|
|
Go to: |
MCGM (v.04)Magnetic Clouds Global ModelModel DescriptionTool for the analysis of magnetic clouds, based on a non-force-free magnetic topology. Fitting the main physical magnitudes, including those related to plasma behavior, one can obtain the parameters associated with the magnetic cloud axis orientation. Torus topology with circular cross-section with maximum variable radius along it. Model Figure(s) :Model Inputs DescriptionMagnetic Field, and Plasma data from CDAweb in requested periods. Magnetic Field components (RTN or GSE), Plasma Beta (Solar wind speed, Proton density, Temperature, Plasma Pressure). Model Outputs DescriptionGraphics for: • RTN or GSE and Total Magnetic Field components (intensity), • Solar Wind speed, • Proton density, • Temperature, • Pressure, • Plasma Beta (see attached examples) • Boundaries of the selected magnetic clouds for the studied phenomena From the fitting of the model the parameters obtained: • Longitudinal angle axis in ecliptic plane • Latitudinal angle axis over the ecliptic plane. • Closest distance of approach of the spacecraft trajectory to the MC • Helicity of the cloud. • Fitted Magnetic Field components Graphics superimposed with the prediction of the model Model CaveatsChange LogFitting of the Magnetic Field components. In a fore coming version the Plasma Pressure, Density Current and Electric Field will be implemented. Model Acknowledgement/Publication Policy (if any)Model Domains:SolarHeliosphere.Inner_Heliosphere Space Weather Impacts:Geomagnetically induced currents - GICs (electric power systems)Ionosphere variability (navigation, communications) Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality) Galactic cosmic rays - GCRs (human exploration, aviation safety, aerospace assets functionality) Phenomena :Solar_Magnetic_FieldCoronal_Mass_Ejections Solar_Energetic_Particles Ambient_Solar_Wind Interplanetary_Shocks Heliospheric_Current_Sheet Coronal_Mass_Ejections_Propagation Coronal_Mass_Ejection_Arrival Simulation Type(s):Physics-basedTemporal Dependence Possible? (whether the code results depend on physical time?)trueModel 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):onboardingCode Language:SigmaPlot 14.0 codeRegions (this is automatically mapped based on model domain):Heliosphere.InnerSun Contacts :Juan.Javier.Jiménez Cuenca, ModelContactAcknowledgement/Institution :Space Research Group at Alcalá UniversityRelevant Links :Solar Orbiter. Energetic Particle Detector. Alcalá University.: https://espada.uah.es/epd/index.phpPublications :Model Access Information :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 |
|