GOES-R Field Campaign Preparation Frank Padula & Steve Goodman 2015 GLM Annual Science Team Meeting September 11, 2015.

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Presentation transcript:

GOES-R Field Campaign Preparation Frank Padula & Steve Goodman 2015 GLM Annual Science Team Meeting September 11, 2015

2 Outline Baseline Plan Summary Overview Campaign Objectives Image courtesy: Brian Hobbs (NASA ER-2 Program)

GOES-R Field Campaign Overview 3 The purpose of the GOES-R field campaign is to support post-launch validation of L1b & L2+ products: Advanced Baseline Imager (ABI) & Geostationary Lightning Mapper (GLM): −Planning ~6 week field campaign (~100 flight hours) with the high- altitude NASA ER-2 platform coordinated with ground based and near surface observations over several Earth targets −An official flight request has been submitted to the NASA ER-2 Program:  April – June 2017 GOES-R Spacecraft

GOES-R Field Campaign Overview 4 GOES-R Field Campaign Workshop – April 8-9, 2015: Established a baseline consensus of the GOES-R field campaign validation plan for L1b & L2+ products - Underflights to be collected, when possible, with low Earth orbit environmental satellites which may include S-NPP, Terra/Aqua, METOP, Landsat, ISS & GPM We invite participation in the field campaign We plan to have an open data access policy Two Phased Approach April – June 2017 Phase 1 (2 weeks)  ER-2 Based in Palmdale, CA (U.S. West Coast) Phase 2 (4 weeks)  ER-2 Based on the East Coast or Central U.S. » Warner Robins AFB, GA

NOAA Science Participation in All Phases of GOES-R Calibration Life-Cycle » GOES-R Calibration Working Group (CWG) has provided excellent support in the pre-launch calibration data analysis to verify the pre-launch instrument performance on behalf of NOAA over the past several years: – CWG has established an in-depth knowledge of the GOES-R instruments through extensive pre-launch support – Established a strong communication line between the CWG and Algorithm Working Group (AWG) as a result of GOES-R pre-launch activities » Understanding both CWG & AWG pre-launch performance concerns & waivers and post-launch validation limitations and challenges fosters a value added opportunity to develop comprehensive field campaign activities 5 GLM Performance Metrics: ABI Performance Metrics: Reflective Solar Bands (RSB) – 5 % radiometric uncertainty Thermal Emissive Bands (TEB) – 1 K radiometric uncertainty 70 % flash detection efficiency 5 % false alarm rate

Open Ocean Desert ER-2 Aircraft Coincident Collection GOES-R Instruments Ground Instruments, Systems & Support Teams Land/Vegetation ABI Field Campaign Approach: 10 km ~Tropopause 2 km Boundary Layer 20 km Stratosphere 10 m Near Surface Primary Objective: provide high-altitude validation of ABI L1b spectral radiance observations to validate SI traceability Secondary objective: provide surface and atmospheric geo-physical measurements to support L1b & L2+ product validation Targets of Interest: Clouds 6

ABI L1b & L2+ Validation Priorities Set of Priorities: Collect coincident & collocated high altitude airborne Hyper-Spectral Imagery (HSI), for all 16 ABI bands, with the same look angle as ABI over “uniform” Earth targets: Required Collection Set (no ground based obs.): − Desert & Water Minimum Collection Set (with ground based & near surface obs.): – Desert – Open Ocean ( ≥ 100 km off-shore) – Vegetation – over the Department of Energy (DOE) Atmospheric Radiation Measurement (ARM) Cloud And Radiation Testbed (CART) site  Other sites as available (i.e. SURFRAD sites, Chesapeake Bay, Great Lakes) Collect coincident & collocated high altitude airborne Lidar & Doppler Radar observations for validation of cloud and microphysical products: Minimum Collection Set for Clouds: – Mixed phase, Multi-layer, Clouds in low light conditions (i.e. terminator) Collect coastline data when possible for INR validation Collect pre-storm environment and convective events Collect U.S. East coast (or subset) 50 km on-shore & 50 km off-shore following frontal passage Collect clouds over snow (if available) Collect active fires (need <100m spatial resolution coincident with VIIRS) ABI Collection Priorities ABI Collections of Opportunity 7

ER-2 Aircraft Coincident Collection GOES-R Instruments GLM Field Campaign Approach: 10 km ~Tropopause 2 km Boundary Layer 20 km Stratosphere 10 m Near Surface Primary Objective: provide validation of GLM flash detection efficiency day through night over land at well characterized total lightning super sites: Northern AL, Lubbock TX, Norman OK, KSC FL, and Wallops/DC area Secondary Objective: provide validation of GLM flash detection efficiency day through night at other land locations and over ocean Tertiary Objective: provide validation of GLM flash location & time stamp accuracy, and GLM image navigation and registration (INR) accuracy Storms 8 Targets of Interest:

1)Validation of GLM flash detection efficiency: collect coincident and collocated high altitude data over thunderstorms with the Fly’s Eye GLM Simulator (FEGS*):  Minimum Collection Set: Over-flights of thunderstorms over total lightning super sites. Emphasis on large scale convection such as Mesoscale Convective Systems (MCSs) from pre-storm through entire evolution (include all times of day & other storm types)  Secondary Collection Set: Over-flights of thunderstorms at other locations (day / dawn or dusk/ night; high / low latitudes; land / ocean; various storm types / regimes) 2)Validation of GLM flash location & time-stamp accuracy, and INR 3)Validation of optical energy calibration for the GLM product (lightning, which consists of events, groups, and flashes) GLM Validation Priorities 9 Achievement Metrics Field campaign success improved by complying with the following:  Sample size on the order of 1000 flashes must be observed for any region and period of interest in order to characterize detection efficiency, and geo-location & time-stamp accuracy.  Generally full storm life-cycle is desired, so do not interrupt life cycle when possible.  More success is achieved by partially sampling multiple storm types (regime /region/time of day) rather than only fully sampling one or two types.

