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MCGM (v.04)

Magnetic Clouds Global Model

Model Description

Tool 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 Description

Magnetic 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 Description

Graphics 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 Caveats


	
	
	
	

Change Log

Fitting 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:

Solar
Heliosphere.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_Field
Coronal_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-based

Temporal Dependence Possible? (whether the code results depend on physical time?)

true

Model is available at?

CCMC

Source code of the model is publicly available?

false

CCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):

onboarding

Code Language:

SigmaPlot 14.0 code

Regions (this is automatically mapped based on model domain):

Heliosphere.Inner
Sun

Contacts :

Juan.Javier.Jiménez Cuenca, ModelContact

Acknowledgement/Institution :

Space Research Group at Alcalá University

Relevant Links :

Solar Orbiter. Energetic Particle Detector. Alcalá University.: https://espada.uah.es/epd/index.php

Publications :

  • Hidalgo, M.A. et al., A new model for the topology of magnetics clouds in the solar wind, Solar Physics., 2000.
  • Cid, C., Hidalgo, M.A., Nieves-Chinchilla, T., Sequeiros, J. and Viñas, A.F., Plasma and magnetic field inside magnetic clouds: a global study. Solar Physics, 2002.
  • Hidalgo, M.A. et al., A non-force-free approach to the topology of magnetics clouds in the solar wind, J. Geophysical Res., 2002
  • Hidalgo, M.A., Nieves-Chinchilla, T. y Cid, C., Elliptical cross-section for the magnetic topology of magnetics clouds, Geophysical Res. Letters, 2002.
  • Hidalgo, M.A. et al., A study of the expansion and distortion of the cross-section of magnetic clouds in the interplanetary medium, J. Geophysical Res., 2003.
  • Hidalgo, M.A., Nieves-Chinchilla, T., A global magnetic topology model for magnetic clouds. I, The Astrophysical Journal, 2012.
  • Hidalgo, M.A., A global magnetic topology model for magnetic clouds. II, The Astrophysical Journal, 2013.
  • Hidalgo, M.A., A global magnetic topology model for magnetic clouds. III, The Astrophysical Journal, 2014
  • Hidalgo, M.A., A global magnetic topology model for magnetic clouds. IV, The Astrophysical Journal, 2016.
  • Carcaboso Morales, Fernando. Suprathermal and Energetic Electrons as Probes of Interplanetary Magnetic Field Topology. PhD Thesis. Alcalá University, 2021.
  • Model Access Information :

    Linked to Other Spase Resource(s) (example: another SimulationModel) :

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