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ASAP (ASAP_1)

Automated Solar Activity Prediction

Model Description

ASAP is a system proposed to predict solar flares based on sunspots McIntosh classification, using SDO HMI Intensitygrams and Magnetograms images. 

Model Figure(s) :

Model Inputs Description


	
	
	
	

Model Outputs Description


	
	
	
	

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Solar

Space Weather Impacts:

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

Phenomena :

Simulation Type(s):

Empirical

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:


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

Sun

Contacts :

Rami.Qahwaji, ModelDeveloper
Omar.Ashamari, ModelDeveloper

Acknowledgement/Institution :

Relevant Links :

Publications :

Model Access Information :

Access URL: https://iswa.ccmc.gsfc.nasa.gov/IswaSystemWebApp/?layout=ASAP
Access URL Name: Continuous/RT Run (ISWA layout)
Repository ID: spase://CCMC/Repository/NASA/GSFC/CCMC
Availability: online
AccessRights: OPEN
Format: HTML
Encoding: None

Access URL: https://iswa.gsfc.nasa.gov/iswa_data_tree/model/solar/asap/
Access URL Name: Continuous/RT Run (ISWA data tree)
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