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The Heterogeneous Interaction of
Atmospheric Trace Gases on Mineral
Aerosols and soot
Federico Karagulian
(Supervisor: M.J. Rossi)

Laboratoire de Pollution Atmosphérique et Sol
(LPAS), Ecole Polytechnique Fédérale de Lausanne
(EPFL), CH-1015-Lausanne (Switzerland)
Which kind of chemistry for atmospheric pollution?

Nitrate’s chemistry: nighttime

Ozone chemistry: daytime

Ozone forms when precursor compounds
react in the presence of sunlight and high
temperatures.

Important nitrate reactions at night
(daytime photolysis in the yellow box)
Atmospheric chemistry: Ozone formation in the troposphere
O 3 + hυ → O(1 D) + O 2

λ < 320 nm

H 2 O + O(1 D) → 2OH
OH + VOCs → R

Organic radical

N 2 O + O( 1 D) → 2NO

R + O 2 → RO 2
RO 2 + NO → RO + NO 2
NO 2 + hν → NO + O( 3 P)
O 2 + O( 3 P) → O 3

OH + NO 2 → HNO3

Polluted
atmosphere

HNO 3 + hν → OH + NO 2
Slow process, therefore HNO3 may represent a
reservoir for O3
erosion and
deforestation

Mineral dust emission
change of landusage: fire and wind

traveling with wind
Intense African dust storm sent a massive dust plume
westward over the Atlantic Ocean on March 2, 2003.

Images courtesy Jeffrey Schmaltz and Jacques Descloitres, MODIS Rapid Response Team, NASA GSFC Animation credit:
NASA Goddard Space Flight Center, Scientific Visualization Studio

http://svs.gsfc.nasa.gov/stories/dust_20030306/index.html
Izaña and Sta. Cruz de Tenerife
Normal situation

Mineral Dust events

MINATROC field campaign (July, 2002)
Izaña and Sta. Cruz de Tenerife
Normal situation

Mineral Dust events

MINATROC field campaign (July, 2002)
Environmental effects of aerosols (Particulate Matter PM):
 Soot aerosol and black carbon (BC) have a warming effect absorbing
sunlight. The contribution of BC and soot to global warming may be second
only to that of CO2. 1
 Mineral dust have a warming and cooling effect
Simulation. increasing of dust load from 4.0 x 104 to 1.3 x 105 mg / m2 brings to:
 0.04  0.21 W/m2 at the top of the atmosphere (heating)2
 -0.74 -1.82 W/m2 at the surface (cooling)2

 Absorption and scattering of UV radiation by aerosol modify the kinetics
of photochemical reactions.
 Temperature modification by aerosols modify the kinetics of chemical reactions
1
2

M.A. Jacobson, Nature vol. 409, p. 695 (2001).
S. Woodward, Geophys. Res. Lett. 32 (18) Sep 28, 2005.
Mineral dust events and heterogeneous chemistry
Mineral dust = mineral aerosol (‘small mineral particle’)
Size = 1 – 10 µm

O3
NOx = NO+NO2
NOy = NO3 + N2O5 +HNO3

+

=>

Reaction
products

Gas + solid reaction = heterogeneous reaction
γ=

number of molecules taken up
total number of collision

=

Probability that a molecule is taken
up on the solid substrate
(uptake coefficient)
Mineral dust aerosol surrogates

Real event: dust storm

Representative Samples

Model substances such as
CaCO3, Natural Limestone,
Kaolinite, Arizona Test
Dust, Saharan Dust

Heterogeneous
Reactions with
trace gases

Atmospheric consequences
a) Reduction of the
atmospheric concentration of
trace gases like
HNO3, NO3, N2O5, O3.
b) Strong influence
on the global ozone
budget
How does mineral dust affect atmospheric chemistry ?
HO2

