We study the interaction between a magnetic dipole mimicking the Gerasimovich magnetic anomaly on the lunar surface and the solar wind in a self-consistent 3-D quasi-neutral hybrid simulation where ions are modeled as particles and electrons as a charge-neutralizing fluid. Especially, we consider the origin of the recently observed electric potentials at lunar magnetic anomalies. An antimoonward Hall electric field forms in our simulation resulting in a potential difference of <300V on the lunar surface, in which the value is similar to observations. Since the hybrid model assumes charge neutrality, our results suggest that the electric potentials at lunar magnetic anomalies can be formed by decoupling of ion and electron motion even withou...
Abstract Kinetic simulations are used to examine the solar wind’s interaction with a 3 km wide regio...
International audienceA detailed understanding of the solar wind interac- tion with lunar magnetic a...
[1] The formation of electric potential over lunar magnetized regions is essential for understanding...
Times Cited: 1 Kallio, Esa/F-9410-2014 1We study the interaction between a magnetic dipole mimicking...
International audienceWe present the first three-dimensional fully kinetic and electromagnetic simul...
Using a two-dimensional hybrid simulation, we study the physics of the interaction of the solar wind...
International audienceA detailed understanding of the solar wind interaction with lunar magnetic ano...
International audienceWe present a general model of the solar wind interaction with a dipolar lunar ...
Unlike the Earth and Mercury, our Moon has no global magnetic field and is therefore not shielded fr...
AbstractWe present the results of the first local hybrid simulations (particle ions and fluid electr...
We present the first three-dimensional fully kinetic and electromagnetic simulations of the solar wi...
International audienceWe present three-dimensional fully kinetic and electromagnetic simulations of ...
International audienceWe present three-dimensional fully kinetic and electromagnetic simulations of ...
Abstract Kinetic simulations are used to examine the solar wind’s interaction with a 3 km wide regio...
International audienceA detailed understanding of the solar wind interac- tion with lunar magnetic a...
[1] The formation of electric potential over lunar magnetized regions is essential for understanding...
Times Cited: 1 Kallio, Esa/F-9410-2014 1We study the interaction between a magnetic dipole mimicking...
International audienceWe present the first three-dimensional fully kinetic and electromagnetic simul...
Using a two-dimensional hybrid simulation, we study the physics of the interaction of the solar wind...
International audienceA detailed understanding of the solar wind interaction with lunar magnetic ano...
International audienceWe present a general model of the solar wind interaction with a dipolar lunar ...
Unlike the Earth and Mercury, our Moon has no global magnetic field and is therefore not shielded fr...
AbstractWe present the results of the first local hybrid simulations (particle ions and fluid electr...
We present the first three-dimensional fully kinetic and electromagnetic simulations of the solar wi...
International audienceWe present three-dimensional fully kinetic and electromagnetic simulations of ...
International audienceWe present three-dimensional fully kinetic and electromagnetic simulations of ...
Abstract Kinetic simulations are used to examine the solar wind’s interaction with a 3 km wide regio...
International audienceA detailed understanding of the solar wind interac- tion with lunar magnetic a...
[1] The formation of electric potential over lunar magnetized regions is essential for understanding...