Observed since 20 Oct, 20:25 UTC
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Calculate the flux of electrons or protons trapped in the Earth's radiation belt using the NASA AE8/AP8 model from IRBEM

This Python package calculates the estimated flux of electrons or protons trapped in the Earth's radiation belt. It is a Python wrapper for the NASA AE8/AP8 model in the IRBEM package. It provides an Astropy-friendly interface, allowing you to specify the location using Astropy coordinates, the time in Astropy time, and the energy using Astropy units. You can pass it a single time and location, or arrays of times and locations.
pip install aep8
>>> from astropy.coordinates import EarthLocation
>>> from astropy.time import Time
>>> from astropy import units as u
>>> import aep8
>>> loc = EarthLocation.from_geodetic(15 * u.deg, -45 * u.deg, 300 * u.km)
>>> time = Time('2025-01-01 18:37:22')
>>> energy = 10 * u.MeV
>>> aep8.model(solar='max', particle='p').integral_flux(loc, time, energy)
<Quantity 3.04495297 1 / (s cm2)>
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| Version | Published | Direct dependencies | Open version |
|---|---|---|---|
| 1.1.0 | 31 Jul 2026 | 1 |
This describes our collected data; it is not a security assessment.
Observed since 20 Oct, 20:25 UTC
No superseded metadata states collected. Unchanged observations do not create new revisions.
package:d106301df9b9bda69ba509c3c55e95cbef04a0269a9d238d4b79a6051b645244