Runs on Request (ROR) is a simulation service accessible to anyone
wishing to execute space science and space weather models hosted by
the CCMC.
Continuous/Real-time Run
Continuous/real-time runs are models that CCMC executes using near
real-time observation data as inputs. Post processed results of such
runs are sent to ISWA for display.
Instant Run
Simulation models that are available for instant execution and viewing
of results online via the Instant-Run web app.
Space Weather Analysis
ISWA
ISWA serves CCMC real-time/continuous model outputs and observational
data.
DONKI
DONKI is a comprehensive online database of space weather events for
the community.
Validation & Scoreboards
CAMEL
CAMEL is an integrated and flexible framework for comparing space
weather and space science model outputs with observational data sets.
ITMAP
ITMAP is a web application for interactive and comprehensive
evaluation of ionosphere and thermosphere (IT) models.
Flare Scoreboard
Real-time Forecasting Methods Validation for predicting Solar Flare
events.
CME Arrival Time Scoreboard
Real-time Forecasting Methods Validation for Coronal Mass Ejections
arrival time at Earth.
SEP Scoreboard
Real-time Forecasting Methods Validation for predicting Solar
Energetic Particle (SEP) events.
IMF Bz Scoreboard
Real-time Forecasting Methods Validation for interplanetary magnetic
field forecasts at L1.
Visualization & Analysis
Kamodo
Kamodo is a CCMC tool for access, interpolation, and visualization of
space weather models and data in python.
Kameleon
Kameleon is a software suite that is being developed at the CCMC to
address the difficulty in analyzing and disseminating the varying
output formats of space weather model data.
Flux Rope and CME measurements
StereoCAT
The Stereo CME Analysis Tool is an online tool enabling space weather
forecasters and researchers to quickly calculate CME kinematic
properties.
SWPC CAT Web
The web version of SWPC CME Analysis Tool enables users to calculate
CME kinematic properties.
EEG
EEG (Eruptive Event Generator) is a tool which uses observational data
to calculate the parameters needed for simulating the generation and
propagation of CMEs in the solar corona and inner heliosphere.