the geosynchronous hurricane observatory...bjorn lambrigtsen jet propulsion laboratory - california...

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Bjorn Lambrigtsen Jet Propulsion Laboratory - California Institute of Technology [email protected] Jet Propulsion Laboratory California Institute of Technology Pasadena, California www.nasa.gov This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology under a contract with the National Aeronautics and Space Administration. Copyright 2011 California Institute of Technology. Government sponsorship acknowledged The Geosynchronous Hurricane Observatory The Geosynchronous Hurricane Observatory Hurricanes & severe storms Warm core anomaly @ 55 GHz (continuously, in real time) Surface pressure anomaly = Intensity, intensification/weakening Radar-emulating reflectivity (continuous coverage of entire life cycle) Convective structure/shear, precipitation, microphysics Complete diurnal-cycle observations (< 15-minute time resolution) Model improvements Real-time atmospheric stability indices (including under full cloud cover) Severe storm warnings, tornado precursor detection AMV-inferred wind vectors (regardless of cloud cover) Improved general forecast accuracy Hurricane forecast initialization (accurate “bogus” location & structure) Improved hurricane forecasts Synergy Complements GEO IR sounders (cloud clearing) Complements LEO sounders (swath-gap & temporal-gap filling) Complements GEO imagers (resolution enhancement of MW) Technology National Aeronautics and Space Administration Principle of aperture synthesis Science Dissecting hurricanes: 3D internal structure Height resolved “R adar reflectivity” Use radar algorithms to derive Precipitation rate Ice water path Convective intensity Vertical structure Vertical slicing through hurricane Emily - July 17, 2005 EDOP HAMSR Nadir along-track view 2 km Scan swath view MW sounder Is equivalent to radar! Correlation between MW-sounder ΔTb and radar reflectivity exceeds 90% at all levels except near surface Inferred from HAMSR 3 km 4 km 5 km 6 km 7 km 8 km 9 km 10 km 11 km 12 km 13 km 14 km 15 km Data products Temperature sounding channels Water vapor sounding channels Physical basis of microwave sounding Absorption spectrum Weighting functions Simulated brightness temperature images (tropospheric temperature sounding channels) Mission plans Near-term GOES-R/S time frame Long-term GOES-U time frame Outdoor scene (far field) Indoor scene (near field) Proof-of-concept prototype demonstrated in 2005 Concept development First images Prototype NASAʼs investments in GeoSTAR are approaching $15M A GeoSTAR mission will meet key NOAA needs re. NWP & hurricanes Technology development 183-GHz LNAs Receiver modules Correlator & digitizer ASICs Antenna modules 0 2 4 6 8 10 12 14 16 18 150 160 170 180 190 Frequency [GHz] Gain [dB], Noise Figure [dB] 300 400 500 600 700 800 900 1000 1100 1200 Noise Temperature [K] Gain [dB] NF [dB] NT [K] New state of the art: order-of-magnitude improvement in NEDT Ultra compact, lightweight & low-power Aalias-rejecting, very high beam efficiency, feedhorn assemblies High-speed ultralow- power circuits Design innovation Multiple-row antenna design maximizes the antenna beam efficiency and radiometric sensitivity and makes it possible to synthesize non-gaussian antenna patterns to limit aliasing. This makes it possible to focus the imaging area on a small region of interest using a small number of large-diameter feedhorns The GeoSTAR team Bjorn Lambrigtsen/JPL - PI Todd Gaier/JPL - Task Manager Alan Tanner/JPL - System Pekka Kangaslahti/JPL - Receivers Boon Lim/JPL - Electronics Chris Ruf/U. Michigan - Correlators Linda Herrell/JPL - Mission Venture mission New NASA program a) Venture-M: Full mission b) Venture-I: Instrument only 4-5 years rapid development Venture-M AO in 2011, 2015, etc. Venture-I AO in 2011, 2012, 2013, etc. GeoSTAR/Venture mission Sensor: GeoSTAR Objective: Hurricanes/storms Funding: NASA + partners Satellite Hosted on commercial commsat Timeline Start: 2012 Launch: 2016 PATH mission Decadal-survey mission Recommended by NRC Third tier 5+ years development Third-tier missions not yet funded GeoSTAR/PATH mission Sensor: “Array radiometer” Objective: Hydrologic-cycle obs. Funding: NASA Satellite Dedicated S/C Timeline Start: 202X Launch: late 2020ʼs?

