EUHFORIA: Conditions of the heliospheric wind and CMEs
Last modified at Apr 24th, 2023, 18:50 GMT
Description
Calculates the parameters of the solar wind in the heliosphere, obtained from the boundary conditions at a distance of 0.1 AU, with superposed CMEs defined by the user or uploaded from a database. Heliospheric characteristics are calculated along the ecliptic and meridional planes and for selected positions such as Earth, Mars, Mercury, Venus, and the STEREO-A spacecraft.
Capabilities
-
Solar wind speed in the heliosphere
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Cadence
- Every 120 minutes
- Vector Representation
- Co-ordinate System
- Units
-
Plasma number density in the heliosphere
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Cadence
- Every 120 minutes
- Units
-
Plasma number density at the selected position
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Units
-
Plasma thermal pressure at the selected position
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Units
-
Solar wind speed at the selected position
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Vector Representation
- Co-ordinate System
- Units
-
Magnetic field at the selected position
- Observed Property
- Dimensionality Instance
- Dimensionality Timeline
- Vector Representation
- Co-ordinate System
- Units
Processing Input Parameters
- Solar wind boundary
- Parameters of the steady-state heliospheric wind are derived from the solar wind boundary.
- Characteristics of CMEs
- Parameters of the heliospheric wind with superposed CMEs defined by the user or uploaded from a database are calculated.
Data Levels
Further Information and Resources
Resources
More Properties
| Property | Value |
|---|---|
| Algorithm | Not used |
| Software Reference | Not used |
| Editor | KU Leuven |
| Version | 1 |
| Created | Wednesday 19th Oct. 2022, 09:55 |
| Last Modified | Monday 24th April 2023, 18:50 |