The Development of a Split-tail Heliosphere and the Role of Non-ideal Processes: A Comparison of the BU and Moscow Models

Global models of the heliosphere are critical tools used in the interpretation of heliospheric observations. There are several three-dimensional magnetohydrodynamic (MHD) heliospheric models that rely on different strategies and assumptions. Until now only one paper has compared global heliosphere m...

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Veröffentlicht in:	The Astrophysical journal 2021-12, Vol.923 (2), p.179
Hauptverfasser:	Kornbleuth, M., Opher, M., Baliukin, I., Gkioulidou, M., Richardson, J. D., Zank, G. P., Michael, A. T., Tóth, G., Tenishev, V., Izmodenov, V., Alexashov, D., Fuselier, S., Drake, J. F., Dialynas, K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Boundary conditions Fluid flow Heliopause Heliosheath Heliosphere Heliospheric models Interstellar magnetic fields Interstellar matter Interstellar medium Interstellar plasma Lobes Magnetic fields Magnetic reconnection Magnetohydrodynamical simulations Magnetohydrodynamics Mathematical models Neutral atoms North Pole Solar magnetic field Solar system Solar wind Termination shock
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