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1HS3 Science Team Meeting - BWI - October 19-20, 2010 HAMSR/Lambrigtsen
HAMSR Status Update (2015)
Bjorn Lambrigtsen (HAMSR PI)Shannon Brown (HAMSR Task Mgr)
– Plots placed as overlays over North America– Allows visualization of full dataset avoiding problem of
track overlays in swath display• TC center positions and times for each eye
overpass added as placemarks– HAMSR operator records TC center coordinates after
each eye overpass using real-time imagery– KML file generated with TC center locations for each
pass– Clicking on placemark provides pop-up display with
plots and text information for that overpass
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Swath data along flight path
75km storm relative gridded image
350km storm relative gridded image
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
TC center locations for each eye overpass
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Clicking on placemark brings up gridded images for that overpass
55.5 GHz TB, 8 km and 12 km reflectivity shown in this example
Information about overpass shown as text
•Time, Lat, Lon
•54.94 [250mb] and 55.5 [150mb] TB anomaly
•Experimental minimum central pressure derived from warm anomaly
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
All data within 30 minutes of overpass shown, so rapid overpasses will fill in 50km grid as shown in this Karl example
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Planned Products and Documentation
• User guide with full product descriptions will be distributed prior to science flightsPlanned products:– Window channel TB imagery (50.3, 113 and 166
GHz)– Total precipitable water and cloud liquid water
(non-precipitating conditions)– Upper air TB imagery (54.94 and 55.5 GHz and 118
GHz equivalent channels)– Derived Reflectivity (3-levels; e.g. 6, 8 and 12km)
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Processing System Upgrade
• Microwave Integrated Retrieval System - MIRS• Developed at NOAA NESDIS by Sid Boukabara’s group• MIRS is now NOAA’s primary MW retrieval system• CRTM has been adapted for HAMSR• MIRS implementation for HAMSR has not yet been done
• New system under development at JPL• Will include scattering Retrievals in the presence of rain• Optimal estimation methodology• Forward model: CRTM
• Also looking at RTTOV• Solver: Under development
• Evaluating solving in geophysical space vs. EOF space
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen
Instrument Status: Green
• Upgrade 50-GHz receiver• Using latest LNA/MMIC technology• Current receiver is perfectly adequate, but expect significantly
better sensitivity (noise performance) with the new receiver• We hope to get it done before 2014 campaign• Replacement transparent to users (but with better data)
• Ready to fly again!
Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, California
HS3 Science Team Meeting – Mountain View – May 5-7, 2015 HAMSR/Lambrigtsen