[Some] Updates on Research into Fire Radiative Power & Energy

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Environmental Monitoring & Modelling Research Group [Some] Updates on Research into Fire Radiative Power & Energy Presented by Martin Wooster (Kings College London, UK) Slide contributions from many others Environmental Monitoring and Modelling Research Group, Dept. of Geography, King s College London, UK. 1

MODIS FRP to FRE [problem is MODIS only provides a few observations per day] 2

Vermote (2009): MODIS FRP to FRE MODIS FRE 8 day 0.5 o resolution [but apparently underestimated compared to geostationary] 3

Country GLC2000 Freeborn et al. (2011) Addressing the spatiotemporal sampling design of MODIS to provide estimates of the fire radiative energy emitted from Africa, RSE.

MODIS FRP to FRE (compared to Vermote [2009])

Use MODIS CMG FRP Product MODIS CMG (8-day / 0.5 deg) Raw MODIS Data 1. Retrieve FRP in centre of MODIS swath 2. Retrieve area in centre of MODIS swath 3. Calculate the FRP per unit area in centre of MODIS swath: 40 FRP A 40 40 4. Multiply FRP per unit area in centre of swath by the total area of the swath: FRP Full A Full 40 A Full 1.897 A 40 FRP Full FRP 40 A A Full 40 FRP Full 1.897 FRP 40 Recommend that the sum of FRP measured within ± 40 of nadir is made available in MODIS Collection 6 CMG fire product (to aid bow tie adjustment). Freeborn et al (2011)

Geostationary FRP 7

Zhang et al. (2012) GEOSTATIONARY FRP Uses all current FRP capable geostationary sats ecept FY (China) WFABBA based fire detection algorithm. FRP calculated using MIR radiance method (linear fn). Applied to network of geostationary (GOES E/ W, Meteosat, MTSAT) Many fire piel records have non detections or saturation and gaps due to cloud cover. Reconstruction of full diurnal cycle using defaults. Zhang et al (2012) Near real time global biomass burning emissions product from geostationary satellite constellation, JGR.

Zhang et al. (2012) GEOSTATIONARY FRP Fuel Mass Combusted (0.25 deg grid cells) Comparison to GFEDv3.1 (Africa)

Effect of Errors of Omission On per fire basis Geosat FRP close to MODIS FRP MODIS (1 1 km) GOES (2.4 4 km) Red = fire piel detects Red = fire piel detects On per region basis Geosat FRP underestimates polar orbiting (MODIS) FRP Non detection of low FRP Fires MODIS Geostationary 10 10 MW 30 MW

GEO to LEO Merging 11

Merging GEO and LEO Datasets Temporal disadvantage of MODIS type data 12 Detection disadvantage of Geostationary type data Varying SEVIRI to MODIS FRP Ratio MODIS SEVIRI ~ 10 MW ~30 MW Freeborn et al. (2009)

Merging GEO and LEO Datasets Temporal disadvantage of Polar Orbiting data [MODIS] 13 Spatial disadvantage of Geostationary data [SEVIRI] MODIS Daily Mean SEVIRI FRP density (Wm 2 ) FRP Density (Wm 2 ) Daily Mean SEVIRI MODIS transfer fn. Merged & Bias Corrected Merged FRP Density (Wm 2 )

FRP merging of GEO & LEO Scientifically not yet solved based on GFAS gridded observations characterisation of bias (GEO FRP, view angle, local time) prediction of bias from previous co located observations Conditional PDF (Jun2010 Jul2012) Also new paper by Heyer et al (2013) Atmospheric Res. Usig MODIS & MTSAT SEVIRI FRP / MODIS FRP SEVIRI FRP / MODIS FRP SEVIRI FRP SEVIRI FRP

Potential to Merge with Burned Area Products 15

Fire Radiative Energy vs. Global Fire Emissions Database (v3) Feb 2004 Jan 2005 Fuel Consumption Totals (Southern and Northern Hemisphere Africa) Southern Africa Northern Africa Large discrepancies between GFED and raw FRE derived emissions...

Solution: Combine FRE & Burned Area Active Fire Detects & FRP Measure Burned Area Map Advantages Well observed fires measure of energy/total fuel consumption Disadvantages: Missing fires occurring between views. Missing data due to cloud cover. Missing data due to low FRP fires below active fire detection limit. Roy et al Advantages More complete coverage (wait for cloud to clear and for overpass) Disadvantages: Requires additional hard to obtain information on fuel load in order to estimate fuel consumption.

Fuel Consumption (g /m²)

Fuel Consumption (g /m²) + FRE = 1.110 8 MJ Total Fuel Burned = 39 ktonnes Burned area = 40.8 km² Fuel Consumption ~ 1.0 kg.m 2 500 m MODIS burned area data (white is day of interest) Closed Lowland Forest Median daily fuel consumption (and 5 day smoothing) Repeat for all well observed fires detected by SEVIRI Etrapolate using burned area for poorly observed fires 19

Fire Radiative Energy vs. Global Fire Emissions Database (v3) Feb 2004 Jan 2005 Fuel Consumption Totals (0.5 cells)

Fire Radiative Energy vs. Global Fire Emissions Database (v3) Feb 2004 Jan 2005 Fuel Consumption Totals (Southern and Northern Hemisphere Africa) Roberts et al. (2011) Integration of geostationary FRP and polar orbiter burned area datasets for enhanced biomass burning inventory, Remote Sensing Environ., 115.

Direct Relationship to Trace Gas Emission 22

Mebust et al. (2011) FRP and NO 2 Derive emissions factors (grammes of NO 2 emitted per kg of fuel burned) from combination of MODIS FRP and GOME NO 2 columns. Based on Ichoku and Kaufman (2005) approach previously used for aerosols rather than trace gases. EFs vary in the epected way, but are lower than previous measures. Underestimated contribution from smouldering previously?

Field Based FRP Studies 24

Remote Determination of Field Portable Open Path FTIR Spectrometry Emissions Factors (EF ) Gas Concentration Time Series FTIR Retrieved (ppm.m) Lab Validation True Pathlength Amount (ppm.m) Time (mins) Wooster et al. (2011) Field determination of biomass burning emission ratios and factors via open path FTIR spectroscopy, Atmos. Chem. Physics, 11, 11591 11615. Smith, Wooster et al. (2011) Absolute accuracy and sensitivity analysis of OP FTIR retrievals, Atmospheric Measurement Techniques, 4, 97 116.

Remote Determination of Emissions Factors (EF ) Emissions Ratio (mol.mol 1 ) Emissions Factor (g.m 2 ) Flaming Smouldering Used to provide environment & time specific EF parameters FRE recorded simultaneously from aircraft used to weight the components to calculate weighted mean EFs

Controls on MODIS FRP in Alaska Used MODIS FRP observations of Alaskan forests to determine the controls of FRP (forest type, large fire year, fire front or residual burning etc) Periods of high fire activity in the Alaskan boreal forest are characterized by a higher proportion of residual burning which may ultimately impact tree mortality and species makeup. Barrett and Kasischke (2012) Controls on variations in MODIS FRP in Alaskan boreal forests: Implications for fire severity conditions 27

New FRP Products NPP VIIRS SENTINEL3 SLSTR 28

Sentinel 3 Satellite Overview MWR OLCI SLSTR Payload Colour Instrument: OLCI Surface Temperature Instrument : SLSTR Radar Altimeter: SRAL Micro Wave Radiometer: MWR GPS receiver: GNSS Laser Retro Reflector: LRR Doris instrument X band antenna DORIS SRAL antenna LRR S band antenna Sentinel 3 SLSTR ~ 2013/14

SLSTR Spectral Bands Band # Centre centre µm Spectral Width µm Lmin/Tmin Lref/Tref Lma/Tma SNR/NEDT Radiometric Accuracy mwm -2 sr -1 nm -1 /K Ref SSD S1 0.555 0.02 2.92 2.92 585 20 2% 0.5km S2 0.659 0.02 2.43 2.43 475 20 2% 0.5km S3 0.865 0.02 1.53 1.53 295 20 2% 0.5km S4 1.375 0.15 0.58 0.58 113.1 20 2% 0.5km S5 1.61 0.06 0.39 0.39 74.0 20 2% 0.5km S6 2.25 0.05 0.13 0.13 24.3 20 2% 0.5km S7 3.74 0.38 200K 270K 323K 0.08K 0.2K (0.1K goal) 1km S8 10.85 0.9 200K 270K 321K 0.05K 0.2K (0.1K goal) 1km S9 12.0 1.0 200K 270K 318K 0.05K 0.2K (0.1K goal) 1km F1 3.74 0.38 350K 500K (634K Goal) 1K 3K 1km F2 10.85 0.9 330K 400K 0.5K 3K 1km @Lref Note: New spectral bands at 1.375um and 2.25um VIS/SWIR Spatial Resolution at Nadir of 0.5km Fire channels at 3.74 and 10.85um Radiometric accuracy requirement of 0.2K with goal of 0.1K Algorithm for active fire detection and FRP assessment should be in ESA ground station