O3

N2O5
NO

NO2

DUST

SO2

HNO3
OH
Global

∆(%) Bauer et al.2

NO3
∆(%) Bian and Zender 3

∆H

∆P+H

∆H

∆O3

-5.4

-0.7

-0.9

∆HNO3

-35.3

-3.5

-3.8

∆NO3

-17.7

-4.7

-5.9

∆N2O5

-10.6

0.0

-2.1

∆NO2

-1.4

+1.1

-0.3

∆OH

-6.6

-11.1

-9.6

Grey line = model simulation
Black line = field measurements 1
(Monte Cimone, 2000)

P. Bonasoni; et al., Atmos. Chem. Phys. 2004, 4, 1201-1215.
Bauer et al., J. Geophys. Res. Atm., Vol. 109, doi:10.1029/2003JD003868, 2004.
3
Bian and Zender, J. Gephys. Res. Atm, Vol 108, doi:10.1029/2002JD003143, 2003.
1
2
Experimental: Knudsen Flow Reactor

Experimental set up

…in the lab
REMPI cell

Knudsen reactor

control panel

pumping

detection chamber
REMPI detection of NO and NO2: λ = 252.6 nm
λ = 511 nm
Visible light emission
Molecular excitation

Pumping laser

−

NO 2 + 3hν 2 + hν 2 → NO + e

(b)

50
40
30

2

20
1

10

+

+
2

NO + 2hν 1 + 2hυ1 → NO + e

(a)

3

2

−

-3

60x10

4

Energy (mJ/cm )

+

NO REMPI signal (Volt x s)

Ions yield

Molecular photoionization

0

0
445

450

wavelength (nm)

455

460
Example: NO3 uptake experiment on 2 g of CaCO3
 MS detection
 NO2 REMPI detection

Multi-Diagnostic Detection
1.6

F0M

N 2O 5 → NO 2 + NO 3
T = 500 K

MS Signal (Volt)

1.4

NO3 inlet

reaction on

FrM

(a)

1.2

(b)

1.0

(a)

0.8

(b)

(c)

0.6
0.4
0.2

(d)x10
(d)x10

0.0
200

Heterogeneous rate loss

(c)

400

600

time (s)

800

1000

MS Signal: (a) = m/e 30; (b) = m/e 46;
(c) = NO2 REMPI signal at λ = 511 nm; (d) = m/e 62 (NO3)

F0M
k ss = ( M − 1) ⋅ k esc = γ ss ⋅ ω
Fr

γ ss = Steady state uptake coefficient
NO3 uptake on 200 mg of Kaolinite

gas residence time τ = 1/kesc = 0.57 s (orifice = 8 mm)
[NO3] = (7.0 ± 1.0) x 1011 cm-3 (30 ppb)
1.5

MS Signal (Volt)

NO2 uptake on adsorbed NO3
(a) = m/e 30; (b) = m/e 46; (c) = NO2
REMPI signal; (d) = m/e 62 NO3;
(e) = m/e 63 HNO3

reaction on

NO3 inlet

(a)
(a)

(b)

1.0

(b)

(c)

(c)

0.5

(d)x10

(d)x10
0.0

N 2 O 5(g) Determined from excess MS signal at

200

400

600

800

time (s)

(e)

1000

1200

m/e 46 after correction for NO2 REMPI signal
0.14

MS Signal (Volt)

NO 3(ads) + NO 2 → N 2 O 5(ads)

reaction on

0.12
0.10

N 2 O 5(ads) → N 2 O 5(g)

(c)

0.08
0.06
0.04

(b)x10

0.02

400

500

N 2 O5(ads) + H 2 O (ads) → 2HNO3(g)

(a) x10

(d)x10

0.00

600

700

800

time (s)

HNO3(g)
Proof of adsorbed NO3: NO2 REMPI detection

NO + NO 3(ads) → 2NO 2
Titration on Arizona Test Dust surface
15

Flow (molecule/s)

12

NO3
inlet

reaction on
NO3 stop
NO admission

10

reaction on

NO 2 + NO 3(ads) → 2NO 2 + 1 O 2
2

8
6

(a)

4

(b)

Saharan Dust

2
0
400

600

time (s)

NO2

800

1000

15

15x10

Flow (molecule/s)

14x10

10

NO3 stop
NO2 admission

reaction on

(b)
NO3
inlet

reaction on

5

(a)

0
600

800

time (s)

1000

1200
NO3 and N2O5 reaction on CaCO3 (powder calcium carbonate)

NO 3 + NO 2

CaCO 3

Formation of an intermediate

N 2 O 5(g)

adsorbed

gas phase

N 2 O 5(ads)

gas phase

CaCO 3 + H 2 O → Ca(OH)(HCO 3 )

N 2 O 5(g) + Ca(OH)(HCO 3 ) → Ca(NO 3 ) 2 + H 2 O (s) + CO 2(g)
Delayed formation of nitric acid
Nitrate formation
on the surface

N 2 O 5(g) + H 2 O (ads) → 2HNO 3(g)
S − OH + HNO 3(ads) → S − NO 3 + H 2 O (ads,g)
N 2 O 5(ads)

2HNO3(g)

+
Fresh CaCO3

H 2 O (ads) Adsorbed water
H2O

Aged CaCO3
Ozone reactivity on mineral dust: reaction or
decomposition?
Ozone
Decomposition: CaCO3

O 3 + SS → O(SS) + O 2

O 2 + O( 3 P) → O 3

O 3 + O(SS) → O 2 + O 2 (SS)

O 2 (SS) → O 2 + SS
net

2O 3 → 3O 2

Ozone
re-formation

r = 1.5

O 3 + SS → adduct

Reduction in of the Ozone
troposphere budget

O 3 + O(SS) → adduct

Ozone
Reactivity: Kaolinite, Saharan Dust;
Arizona Test Dust; natural limestone
Mineral dust and Atmospheric implications
Example of the N2O5 reactivity at T= 293K; lifetime increasing
cAγ
k het =
= 1/τ het (s −1 )
4

Loss rate constant due to heterogeneous uptake
of a gas species onto small particles (<2µ m)

A = 1.5 x 10-6 cm2 cm-3 (surface area density for Saharan Dust; c = mean
molecular speed; γ (NO3, N2O5) ~ 0.2
[NO2] = 10 ppb

loss ←O5 N 2 O 5

k N2
het

k

hydr
het

−4 −1

= 2.25x10 s

NO 2 + NO 3

k −1 [ NO 2 ] = 0.48s −1

NO
k het 3 = 2.4x10 −3 s −1

loss

HNO3
N2
k hetO5 = 2.0x10 −3 s −1

τ = 20s

k1 (293K) = 4.6x10 −2 s −1

NO
k ph 3 = 0.2s −1

−1

N
τ ss 2O5

NO
 N 2O5 k het 3 k1 (293) 
 = 8.5 min
=  k het +

k -1 [ NO 2 ] 



NO
τ het 3 = 7 min
NO
τ ph 3 = 5s
Soot production: incomplete fuel combustion
Flame Type
(Decane)
Rich

“gray”

40

Lean

Flame soot

Soot
type

“black”

20

3

Diameter soot
particle [nm]

Laboratory flame soot
Fuel: hexane,
octane, decane,
toluene, Diesel

 Black soot- low air/fuel ratios: soot highly agglomerated and consisted primarily of elemental C.
 Grey soot-high air/fuel ratios: soot less agglomerated and consisted of volatile organic materials.
N2O5 reaction on soot
0.7

N2O5 on 10 mg of grey soot

MS Signal (Volt)

0.6

reaction on (sample exposed)

plunger lowered

plunger lowered

0.5
N2O5

0.4
0.3
0.2

gas phase NO production

0.1

NOy

0.0
200

400

600
time (s)

800

1000

soot
renoxificatio
n

NOx = NO + NO2
0.7

MS Signal (Volt)