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Page 1: The Geosynchronous Hurricane Observatory...Bjorn Lambrigtsen Jet Propulsion Laboratory - California Institute of Technology lambrigtsen@jpl.nasa.gov Jet Propulsion Laboratory California

Bjorn LambrigtsenJet Propulsion Laboratory - California Institute of Technology

[email protected]

Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadena, Californiawww.nasa.gov This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology under a contract with the National Aeronautics and Space Administration. Copyright 2011 California Institute of Technology. Government sponsorship acknowledged

The Geosynchronous Hurricane ObservatoryThe Geosynchronous Hurricane Observatory

Hurricanes & severe storms Warm core anomaly @ 55 GHz (continuously, in real time)

⇒ Surface pressure anomaly = Intensity, intensification/weakening Radar-emulating reflectivity (continuous coverage of entire life cycle)

⇒ Convective structure/shear, precipitation, microphysics Complete diurnal-cycle observations (< 15-minute time resolution)

⇒ Model improvements Real-time atmospheric stability indices (including under full cloud cover)

⇒ Severe storm warnings, tornado precursor detection AMV-inferred wind vectors (regardless of cloud cover)

⇒ Improved general forecast accuracy Hurricane forecast initialization (accurate “bogus” location & structure)

⇒ Improved hurricane forecasts

Synergy Complements GEO IR sounders (cloud clearing) Complements LEO sounders (swath-gap & temporal-gap filling) Complements GEO imagers (resolution enhancement of MW)

Technology

National Aeronautics and Space Administration

Principle of aperture synthesis

Science

Dissecting hurricanes: 3D internal structure

Height resolved “R adar reflectivity” ⇒ Use radar algorithms to derive

• Precipitation rate• Ice water path• Convective intensity• Vertical structure

Vertical slicing through hurricane Emily - July 17, 2005

EDOP

HAMSR

Nadir along-track view

2 km

Scan swath view

MW sounderIs equivalent

to radar!

Correlation between MW-sounder ΔTb and radar reflectivity exceeds 90% at all levels except near surface

Inferredfrom

HAMSR

3 km

4 km

5 km

6 km

7 km

8 km

9 km

10 km

11 km

12 km13 km

14 km15 km

Data products

Temperaturesoundingchannels

Water vaporsoundingchannels

Physical basis of microwave sounding

Abs

orpt

ion

spec

trum

Wei

ghtin

g fu

nctio

ns

Simulated brightnesstemperature images(tropospheric temperaturesounding channels)

Mission plans

Near-termGOES-R/S time frame

Long-termGOES-U time frame

Outdoor scene (far field)

Indoor scene (near field)

Proof-of-concept prototypedemonstrated in 2005

Concept developmentFirst imagesPrototype

NASAʼs investmentsin GeoSTAR

are approaching $15M

A GeoSTAR mission willmeet key NOAA needsre. NWP & hurricanes

Technology development183-GHz LNAs Receiver modules Correlator & digitizer ASICs

Antenna modules

0

2

4

6

8

10

12

14

16

18

150 160 170 180 190

Frequency [GHz]

Gai

n [d

B],

Noi

se F

igur

e [d

B]

300

400

500

600

700

800

900

1000

1100

1200

Noi

se T

empe

ratu

re [K

]

Gain [dB]NF [dB]NT [K]

New state of the art:order-of-magnitude

improvement in NEDT

Ultra compact,lightweight & low-power

Aalias-rejecting, veryhigh beam efficiency,feedhorn assemblies

High-speed ultralow-power circuits

Design innovation

Multiple-row antenna design maximizes the antenna beam efficiency and radiometric sensitivity andmakes it possible to synthesize non-gaussian antenna patterns to limit aliasing. This makes it possible to

focus the imaging area on a small region of interest using a small number of large-diameter feedhornsThe GeoSTAR team

Bjorn Lambrigtsen/JPL - PITodd Gaier/JPL - Task Manager

Alan Tanner/JPL - SystemPekka Kangaslahti/JPL - Receivers

Boon Lim/JPL - ElectronicsChris Ruf/U. Michigan - Correlators

Linda Herrell/JPL - Mission

“Venture” missionNew NASA program

a) Venture-M: Full missionb) Venture-I: Instrument only4-5 years rapid developmentVenture-M AO in 2011, 2015, etc.Venture-I AO in 2011, 2012, 2013, etc.

GeoSTAR/Venture missionSensor: GeoSTARObjective: Hurricanes/stormsFunding: NASA + partners

SatelliteHosted on commercial commsat

TimelineStart: 2012Launch: 2016

“PATH” missionDecadal-survey mission

Recommended by NRCThird tier5+ years developmentThird-tier missions not yet funded

GeoSTAR/PATH missionSensor: “Array radiometer”Objective: Hydrologic-cycle obs.Funding: NASA

SatelliteDedicated S/C

TimelineStart: 202XLaunch: late 2020ʼs?