Published September 11, 2020
| Version 1
Conference paper
Open
CME Acceleration as a Probe of the Coronal Magnetic Field
Creators
- 1. University of Colorado at Boulder
- 2. University of Graz
- 3. Northwest Research Associates
- 4. NASA Goddard Space Flight Center
Description
By 2050, we expect that CME models will accurately describe, and ideally predict, observed solar eruptions and the propagation of the CMEs through the corona. We describe some of the present known unknowns in observations and models that would need to be addressed in order to reach this goal. We also describe how we might prepare for some of the unknown unknowns that will surely become challenges.
Files
Mason 2020 Helio2050 White Paper on SunCET Science.pdf
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