EGU2020-5224, updated on 12 Jun 2020
https://doi.org/10.5194/egusphere-egu2020-5224
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

SOLSTICE: Space Weather Modeling Meets Machine Learning

Tamas Gombosi1 and the SOLSTICE Team*
Tamas Gombosi and the SOLSTICE Team
  • 1University of Michigan, CLaSP, Ann Arbor, United States of America
  • *A full list of authors appears at the end of the abstract

The last decade has truly witnessed the rise of the machine age. The enormous expansion of technology that can generate and manipulate massive amounts of information has transformed all aspects of society. Missions such as SDO and MMS, and numerical models such as the Space Weather Modeling Framework (SWMF) are now routinely generating terabytes of science data, far beyond what can be analyzed directly by humans. Fortunately, concurrent with this explosion in information has come the development of powerful capabilities, such as machine learning (ML) and artificial intelligence (AI), that can retrieve revolutionary new understanding and utility from the massive data sets. 

SOLSTICE (Solar Storms and Terrestrial Impacts Center) is a recently selected NASA/NSF DRIVE Center. It will serve as the vanguard for developing and applying ML methods, which will then raise the capabilities of the entire community. We will combine next generation ML technology with our world-leading numerical models and the exquisite data from the space missions to make breakthrough advances in Heliophysics understanding and space weather capabilities, and then transition our technology to the CCMC for the benefit of all.

We use ML to attack Grand Challenge Problems that cover the major aspects of space weather science: (i) use interpretable deep learning models, archived solar observations and high-performance physics-based simulations to identify the onset mechanism of solar flares and coronal mass ejections; and (ii) use high-cadence observations and physics-based feature learning to predict solar storms many hours before eruption, training time-to-event models to predict event times and flare magnitudes using innovative machine learning techniques.

SOLSTICE Team:

Yang Chen, David Fouhey, Tamas I. Gombosi, Natalia Ganushkina, Alfred Hero, Bart van der Holst, Zhenguang Huang, Justin Kasper, Enrico Landi, Mike Liemohn, Ward Manchester, Tuija Pulkkinen, James Raines, James Slavin, Igor Sokolov, Valerii Tenishev, Gabor Toth, Shasha Zou (U. Michigan); Monica Bobra, Todd Hoeksema, Yang Liu, Phil Scherrer (Stanford); Spiro Antiochos, Maria Kuznetsova, Peter Schuck (GSFC); Graham Barnes, KD Leka (NWRA); Mark Cheung, Meng Jin (LMSAL); Howard Singer (NOAA SWPC); Enrico Camporeale (CIRES); Dan Welling (UT Arlington), Michael Hesse (U. Bergen).

How to cite: Gombosi, T. and the SOLSTICE Team: SOLSTICE: Space Weather Modeling Meets Machine Learning, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-5224, https://doi.org/10.5194/egusphere-egu2020-5224, 2020