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Sources of Primary and Secondary Particles in the Houston Area in 2006
Objectives•Examine relative importance of primary and secondary aerosol sources•Evaluate contribution from Parish power plant and industrial emissions•Compare with TexAQS 2000 data
Charles Brock, Adam Wollny, Rebecca Washenfelder, Ann Middlebrook, Roya Bahreini, Ryan Spackman, Shuka Schwarz, John Holloway, Jeff Peischl, Tom
Ryerson, Andy Neuman, John Nowak, Joost de Gouw, Carsten Warneke, Michael Trainer, Andreas Stohl, Tahllee Baynard, and others. . ..
Aerosol Measurements on the NOAA P-3Particle size distributions, .005-8 µm, 1 sec.• Calculate integrated number and volume (proportional to
mass), uncertainties in integrated volume ~25%
Aerosol mass spectrometer, submicron sulfate, nitrate, ammonium, organics, 10 s
• mission absolute uncertainties ~50% (single-flight variability ~25%), good sensitivity
• Middlebrook talk, Bahreini poster
Particle-in-liquid sampler, submicron water-soluble organic (Hecobian poster)Single particle soot photometer (Spackman poster)Cavity ringdown extinction, f(rh), absorption (Baynard poster; Lack talk, Massoli poster for ship instruments)Actinic flux spectral radiometer (Stark poster)
Aerosol Measurements on the NOAA P-3Particle size distributions, .005-8 µm, 1 sec.• Calculate integrated number and volume (proportional to
mass), uncertainties in integrated volume ~25%
Aerosol mass spectrometer, submicron sulfate, nitrate, ammonium, organics, 10 s
• mission absolute uncertainties ~50% (single-flight variability ~25%), good sensitivity
• Middlebrook talk, Bahreini poster
Particle-in-liquid sampler, submicron water-soluble organic (Hecobian poster)Single particle soot photometer (Spackman poster)Cavity ringdown extinction, f(rh), absorption (Baynard poster; Lack talk, Massoli poster for ship instruments)Actinic flux spectral radiometer (Stark poster)
Not available in 2000 campaign
Focus on 27 September 2006:•High O3 day•Wind ~constant in direction, ~2x variable in speed•Many downwind transects•Source plumes ~separated•Qualitatively similar to days examined in 2000
30.6
30.4
30.2
30.0
29.8
29.6
29.4
29.2
29.0
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
31.0
30.8
30.6
30.4
30.2
30.0
29.8
29.6
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
28 August, 2000 27 September, 2006
Color & size proportional to particle volume. Scales differ.
Parish Industries
Parish
Industries
WindWind
30.6
30.4
30.2
30.0
29.8
29.6
29.4
29.2
29.0
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
31.0
30.8
30.6
30.4
30.2
30.0
29.8
29.6
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
Color & size proportional to particle volume. Scales differ.
But relative to August 2000. . .•Temperature cooler•Mixing less vigorous ↕ and ↔•Fewer photons•Background more variable, so uncertainties in Δ larger
28 August, 2000 27 September, 2006
Parish Industries
Parish
Industries
Background variability caused by recirculation of Houston/Beaumont area plume from previous day.
FLEXPART model transport footprint from 40,000 backtrajectories at aircraft location. Color proportional to backtrajectory residence time in
lowest 100 meters. Dots are MODIS fire hotspots.
Subtracting the background to isolate Parish and ship channel industrial plumes:
31.0
30.8
30.6
30.4
30.2
30.0
29.8
29.6
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
12
10
8
6
4
2
Part
icle
Vol
ume
and
SO2
-95.6 -95.4 -95.2 -95.0 -94.8 -94.6Longitude
Particle Volume µm3 cm-3
SO2 (ppbv)
Subjective and prone to error-->30% in volume?
