IPIM : Ionosphere-Plasmasphere IRAP Model
Last modified at Oct 27th, 2022, 14:30 GMT
Description
This process describes the equations solved to provide the temporal evolution of the main thermodynamics parameters of the ionospheric plasma as a function of altitude along a magnetic field-line, for a given solar and geomagnetic activity.
Computation Components
Data Levels
Quality Assessment
Data Quality Flags
Further Information and Resources
Resources
Editor | University Toulouse III |
Version | 1 |
Created | Thursday 27th Oct. 2022, 14:30 |
Last Modified | Thursday 27th Oct. 2022, 14:30 |