Cosgrove Poynting Flux

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.

IONOSPHERE/THERMOSPHERE

Contributor(s)

Initial contribute: 2020-07-02

Authorship

:  
Center for Geospace Studies, SRI International, Menlo Park, California, USA
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Classification(s)

Application-focused categoriesNatural-perspectiveSpace-earth regions
Method-focused categoriesData-perspectiveGeostatistical analysis
Method-focused categoriesProcess-perspectivePhysical process calculation

Detailed Description

English {{currentDetailLanguage}} English

Quoted from: https://ccmc.gsfc.nasa.gov/models/modelinfo.php?model=Cosgrove-PF

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)
Lutz Rastaetter
301-286-9571

Developer Contact(s)
Russel Cosgrove

模型元数据

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Russel B. Cosgrove (2020). Cosgrove Poynting Flux, Model Item, OpenGMS, https://geomodeling.njnu.edu.cn/modelItem/845f87c5-67ba-4468-bf00-7934f728eb5f
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Contributor(s)

Initial contribute : 2020-07-02

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Authorship

:  
Center for Geospace Studies, SRI International, Menlo Park, California, USA
Is authorship not correct? Feed back

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