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Last Updated: 05/26/2022

Cosgrove-PF

Version: 2.0

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.

Figures

SampleOutput 1 for Cosgrove-PF 2.0SampleOutput2 for Cosgrove-PF 2.0

Inputs

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

Outputs

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

Domains

  • High Latitude Ionosphere / Auroral Region

Phenomena

  • Energy Flow into Ionosphere

Publications

Code

Code Languages: Matlab, IDL

Contacts

Publication Policy

In addition to any model-specific policy, please refer to the General Publication Policy.