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

Metadata Information
Editor University Toulouse III
Version 1
Created Thursday 27th Oct. 2022, 14:30
Last Modified Thursday 27th Oct. 2022, 14:30