solar image recognition workshop summary & conclusions
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Solar Image Recognition Workshop Summary & Conclusions. Bob Bentley UCL. Several spatial and temporal regimes. Small scale phenomena Small scale, restricted FOV, short lifetimes Bright points, transient brightenings, granules… Generally, analysis restricted to limited time intervals - PowerPoint PPT PresentationTRANSCRIPT
Solar Image Recognition WorkshopSummary & Conclusions
Bob Bentley
UCL
Several spatial and temporal regimes• Small scale phenomena
– Small scale, restricted FOV, short lifetimes• Bright points, transient brightenings, granules…
– Generally, analysis restricted to limited time intervals– Concern over coverage, etc. – hard to construct catalogs
• “Global” Phenomena– Medium/large scale, whole/extended sun, longer lifetimes – Typically described features
• Spots, filaments, CH, AR… – slow evolution• CMEs, filament eruptions… – rapid evolution
– Scope for coordinated effort to develop tools and catalogs
• Outriders– Poorly described, few observations… – Trans equatorial loops, sigmoids?, active regions?, others??
To coordinate things we need to:• Adopt understood/common way of preparing, correcting and enhancing
the data prior to recognition• Examine carefully whether techniques giving the same results
– Consider how to “normalize” results– Use different wavelengths to confirm/provide information
• Think about more formal definitions of features• Consider if we should create new indices
– Related in some way to existing indices
• Agree on ways of describing features in catalogs– Describe how data treated, etc…– Issues related to coordinates, etc. (helio, pixel…)– Must be able to handle annotation
• Magnetic field strength of spots; classification of spots and Ars• Barbs on filaments• Structure of CMEs and velocity• AR structure, etc… – ARM????
– EGSO discussion document on this and related issues out shortly
Other things…• Use of information
– Many techniques designed to recognize and classify features
– Some designed to detect change
– Both could be used for Space Weather if appropriate information is available
– Need to decide what we need
– Need discussion to ensure what is being derived is of use
• Folding things like ARM into the VO effort – QLK/Web service interface– Metadata, registry?? (JTM?)
Also…• Sharing Software
– Special branch for feature recognition in SSW• Related mainly to medium/ large scale features?
• What about software for very small scale features??
– Submission procedure – issues related to quality
• Next Solar Image Recognition Workshop??
Missing presentations
• Nicolas Fuller
• Benkhali, Ali
• Antoine, Jean-Pierre
• Laurent Jacques
• Portier-Fozzani, Fabrice
• Dudok de Wit