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SSVT (v.1.0)

Suprathermal Spectrum Visualization Tool

Model Description

A visualization tool to aid modelers in examining the pre-event particle and plasma conditions at multiple 1 AU observers. The user decides on a mission and time frame of interest and, by examining the initial plots, determines a valid pre-event time window. The user can then produce a visualization of the observed and best-fitted energy spectrum during said time window that can be used as input to their model.

Model Figure(s) :

Model Inputs Description

Start and stop time for any time frame after 1998, flare info (optional), mission (ACE, Wind, STA and STB), element (H, He, O, Fe) 

Model Outputs Description

Particle, plasma, and magnetic field plots from each of the missions and their respective instruments for the duration of the input time frame (GOES XRAY and energetic particle data always appears). The locations of the different 1 AU missions with respect to the flare are also shown. After inspecting the plots, the user then decides on a valid pre-flare start and stop time for the appropriate missions. After inputting the pre-event time window, desired mission, fit type (roll-over spectra or power law), and desired suprathermal energies, the user will receive a second output - the energy spectrum for each desired mission during the period of interest. This pre-event spectrum can be used as a seed particle proxy, scaled by a proper radial power law (TBD / user-defined).

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Heliosphere.Inner_Heliosphere

Space Weather Impacts:

Solar energetic particles - SEPs (human exploration, aviation safety, aerospace assets functionality)

Phenomena :

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?

false

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

onboarding

Code Language:

Python

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

Heliosphere.Inner

Contacts :

Maher.A.Dayeh, ModelContact

Acknowledgement/Institution :

Relevant Links :

Publications :

Model Access Information :

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