Modes for Running AE9/AP9/SPM
AE9/AP9/SPM Contents
- AE9AP9 Home
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- Modes for running the model
- Recommended time sampling
- Known issues and limitations
- Versions (public releases)
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- Best Practices for Generating Space Environment Specifications with Modern Tools
- Radiation belt missions factsheet
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- AE9/AP9/SPM Team
- DSX
The AE9/AP9/SPM model suite introduces data-based statistics for estimates of the particle environment hazard, in contrast to legacy models which often provided estimates based only on a median environment state. AE9/AP9/SPM provides three mode options to variously access this capability:
- Mean
- using the mean flux maps with no variance statistics (analogous to most legacy models);
- Perturbed mean
-
run as scenarios with fluxes perturbed by uncertainties in measurements and in gap-filling/extrapolation results;
- Monte Carlo
- run as scenarios representing the perturbed mean uncertainties but with the addition of space weather variability (not available for SPM).
In perturbed mean and Monte Carlo modes, each scenario run is randomly initialized to provide one realization of the expected environment. Statistics compiled from multiple scenarios then yield estimates of the uncertainty of the environment.
Specification desired | Run mode | Duration | Combination of results |
---|---|---|---|
Total dose | Perturbed mean | several orbits or days | SPME + AE9, SPMH + AP9 + solar* |
Displacement damage (proton fluence) | Perturbed mean | several orbits or days | AP9 + solar* |
Proton SEE (proton worst case) | Monte Carlo | full mission | AP9 + solar* |
Internal charging (electron worst case) | Monte Carlo | full mission | AE9 |
The table above summarizes choices of AE9/AP9/SPM model runs suggested for typical specifications:
Note (*): solar particles are not currently included in AE9/AP9/SPM; a separate model must be used for estimates of solar protons, see e.g. M. A. Xapsos, P. M. O'Neill and T. P. O'Brien, “Near-Earth space radiation models,” IEEE Trans. Nucl. Sci., 60(3):1691-1705 (2013). [1]