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Cosgrove-PF (2.0)

Cosgrove Poynting Flux

Model Description

Statistical model returning Poynting Flux (in W/m^2) energy flux into the ionosphere. The model was compiled using FAST satellite observations that are binned and mapped on magnetic coordinates.

Model Figure(s) :

Model Inputs Description

Solar wind Density (N in cm^-3), velocity V (in km/s), magnetic field Bx, By, Bz (in nT), Altitude (optional).

Model Outputs Description

Pattern of Poynting Flux distribution in auroral zone (> 50 degrees magnetic latitude), separate patterns for northern and southern hemisphere.

Model Caveats

Change Log

The updated model accounts for asymmetries between the northern and southern hemisphere and thus outputs different patterns for each hemisphere.

Model Acknowledgement/Publication Policy (if any)

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Space Weather Impacts:

Phenomena :

Simulation Type(s):

Temporal Dependence Possible? (whether the code results depend on physical time?)

Model is available at?

Source code of the model is publicly available?

CCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):

Code Language:

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Linked to Other Spase Resource(s) (example: another SimulationModel) :

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement