Information about your group/project:
    Name(s) and e-mail (s) (please list primary contact first)*:
    	    Mark Dierckxsens, Mark.Dierckxsens@aeronomie.be
	    	 Norma Crosby, Norma.Crosby@aeronomie.be
    Associated Institution/Project name/Group name*:
    	       Royal Belgian Institute for Space Aeronomie (BIRA-IASB), Space Physics Division, Space Weather Group
    Website url(s):
    	    http://www.comesep.eu/
		http://www.aeronomie.be/

Information about your method:
    Forecasting method name*: COMESEP SEPForecast > 10 MeV 
    Shorthand unique identifier for your method (methodname_version, e.g. ModelName_1 or ModelName_201201): sepforecast_10mev
    Short description*: Occurance probability for a >10 MeV proton event and expected strength following an M1 flare or stronger.
    Model Inputs*: X-ray peak flux (GOES), flare location (SDO/AIA 94, Solar Demon), CME width & velocity (SOHO/LASCO, Cactus), GLE observations (GLE ALert Plus)
    Model Outputs*:  Radiation storm scale (based on E>10 MeV integral proton energy peak flux), probability, event onset and length
    References:
    

Further Model Details:
    (1)* Is the forecast made continuously (e.g. probability for the next 24 hours, or a time series), or event-triggered (e.g. by a flare or CME).
    	 The forecast is event triggered (flares)
	     
    (2)* Is the forecast human generated, human generated but model-based, model-based, or other. 
    	 Model-based and automaticly generated after detection of a >= M1 flare and updated in case the other inputs are available later. 

    (3)* If model-based: is the model empirical, physics-based or both.
    	 empirical model for probability and scale, physics based for event onset and length (SPARX model)