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BRaVDA (1.9)

Burger Radius Variational Data Assimilation

Model Description

This is a variational data assimilation scheme applied to a solar wind propagation model.

Model Figure(s) :

Model Inputs Description


	
	
	
	

Model Outputs Description


	
	
	
	

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
High_Speed_Stream
Stream_Interaction_Regions

Simulation Type(s):

Data Assimilation

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?

true

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

resultOnly

Code Language:

Python

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

Heliosphere.Inner

Contacts :

Harriet.Turner, ModelContact

Acknowledgement/Institution :

SCENARIO (NERC)

Relevant Links :

Publications :

Model Access Information :

Access URL: https://zenodo.org/record/7892408#.ZFJ8o3bMK3A
Access URL Name: Public Repository
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) :

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Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement