymede
KW - fluid simulation
KW - kinetic simulation
KW - magnetic reconnection
KW - magnetosphere simulation
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U2 - 10.1002/2017JA024761
DO - 10.1002/2017JA024761
M3 - Article
AN - SCOPUS:85047566711
SN - 2169-9402
VL - 123
SP - 2815
EP - 2830
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 4
ER -