Last Updated: 01/30/2023

Cosgrove-PF

Version: 1.0

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 into the ionosphere altitude range (~ 1210 km) on magnetic coordinates.

Figures

Cosgrove-PF 1.0 Sample Output

Inputs

Solar wind Density (N in cm^-3), velocity V (in km/s), magnetic field By, Bz (in nT), AL index (auroral magnetic perturbation).

Outputs

Pattern of Poynting Flux distribution in auroral zone (> 50 degrees magnetic latitude), averaged over both hemispheres.

Domains

  • High Latitude Ionosphere / Auroral Region

Phenomena

  • Energy Flow into Ionosphere

Publications

Contacts

Publication Policy

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