Accurately determining the spatial and energy characteristics of different auroral particle precipitation types has been a significant challenge in sp...

The energy coupling between the solar wind and magnetosphere and the internal dynamics within the tail of the magnetosphere have both been shown to be...

Within the Climate and Space Sciences and Engineering department at the University of Michigan, students have organized, facilitated, and led monthly ...

The energy distribution of auroral precipitation is strongly controlled by the processes that are occurring in the magnetosphere, and the deposition o...

Cross-campus discussion on graduate student inclusivity at the University of Michigan led to the creation of a professional development seminar for fi...

Solar wind entry into the magnetosphere occurs through several mechanisms. The magnetospheric plasma is thus formed by a combination of protons (H+), ...

We investigate the plasma transport process known as the interchange instability. Injections resulting from this process have been observed by the Cas...

Earth's geomagnetic field acts as an effective shield against solar space weather, essential for modern infrastructure and communications. Since the l...