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WindPredict (1)

Wind Predict with Alfvén Waves (WP-AW)

Model Description

3D MHD coronal model for solar wind with Alfvén-wave heating based on the PLUTO code.

Model Figure(s) :

Model Inputs Description

GONG mrmqs synoptic map of CR2075, CR2077, CR2231, projected on the first 15 modes of the spherical harmonics.

Model Outputs Description

Binary files with main physical quantities (velocity, magnetic field, density, pressure).

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Heliosphere.Inner_Heliosphere

Space Weather Impacts:

Near-earth radiation and plasma environment (aerospace assets functionality)

Phenomena :

Ambient_Solar_Wind
Magnetic_Connectivity
High_Speed_Stream
Heliospheric_Current_Sheet

Simulation Type(s):

Physics-based
Physics-based.MHD

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

false

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):

resultOnly

Code Language:

C

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

Heliosphere.Inner

Contacts :

Barbara.Perri, ModelContact

Acknowledgement/Institution :

Relevant Links :

Publications :

  • The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 data.
  • Adding a transition region in global MHD models of the solar corona, 2021sf2a.conf..230R (Bibcode from ADS)
  • Validation of a Wave Heated 3D MHD Coronal-wind Model using Polarized Brightness and EUV Observations
  • Flux rope and dynamics of the heliospheric current sheet Study of the Parker Solar Probe and Solar Orbiter conjunction of June 2020
  • Model Access Information :

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

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