| |
 |
| Paper: |
Two Types of Spicules “Observed” in 3D Realistic Models |
| Volume: |
454, The 3rd Hinode Science Meeting |
| Page: |
133 |
| Authors: |
Martínez-Sykora, J. |
| Abstract: |
Realistic numerical 3D models of the outer solar atmosphere show two different kind of spicule-like phenomena, as also observed on the solar limb. The numerical models are calculated using the Oslo Staggered Code (OSC) to solve the full MHD
equations with non-grey and NLTE radiative transfer and thermal conduction along
the magnetic field lines. The two types of spicules arise as a natural result of the dynamical evolution in the models. We discuss the different properties of these two types of spicules, their differences from observed spicules and what needs to be improved in the models. |
|
|
|
|
|
