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Mojtaba Akhavan-Tafti

Research Interests:
>> Plasma instabilities, leading to the formation of magnetic discontinuities in the solar wind
>> 3D characteristics and temporal evolution of mesoscale solar wind structures
>> Solar wind-magnetosphere-ionosphere-thermosphere coupling during geomagnetic storms
>> Non-thermal emission by orbital debris

Activities:
>> Principal Investigator of Space Weather Investigation Frontier (SWIFT)
>> Institutional Principal Investigator of the Solar Wind Electrons Alphas and Protons (SWEAP) instrument aboard NASA’s flagship Parker Solar Probe
>> Co-Investigator of the Space Debris Identification and Tracking (SINTRA) project
>> Team member of the Global Dynamics Constellation (GDC) magnetometer instrument
>> Team member of the Sun Radio Interferometer Space Experiment (SunRISE) mission
>> Principal Investigator of SunRISE Ground Radio Lab, engaging 2,500 high school students nationwide in hands-on STEM activities to promote space sciences and engineering

Translational R&D:
>> 3D Photovoltaics for solar and power beaming applications
>> On-demand mobile electric vehicle charging service

An image of magnetic loops on the sun, captured by NASA's Solar Dynamics Observatory on July 18, 2012.

“Space Tornadoes” Could Cause Geomagnetic Storms

But these phenomena, spun off ejections from the Sun, aren’t easy to study.