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Cosgrove Poynting Flux


CCMC Services available for Cosgrove-PF
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Model Developer(s)
Russel B. Cosgrove
Center for Geospace Studies, SRI International, Menlo Park, California, USA

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

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

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

References and relevant publications

Russell B. Cosgrove et al., "Empirical model of Poynting flux derived from FAST data and a cusp signature", JGR 119 (1), 411-430, (2014), DOI: 10.1002/2013JA019105, http://onlinelibrary.wiley.com/doi/10.1002/2013JA019105/abstract

CCMC Contact(s)

301-286-9571

Developer Contact(s)

National Aeronautics and Space Administration Air Force Materiel Command Air Force Office of Scientific Research Air Force Research Laboratory Air Force Weather Agency NOAA Space Environment Center National Science Foundation Office of Naval Research

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