24
Sources and fate of submicron particles: How observations can constrain emissions and deposition Delphine K. Farmer, Lauren Garofalo, Matson Pothier, Sonia Kreidenweis, Ezra Levin, Ethan Emerson Colorado State University

Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

  • Upload
    others

  • View
    2

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Sources and fate of submicron particles:How observations can constrain emissions and deposition

Delphine K. Farmer, Lauren Garofalo, Matson Pothier,Sonia Kreidenweis, Ezra Levin, Ethan Emerson

Colorado State University

Page 2: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire
Page 3: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire
Page 4: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

AQUARIUS-relevant aerosol questions

• How do organic and inorganic components contribute to wintertime PM?Organics NHx, NOx, Cl

• What is the size-dependence of composition?

• What chemistry is controlling PM mass and composition, and how does this vary with meteorology?

• How accurate are emissions inventories (traffic, agriculture, VCPs, etc)?

• How does deposition affect gas and particle fate – and thus chemistry?

Page 5: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Observational constraints on atmospheric chemical processes

Ground sites Aircraft platform

• Detailed chemical analysis• Longer-term measurements • Temporal variability• Flux measurements: emission & deposition• Single point locations

• Chemical processes, emissions• (Slightly less) detailed chemical analysis• Fast time-resolution measurements• Spatial & vertical gradients• Multiple locations

Example of ground-based flux measurements to think about particle dry deposition

Example of using bulk aerosol measurements to study emissions & chemistry

Page 6: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire
Page 7: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Manitou Forest, CO (NOAA)4 seasons, 2015*array of turbulence conditions

Investigating dry deposition by size-resolved particle & black carbon flux measurements (eddy covariance + UHSAS, SP2)

Southern Great Plains, OK (DOE)6 weeks, 2016

Page 8: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Manitou Forest, CO (NOAA)4 seasons, 2015*array of turbulence conditions

Investigating dry deposition by size-resolved particle & black carbon flux measurements (eddy covariance + UHSAS, SP2)

Southern Great Plains, OK (DOE)6 weeks, 2016

Page 9: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Zhang et al., (2001); Petroff & Zhang, (2010)

* Model shown is for forested terrain

Sophisticated deposition models capture the observations (but widely used simpler ones generally do not)

Page 10: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Zhang et al., (2001); Petroff & Zhang, (2010)

* Model shown is for forested terrain

Sophisticated deposition models capture the observations (but widely used simpler ones generally do not)

Page 11: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Standard vs revised parameterizations for dry deposition impact (size-resolved) particle lifetime

[Emerson et al. In prep]

Page 12: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

*Collaboration with Anna Hodshire + Jeff Pierce (CSU); Manuscript in prep

Revised particle dry deposition parameterizations have a substantial effect on modeled aerosols + radiative effects

Page 13: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

• We can use flux observations to constrain model parameterizations of sources & sinks

• Particularly large particle deposition uncertainties over cryosphere & water

• Remote / receptor sites offer an opportunity to investigate particle fate – and other impacts of deposition on C,N cycles –using flux measurements

• In contrast, urban & agricultural sites offer opportunity to study source emissions by direct flux measurements (VCPs, BC, NH3)

→ few urban flux sites/measurements in the US

Page 14: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire
Page 15: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

The Western Wildfire Experiment for Cloud Chemistry, Aerosol Absorption & Nitrogen

WE-CAN was led by Emily Fischer (CSU)HR-AMS [coPI Sonia Kreidenweis, postdoc Lauren Garofalo + PhD student Matson Pothier]

Page 16: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Sub-micron aerosol in wildfire smoke is overwhelmingly organic

AMS provides bulk sub-micron measurements and some useful markers for specific molecules, along with factor analysis for characteristic components Organic

ChlorideSulphateAmmoniumNitrateBlack carbon

[Garofalo et al. ACS Earth & Space Chemistry. 2019]

Page 17: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Source

0.5

0.4

0.3

0.2

0.1

0.0

OA E

miss

ion R

atio,

µg m

-3 pp

bv-1

Wigw

am F

ireSh

arps

Fire

Monu

ment

Fire

South

Sug

arloa

f Fire

Beav

er C

reek

Fire

Kiwa

h Fire

Red F

eathe

r Lak

es R

x Fire

Carr

Fire

Taylo

r Cre

ek F

ireSi

lver C

reek

Fire

RF06

Rab

bit F

oot F

ireRF

10 R

abbit

Foo

t Fire

RF11

Rab

bit F

oot F

ireBe

ar T

rap F

ireGo

ldston

e Fire

ER =

Em

issio

ns R

atio

[Garofalo et al. ACS Earth & Space Chemistry. 2019]

We can calculate emissions ratios, accounting for simple dilution, and find that organic aerosol emissions are relatively consistent

-

-bkg

bkg

X XXNEMRCO CO CO∆

= =∆

Page 18: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

SourceMeasurements

Dilution

ER =

Em

issio

ns R

atio

Does the fire plume chemically evolve in the near-field?

Page 19: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

RF09: Bear Trap Fire, UtahPine + Aspen

Does the fire plume chemically evolve in the near-field?

MAX

MIN

400

300

200

100

0

OA,

ug

sm-3

9:00 PM8/9/2018

9:30 PM 10:00 PM 10:30 PM 11:00 PM 11:30 PM 12:00 AM8/10/2018

Date and Time, UTC

Org

anic

Aer

osol

, ug

sm-3

Date and Time, UTC

(b)

Page 20: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

OA changes: oxidation & dilution-driven evaporation balance!

fC2H4O2+: Evaporation of more volatile components (anhydrous sugars)

fCO2+: Addition of oxidized organics (SOA)

[Garofalo et al. ACS Earth & Space Chemistry. 2019]

Page 21: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

What happens on longer timescales and in polluted environments?

Old smoke Residual smoke from Central Valley (smoke + urban)

Page 22: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

What else would have been useful for this type of work?

• Size distribution measurements are not trivial

• Organic aerosol molecular speciation can compliment bulk aerosol composition

• Refractory inorganic ions provide additional information

• Understanding of volatility (PMF can only get you so far, although thermal denuders have time resolution challenges)

• AMS only measures the non-refractory component of PM0.8-800– what about the rest of the aerosol?

Page 23: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Observational constraints on emission and deposition terms are useful – and provide insight on chemistry

Organic aerosol is complex: chemical tracers are useful for separating out processes*But it’s important to recognize measurement limitations

Dry deposition is an important – but poorly characterized – loss process for sub-micron particles

Flux measurements provide insight on both sources and sinks of trace gases and particles

Page 24: Sources and fate of submicron particles: How observations ... · Source. 0.5 0.4 0.3 0.2 0.1 0.0. OA Emission Ratio, µg m-3. ppbv-1. ER = Emissions Ratio. Wigwam Fire Sharps Fire

Dr. Lauren Garofalo Matson Pothier

+ Prof. Sonia Kreidenweis (coPI), Dr. Ezra Levin (CSU, black carbon), Dr. Teresa Campos (NCAR for CO measurements) and the entire WE-CAN Science Team

+ Holly DeBolt (CSU, aerosol fluxes)

Acknowledgements

Ethan Emerson & Gavin McMeeking [Handix]