This is a library of codes that allows running different models of the high latitude ionospheric electrodynamics.

Available auroral models:

• Feature Tracking of the Auroral (FTA): Requires AU and AL indices
• Fuller Rowell and Evans [1986]: Requires hemispheric power, which can be derived using the AE index.
• OVATION-Prime: Requires IMF and solar wind.
• OVATION-SME: Requires AE.

Available electric potential models:

• Weimer: Requires IMF and solar wind.
• Heppner-Maynard: Requires IMF and Kp.

Available file formats:

• Binary file from AMIE files.

Products that can be provided:

• High-latitude electric potential (in kV)
• Diffuse auroral electron total energy flux (in mW/m2 or ergs/cm2/s)
• Diffuse auroral electron average energy (in keV)
• Diffuse auroral ion total energy flux (in mW/m2 or ergs/cm2/s)
• Diffuse auroral ion average energy (in keV)
• Monoenergetic auroral electron total energy flux (in mW/m2 or ergs/cm2/s)
• Monoenergetic auroral electron average energy (in keV)
• Wave-driven auroral electron total energy flux (in mW/m2 or ergs/cm2/s)
• Wave-driven auroral electron average energy (in keV)
• Future: high-latitude field-aligned currents