What is a Better Way for Data-based Solar Magnetohydrodynamic Simulations?

Authors: Satoshi Inoue (Center for Solar-Terrestrial Research, New Jersey Institute of Technology), Keiji Hayashi (George Mason University), Takahiro Miyoshi (Graduate School of Science, Hiroshima UniversityView More

Eruptive vs. confined solar flares: statistical comparison of their solar source properties

Authors: Maria D. Kazachenko (CU Boulder / NSO) What is the difference between confined and eruptive flares in terms of their physical properties at theView More

Emulating Coronal Field Models with Physics-Informed Neural Nets

Authors: Nathaniel H. Mathews (NASA GSFC), Barbara J. Thompson (NASA GSFC) Predicting the current or future state of the coronal magnetic field requires high-resolution modelsView More

PHP Code Snippets Powered By : XYZScripts.com
PAGE TOP