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Cosgrove-PF (1.0)Cosgrove Poynting FluxModel DescriptionStatistical 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 Figure(s) :Model Inputs DescriptionSolar wind Density (N in cm^-3), velocity V (in km/s), magnetic field By, Bz (in nT), AL index (auroral magnetic perturbation). Model Outputs DescriptionPattern of Poynting Flux distribution in auroral zone (> 50 degrees magnetic latitude), averaged over both hemispheres. Model CaveatsChange LogModel Acknowledgement/Publication Policy (if any)Model Domains:High_Latitude_Ionosphere/Auroral_RegionSpace Weather Impacts:Phenomena :Energy_Flow_into_IonosphereSimulation Type(s):EmpiricalTemporal Dependence Possible? (whether the code results depend on physical time?)falseModel is available at?CCMCSource code of the model is publicly available?falseCCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):productionCode Language:Regions (this is automatically mapped based on model domain):Earth.NearSurface.AuroralRegionContacts :Russell.Cosgrove, ModelDeveloperLutz.Rastaetter, ModelHostContact Acknowledgement/Institution :Relevant Links :Publications :Model Access Information :Access URL: https://ccmc.gsfc.nasa.gov/requests/IT/user_registration_stat.php?model=CosgrovePFAccess URL Name: Runs-on-Request Repository ID: spase://CCMC/Repository/NASA/GSFC/CCMC Availability: online AccessRights: OPEN Format: HTML Encoding: None 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 |