Solar Algorithms

Literature searches, descriptions, relevant routines and libraries, etc. Click on the algorithm name below for more information. The institute with the primary responsibility for each algorithm is included in the list below. Please see PhaseAAlgorithmRequirements for details on the deliverables expected for each algorithm by the end of Phase A, 30 September 2005. AlgorithmVOintegration is a description of how these algorithms will be made accessible through the Virtual Observatory. See SolarAlgorithms1111 for a formal document.

• ModeParametersAnalysis – Birmingham (primary), Sheffield (secondary)
• ModeAsymmetryAnalysis – Birmingham (primary), Sheffield (secondary)
• SubsurfaceFlowAnalysis - Sheffield
• PerturbationMapGeneration – Sheffield
• LocalHelioseismologyInversionWorkbench - Sheffield
• LoopRecognition - MSSL
• MagneticFieldExtrapolation - MSSL
• HelicityComputation - MSSL
• CmeDimmingRegionRecognition - RAL
• DemComputation - RAL
• SmallEventDetection – RAL
• SolarRotationProfiling (if time permits) - Sheffield
• OscillationSourcesAnalysis (if time permits) – Birmingham / Sheffield

Other algorithm links:

• AlgorithmTestData - list of test data used during algorithm development
• PhaseAAlgorithmDeliverables - list of individual algorithm deliverables for eSDO 1121

-- ElizabethAuden - 11 Jan 2005