Add to ORKGA computational model was developed for the determination of the plasma and magnetic field properties of the global interaction of the solar wind with terrestrial planetary magneto/ionospheres. The theoretical method is based on an established single fluid, steady, dissipationless, magnetohydrodynamic continuum model, and is appropriate for the calculation of supersonic, super Alfvenic solar wind flow past terrestrial planets. A summary is provided of the important research results
An electrodynamic model for an ionosphere-solar wind interaction is developed based on the existence...
The overall objective of the proposed research was to use numerical solutions of the magnetohydrodyn...
International audienceThe study of the interaction of the solar wind with magnetized and unmagnetize...
A computational model for the determination of the detailed plasma and magnetic field properties of ...
The interaction of the solar wind with terrestrial planets can be predicted using a computer program...
The investigations undertaken in this report relate to studies of various solar wind interaction phe...
Computational procedures are developed and applied to the prediction of solar wind interaction with ...
The considerable variety of atmospheric and magnetic field properties possessed by the planets resul...
Problems in space physics are discussed whose models, in simplified form, reduce to a supersonic flo...
The development of a global, 3-D magnetohydrodynamic computational model is described. This model is...
Progress is reported in the development of a global, 3-D magnetohydrodynamic computational model to ...
The overall objective of this research program is to better understand the interaction of a magnetiz...
A bow wave was previously observed in the solar wind upstream of each of the first six planets. The ...
The results of the research related to solar winds are presented. Also included is a summary of pape...
Electrodynamic processes in the ionopause are examined as well as the structure of the induced magne...
An electrodynamic model for an ionosphere-solar wind interaction is developed based on the existence...
The overall objective of the proposed research was to use numerical solutions of the magnetohydrodyn...
International audienceThe study of the interaction of the solar wind with magnetized and unmagnetize...
A computational model for the determination of the detailed plasma and magnetic field properties of ...
The interaction of the solar wind with terrestrial planets can be predicted using a computer program...
The investigations undertaken in this report relate to studies of various solar wind interaction phe...
Computational procedures are developed and applied to the prediction of solar wind interaction with ...
The considerable variety of atmospheric and magnetic field properties possessed by the planets resul...
Problems in space physics are discussed whose models, in simplified form, reduce to a supersonic flo...
The development of a global, 3-D magnetohydrodynamic computational model is described. This model is...
Progress is reported in the development of a global, 3-D magnetohydrodynamic computational model to ...
The overall objective of this research program is to better understand the interaction of a magnetiz...
A bow wave was previously observed in the solar wind upstream of each of the first six planets. The ...
The results of the research related to solar winds are presented. Also included is a summary of pape...
Electrodynamic processes in the ionopause are examined as well as the structure of the induced magne...
An electrodynamic model for an ionosphere-solar wind interaction is developed based on the existence...
The overall objective of the proposed research was to use numerical solutions of the magnetohydrodyn...
International audienceThe study of the interaction of the solar wind with magnetized and unmagnetize...