The new version - CORHEL V5.0 differs from the previous versions principally in the inclusion of a version of MAS supporting a full thermodynamic energy equation, as well as the polytropic implementation in the previous version.
CORHEL is a software package that: (1) obtains and processes photospheric magnetograms; (2) runs the coronal model (either MAS or WSA); (3) processes the results to generate boundary conditions for the heliospheric code; and (4) runs the heliospheric model (either MAS or ENLIL).
Coronal base plasma temperature and density.
Radial magnetic field Br from synoptic magnetogram (Kitt Peak Observatory) for selected Carrington Rotation on solar surface, filtered for use in model.
Stationary state in spherical coordinates (r,p,t, or Radius, Long.,Lat.): -Solar coronal temperature T -Plasma Pressure P -Density N -Velocity V -Magnetic fields B
Model is time-dependant.
- Heliosphere / Inner Heliosphere
- Coronal Holes
- Coronal Mass Ejections
- Ambient Solar Wind
- Magnetic Connectivity
- High Speed Stream
- Stream Interaction Regions
- Heliospheric Current Sheet
- Coronal Mass Ejections Propagation
- Coronal Mass Ejection Arrival
In addition to any model-specific policy, please refer to the General Publication Policy.