Parish
IndustriesParish
Industries
27 September, 2006
Particle volume enhancements above background
Enhancements are <2 µm3cm-3 on average
Growth does not continue far downwind
Very little volume enhancement immediately downwind of sources
5
4
3
2
1
0
Particle Volume Enhancem
ent (µm3 cm
-3)
Parish
Industries
27 September, 2006
800
600
400
200
0
Part
icle
Vol
ume
Flux
(cm
3 s-1
)
86420Time Since Emission (hr)
Ship Channel Parish Power Plant Ship Channel 09/19 Ship Channel 09/21
Estimate flux of particle volume (mass) in ship channel and Parish power plant plumes
Uncertainties large due to background subtraction, wind speed at time of emission, PBL height (transport time uncertainties not shown)
Ship channel flux ~2x Parish flux
“Primary” mass emissions are small compared with secondary formation, but not negligible in ship channel area
Composition of particles from ship channel and Parish power plant
Ship channel particle mass is ~50% organic
Parish plume has no significant organic component
Black carbon flux from ship channel ~10 g s-1
(not shown), small but not negligible
1200
1000
800
600
400
200
0
Part
icle
Mas
s Fl
ux (g
s-1
)
86420Time Since Emission (hr)
Mass Fluxes from AMS Measurements Ship Channel Inorganic Ship Channel Organic Parish Inorganic Ship Channel Sulfate 09/19 Ship Channel Sulfate 09/21
Fluxes of SO2 from Ship Channel and Parish are comparable
3.5x1025
3.0
2.5
2.0
1.5
1.0
0.5
0.0
SO2 F
lux
(mol
ec s
-1)
86420Time Since Emission (hr)
Ship Channel Parish Power Plant
First Parish transect is in agreement with CEMS
Decline in flux with time may be caused by:•lower fluxes at time of emission (<10% var.)•dry deposition•g-p conversion (~20%)•background subtraction and other analysis biases
See Washenfelder et al. poster
0.35
0.30
0.25
0.20
0.15
0.10
0.05
0.00
Frac
tion
of P
lum
e S
as S
ulfa
te
86420Time Since Emission (hr)
Ship Channel Parish Power Plant
Oxidation of SO2 to form sulfate is comparable in Ship Channel and Parish plumes
Compare 2006 volume fluxes with 2000•Fluxes appear to be 5-10x lower in ship channel plume in 2006•Fluxes 2-4x lower even in Parish plume in 2006
Same Scale!Color & size proportional to particle volume, same dynamic range.
30.6
30.4
30.2
30.0
29.8
29.6
29.4
29.2
29.0
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
31.0
30.8
30.6
30.4
30.2
30.0
29.8
29.6
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
28 August, 2000 27 September, 2006
Compare sulfur oxidation in Parish plume2006 vs 2000
Oxidation is ~2x lower in Parish plume in 2006 than estimated in 2000
Remember SO2 flux decreases of ~2x also due to dry deposition or analysis biases.
Many possible causes:need careful evaluation of oxidative environment in 2006 and 2000
Not in time for RSS!
0.7
0.6
0.5
0.4
0.3
0.2
0.1
0.0
Frac
tion
of P
lum
e Su
lfur i
n Pa
rtic
ulat
e Su
lfate
86420
Transport Time (hr)
27 September 2006 27& 28 August 2000
Small particles are rapidly formed downwind of sources, especially of SO2.
31.0
30.8
30.6
30.4
30.2
30.0
29.8
29.6
latit
ude
-96.0 -95.5 -95.0 -94.5
longitude
50x103
40
30
20
10
0
Particle number concentration (cm
-3)
27 September, 2006
Map color-coded by particle number concentration
Number may be correlated with health effects
As in 2000 data, number maximum occurs immediately downwind of SO2sources
Coagulation rapidly depletes number
Sources of Primary and Secondary Particles in the Houston Area in 2006
Conclusions•Secondary sources of particle mass dominate primary sources. “Primary” emissions (<20 minutes old) are not negligible in ship channel•On this day, the ship channel region produced fluxes of particle mass ~2x that of the Parish power plant•On this day, secondary mass formation ~2-10x lower than on comparable day during TexAQS 2000. Variability driven by meteorology, emissions, photochemistry, analysis biases? Need much more analysis for concrete results