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1 Air Force Research Laboratory AE9, AP9, and SPM: New Features and Future Version Plans 30 June 2013 W. R. Johnston 1, T. P. O Brien 2, G. P. Ginet 3, C. J. Roth 4, R. A. Quinn 4, P. Whelan 4, S. L. Huston 4, and T. B. Guild 2 1 Air Force Research Laboratory, Integrity Service Excellence Space Vehicles Directorate, Kirtland AFB, NM 2 Aerospace Corporation 3 MIT Lincoln Laboratory 4 Atmospheric and Environmental Research, Inc. Distribution A. Approved for public release; distribution unlimited. 377ABW
2 Recent AE9/AP9 Improvements CmdLineAe9Ap9 Program Support more ShieldDose2 options Improved Linux compiler optimization settings Documented command-line options Multiple file limit resolved MJD conversion fixed Graphical User Interface Clarified labels & error messages Added more tooltip information Various GUI behavior fixes User s Guide Document Additional information provided for ShieldDose2 model parameters Legacy model advanced options Model performance tuning Orbit definition parameters Coordinate system details Modified Julian Date conversions New Utility Programs PlasmaIntegral Adjusts Plasma integral flux calculations (for non-gui runs) CoordsAe9Ap9 Calculates Adiabatic Invariant coordinates from satellite ephemeris 2 Distribution A. Approved for public release; distribution unlimited. 377ABW
3 Comparison of AE8/AP8 (legacy) models to external implementations Model Run Parameters Ax8 in CmdlineAe9Ap9, IRBEM and SPENVIS CRRES satellite orbit (GTO) Fixed Epoch & Shift SAA options on 28 Feb 2005 (arbitrary), 24 hours, Δt=120 sec Comparison Results Most model results nearly matching Different magnetic field models used Integral Flux results match Differential Flux results near match Differences due to calculation method ShieldDose2 results mostly match Slight offset due to Diff Flux differences Full report documents all findings 3 Distribution A. Approved for public release; distribution unlimited. 377ABW
4 Version 1.1 We recently identified an error affecting some cross calibrations in AE9 Incorrect data set version was used in CRRES to LANL-GEO cross calibration Result affects relative calibration of LANL-GEO/SOPA datasets, along with error estimates for LANL-GEO/SOPA, CRRES, and POLAR datasets Effect is likely small: GEO flux ~20% greater for E>1 MeV GEO flux ~20-50% less for E<0.5 MeV Plot illustrates estimated effect on GEO electron spectra Expected public release in July 2013 AE9 V1.1 est AE9 V Distribution A. Approved for public release; distribution unlimited. 377ABW
5 Version 1.2 New data set (first new data to be added): TacSat-4/CEASE proton data captures new observations of elevated 1-10 MeV protons Additional plasma data, TBD but likely THEMIS/ESA New electron templates Improvements for inner zone electrons and for >3 MeV spectra Feature improvements More options for orbit element input and coordinates Fix flux-to-fluence calculations to cover variable time steps supports optimizing time steps for shorter run times Allow selection of time period for calculation of fluence supports different time periods for different effects Mac OSX build Expected public release in January Distribution A. Approved for public release; distribution unlimited. 377ABW
6 Version 1.5 New data: Protons: Azur, Van Allen/MagEIS & REPT Electrons: DEMETER/IDP, Van Allen/MagEIS & REPT Plasma: SCATHA/SC8, AMPTE/CCE & CHEM New features Parallelization capability for runs on clusters needed to speed up long runs Pitch angle tool make internal pitch angle calculations accessible to users Expected public release in October 2014 International collaborators on board with new model name 6 Distribution A. Approved for public release; distribution unlimited. 377ABW
7 Version 2.0 Major feature changes: Standard solar cycle introduces a full solar cycle reanalysis as a flythrough option New module frameworks for e.g. plasma species correlations, SPM stitching with AE9/AP9, auroral electrons, additional coordinates for MLT variation in SPM AP9 improvements: solar cycle variation in LEO, east-west effect Improved algorithms for faster run times New data Van Allen/MagEIS & REPT protons and electrons PAMELA protons addresses high energy proton spectra Other international data sets: possibilities include Cluster/RAPID-IIMS, ESA SREMs, CORONAS, NINA, Akebono/EXOS-D, SAC-C, Jason2 Expected public release in December 2015 Subsequent releases will include new data DSX/SWx, ERG 7 Distribution A. Approved for public release; distribution unlimited. 377ABW
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