Tracing the origin of spicules in 3D radiative MHD models
Abstract
Are the flux emergence and ambipolar diffusion essential for the production of solar spicules? What is the role of vorticity and magnetic reconnection? Are RBEs and RREs traces of plasma flows? We try to give answers to these questions by analyzing 3D model of a solar plage.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2020
- Bibcode:
- 2020AGUFMSH004..07D
- Keywords:
-
- 7507 Chromosphere;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7509 Corona;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7524 Magnetic fields;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7546 Transition region;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY