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![Page 1: 1 Solar Ultraviolet Imager (SUVI) Thematic Maps Proving Ground NOAA Satellite Science Week - Kansas City, Missouri - May 2012 S. M. Hill, J. Vickroy, R.](https://reader035.fdocuments.in/reader035/viewer/2022062719/56649ec95503460f94bd6e69/html5/thumbnails/1.jpg)
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Solar Ultraviolet Imager (SUVI)Thematic Maps Proving Ground
NOAA Satellite Science Week - Kansas City, Missouri - May 2012
S. M. Hill, J. Vickroy, R. Steenburgh
NOAA Space Weather Prediction Center (SWPC), Boulder, CO
E. J. RiglerUS Geological Survey
Golden, CO
• Background
• Development and Implementation
• Results and Planned Assessment
• Next Steps
J. DarnellNational Geophysical
Data CenterBoulder, CO
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Outline
• Background
• Development and Implementation
• Results and Planned Assessment
• Next Steps
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The Space Weather Domain
GOESOrbit
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Phenomena and Impacts
G-Scale: Geomagnetic Storms
S-Scale: Solar Radiation Storms
R-Scale: Radio Blackouts
NOAA Scale ImpactsSolar Phenomena
Flares
Coronal Holes
Active Regions
Filaments CMEs
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Forecaster Workflow and Tasking
• Scheduled– Synoptic Analysis Drawings– Coronal hole boundaries for
recurrent solar wind– Active regions for situational
awareness and flare probabilities
• Event-Driven– Flare location (2 min) for solar
radiation storms and radio blackouts
– CME source region for model initiation
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SUVI Image Interpretation
The Sun presents highly complex surface and atmospheric features that are currently interpreted by forecasters by subjective visual inspection.
GOES-R SUVI will provide six spectral channels in the EUV at rapid cadence.
The current approach can be time consuming and exhibit substantial forecaster-to-forecaster variability.
Image Credit: NASA SDO AIA
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Observation and Interpretation Challenges
• Coronal holes: Very low EUV radiance• Issue: LOS confusion with bright material
• Flares: Intense radiance & high temperatures• Issue: Scattering and saturation in major flares• Issue: Minor flares appear similar to active regions
• Filaments: Optically thick in some bands• Issue: Low radiance confusion with coronal holes
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Automated Classification and Retrieval Challenges
• Line-of-Sight Integration– Sun’s atmosphere (corona) is thick shell with very large
heliographic variations in surface conditions and scale height
– Mostly optically thin leads to integration along LOS• Broadband (SXI)
– Gives good qualitative separation of features due to greater contrast dependence on temperature in X-rays
– Mix of continuum and many lines makes quantitative retrievals difficult
• Narrowband (SUVI)– Very good for quantitative retreivals because of (mostly)
single line temperature dependencies– Contrast is lower at longer wavelengths
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Outline
• Background
• Development and Implementation
• Results and Planned Assessment
• Next Steps
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Algorithm Selection
• Physics-Based• Differential Emission Measure (DEM) Retrieval• Continuum of values do not necessarily simplify
forecaster interpretation• Models are not mature enough to ingest such data
Statistical• Multispectral Bayesian classification • Segments images in to a limited number of
meaningful classifications• Extensive heritage in terrestrial remote sensing • Forecaster training of algorithm ensures results are
aligned with traditional visual interpretation
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Proving Ground Plan
• Year 1 (6/11-5/12): Develop pseudo-operational system• Establish proxy data pipeline• Create framework to run algorithm• Develop decoder to display outputs on AWIPS2
• Year 2 (6/12-5/13): Evaluate system• Present in real-time to forecasters• Create software for more routine (re-)training of
algorithm• Retrain and modify algorithm accoring to
forecaster feedback
• Using AIA synoptic data at 3 min cadence.• Processed in pseudo-operational mode (no
24x7 support)• Will be presented in GRIB2 format and
displayed in NAWIPS• Forecaster evaluation will lead to further tuning
of algorithm classification statistics
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Algorithm/Program Description
• Code• Algorithm implemented in AWG standard
FORTRAN• Framework built in Python
• Data source• NASA Solar Dynamics Observer (SDO)
Atmospheric Imaging Array (AIA)• Synoptic real-time data set on 3-minute
cadence• 1024x1024 pixels, 2.5 arcsec sampling• Six spectral channels
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Outline
• Background
• Development and Implementation
• Results
• Next Steps
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SXI “Active Region” Image
Flare
Active Regions
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SXI “Coronal Structure” Image
Flare
Active Regions
Coronal Hole
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SUVI Proxy Tri-Color Image
Flare
Active Regions
Coronal Hole
Filaments
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SUVI Thematic Map
Flare
Active Regions
Coronal Hole
Filaments
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Outline
• Background
• Development and Implementation
• Results
• Next Steps
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Planned Improvements
• AWIPS 2 display to forecasters
• Broader training scenarios
• Additional contextual constraints
• Probability thresholds• Null identifications
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Data Diversity
• Incorporate additional, non-GOES spectral channels, e.g. H-alpha
• Study incorporation of ‘non-spectral’ data sets, e.g., magnetograms
• Study uses of temporal differences
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Downstream Products
• Planned• Coronal hole
boundaries• Flare location• Active region statistics
• Research• Temporal differences
for coronal dimmings and waves
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Summary
• SUVI Thematic Maps are ready for forecaster evaluation
• The Maps have been integrated into a prototype AWIPS 2 system
• Product provides guidance, forecaster is always in-the-loop
• Successful evaluation will lead to reduced forecaster workload and less variability
• A number of improvements are being considered