IPIM : Ionosphere-Plasmasphere IRAP Model

Last modified on Oct 27th, 2022

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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

Computation_IPIM

Further Resources and Information

Resources

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Quality Assessment

Data Quality Flags: DQ4

Data Levels

Metadata Information

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