SPP seminar
Thursday 21 March 2019, 11:00am to 12:00pm
Venue
Physics C36Open to
Postgraduates, Public, Staff, UndergraduatesRegistration
Registration not required - just turn upEvent Details
Numerical modeling of the solar wind interaction with Mars based on multiple fluid MHD method
Due to the fact that the intrinsic magnetic field is absent on Mars, it is of importance to study the solar wind interaction with Mars and the consequent Martian outer space plasma environment. Our study aims on modeling the process of solar wind interaction with Mars by using a global multiple fluid method, in conjunction with the ionospheric ion chemical reactions and the induced magnetic equation. Several significant effects, including Hall effect, entire Mars rotation and crustal field on Mars, would be considered in the model.
Speaker
Haoyu Lu
School of Space and Environment at Beihang Univers
Contact Details
Name | Dr Maria Walach |