HAO Colloquium - Maria Kazachenko, NSO/U of Colorado/U of California

Data-driven Models of the Solar Corona Magnetic Fields: Present and Future

The advent of high-cadence, large-scale photospheric vector magnetic field and Doppler velocity measurements from the Solar Dynamics Observatory and progress in the computational techniques have facilitated development of the time-dependent data-driven models of the coronal magnetic fields. In this talk I will first review current state and challenges of these models. I will then describe recent progress of the Coronal Global Evolutionary Model (CGEM), a collaborative effort between UC Berkeley, Lockheed Martin and Stanford University that computes electric fields in the photosphere to drive a 3D non-potential model of the solar corona magnetic fields. Finally I will tell how DKIST observations would help to move these data-driven models forward.

Date and time: 
Wednesday, January 30, 2019 - 2:00pm to 3:00pm
Building: 
CG-1
Room: 
2126