Value of the GOES-R Field Campaign GLM: » Provides independent persistent and flexible validation capability for: −Flash detection efficiency −Geo-location & time-stamp accuracy characterization −Optical energy calibration » Ability to collect full storm life-cycle » Greater flexibility to collect over multiple storm types at different times of day and geospatial regions » No current satellite observations for cross validation as TRMM ended its data collection on April 8, 2015 » The ISS Lightning Imager Sensor (LIS) instrument may be available for comparison (planned launch early 2016), but Airborne GLM Simulator guarantees an optical to optical cross comparison 10

Candidate Instruments AVIRISngNext-Generation Airborne Visible/Infrared Imaging Spectrometer S-HISScanning High-resolution Interferometer Sounder FEGS Fly’s Eye GLM Simulator LIPLightning Instrument Package CPLCloud Physics Lidar CRS94-GHz (W-band) Cloud Radar System (CRS) ABI & GLM combined campaign provides an opportunity for data collection with broad suite of instruments GOES-R Field Campaign Candidate Instruments InstrumentTypeSpectral RangeSpectral Res.GSDFOV Swath Width AVIRISngHSI380 – 2510 nm5 nm0.3 m to 20 m34 deg~11 km S-HISHSI µm0.5 cm km40 deg40 km FEGSPassive EOnear-infrared (777.4 nm)10 nm~10 km LIP Passive Electrical CPLLidar1064, 532, & 355 nm30x200 m CRSDoppler Radar 94 GHz (W-band; 3 mm wavelength) na 11 Minimum Set of Instruments Add-on Capability

GLM Field-Of-View 89.5 W: PLT & PLPT 12

ABI & GLM Validation 13 Circles are intended as visual guides for discussion purposes only Phase 1: Palmdale, CA ~ 2 weeks Phase 1: Palmdale, CA ~ 2 weeks Phase 2: East Coast ~4 weeks Phase 2: East Coast ~4 weeks NALMA – Huntsville, AL DCLMA – Washington DC OKLMA – Norman, OK WTLMA – Lubbock, TX KSCLMA – Kennedy Space Center, FL NMLMA – Socorro, NM HLMA – Houston, TX FCLMA – Ft. Collins, CO WILMA – Wallops Island, VA NGLMA – Atlanta, GA TLMA – Toronto, Canada List of LMA Sites: GLM LMA Sites ABI Cal/Val Sites

ER-2 Loiter Time (based on an 8 hr mission) Phase 1 & 2 14 Image courtesy: Brian Hobbs (NASA ER-2 Program)

Moving Forward 15 Rotary SystemsFixed-Wing Systems » Developing a campaign validation matrix » Refining field deployment plans and identifying collaborators » Enhancing our data management planning and developing a GOES-R field campaign portal » Strengthening our collaboration efforts to ensure mission success Mid/High-Altitude Systems Collaborating with the NOAA Unmanned Aircraft System (UAS) Program to develop an enduring NOAA/NESDIS operational validation capability: » GOES-R Funded a “Near Surface UAS Feasibility Demonstration Study” - NOAA Cooperative Institute Partnership with the University of Maryland (UMD) -- ABI Validation Focus » Potential opportunities for GLM UAS validation capabilities

Timeframe: April – June 2017 Duration: ~2 weeks Flight hours: ~20-30 hrs Summary: Focus is to achieve ABI primary validation objective (L1b) Opportunity for ABI Intensive ground campaign at WSMR Opportunity for GLM validation targets: – GLM LMAs within range: Socorro, NM Ft. Collins, CO Lubbock, TX Norman, OK Collections of opportunity for ABI & GLM 16 Phase 1 Summary: GOES-R Field Campaign ER-2 Loiter Time (based on an 8 hr mission)

Phase 2 Summary: GOES-R Field Campaign Timeframe: April – June 2017 Duration: ~4 weeks Flight hours: ~70-80 hrs Summary: Focus is to achieve GLM validation objectives and ABI secondary objectives GLM LMAs within range (dependent upon location of GOES-R): −Huntsville, AL −Washington, DC −Kennedy Space Center, FL −Houston, TX −Wallops Island, VA Opportunity for ABI Intensive ground campaigns in the Gulf of Mexico & at the DOE ARM site Collections of opportunity for ABI & GLM 17 −Atlanta, GA −Toronto, Canada −Lubbock, TX −Norman, OK ER-2 Loiter Time (based on an 8 hr mission)

18 Questions?