NOy

0.5

plunger lowered

reaction on (sample exposed)

plunger lowered

0.6

N2O5 on 10 mg of grey soot

N2O5

0.4
0.3
0.2
gas phase NO2 production

0.1
0.0
0

200

400

600

800
time (s)

1000

1200
Soot is a potential source of tropospheric HONO
NO 2 + soot(grey) → HONO + products

NO3 reaction on soot

NO + products

Heterogeneous reactions

(NO3 + NO2) reaction on soot (grey)

HONO formation
Heterogeneous interaction of trace gases on substrates of
technological importance: inkjet print paper
Samples: Polyester + AlOOH or SiO2 + Dye + additives

Fading effect

5 Torr NO2

1 Torr NO2
Acknowledgment
 M.J. Rossi
 Hubert Van den Bergh
 MINATROC project
 OFES foundation
 ILFORD Imaging GmbH (CH)
 Maria S.
 Cristina
 Flavio Comino

Thanks

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Mineral Dust and Soot: Atmospheric Chemistry

  • 1. The Heterogeneous Interaction of Atmospheric Trace Gases on Mineral Aerosols and soot Federico Karagulian (Supervisor: M.J. Rossi) Laboratoire de Pollution Atmosphérique et Sol (LPAS), Ecole Polytechnique Fédérale de Lausanne (EPFL), CH-1015-Lausanne (Switzerland)
  • 2. Which kind of chemistry for atmospheric pollution? Nitrate’s chemistry: nighttime Ozone chemistry: daytime Ozone forms when precursor compounds react in the presence of sunlight and high temperatures. Important nitrate reactions at night (daytime photolysis in the yellow box)
  • 3. Atmospheric chemistry: Ozone formation in the troposphere O 3 + hυ → O(1 D) + O 2 λ < 320 nm H 2 O + O(1 D) → 2OH OH + VOCs → R Organic radical N 2 O + O( 1 D) → 2NO R + O 2 → RO 2 RO 2 + NO → RO + NO 2 NO 2 + hν → NO + O( 3 P) O 2 + O( 3 P) → O 3 OH + NO 2 → HNO3 Polluted atmosphere HNO 3 + hν → OH + NO 2 Slow process, therefore HNO3 may represent a reservoir for O3
  • 4. erosion and deforestation Mineral dust emission change of landusage: fire and wind traveling with wind
  • 5. Intense African dust storm sent a massive dust plume westward over the Atlantic Ocean on March 2, 2003. Images courtesy Jeffrey Schmaltz and Jacques Descloitres, MODIS Rapid Response Team, NASA GSFC Animation credit: NASA Goddard Space Flight Center, Scientific Visualization Studio http://svs.gsfc.nasa.gov/stories/dust_20030306/index.html
  • 6. Izaña and Sta. Cruz de Tenerife Normal situation Mineral Dust events MINATROC field campaign (July, 2002)
  • 7. Izaña and Sta. Cruz de Tenerife Normal situation Mineral Dust events MINATROC field campaign (July, 2002)
  • 8. Environmental effects of aerosols (Particulate Matter PM):  Soot aerosol and black carbon (BC) have a warming effect absorbing sunlight. The contribution of BC and soot to global warming may be second only to that of CO2. 1  Mineral dust have a warming and cooling effect Simulation. increasing of dust load from 4.0 x 104 to 1.3 x 105 mg / m2 brings to:  0.04  0.21 W/m2 at the top of the atmosphere (heating)2  -0.74 -1.82 W/m2 at the surface (cooling)2  Absorption and scattering of UV radiation by aerosol modify the kinetics of photochemical reactions.  Temperature modification by aerosols modify the kinetics of chemical reactions 1 2 M.A. Jacobson, Nature vol. 409, p. 695 (2001). S. Woodward, Geophys. Res. Lett. 32 (18) Sep 28, 2005.
  • 9. Mineral dust events and heterogeneous chemistry Mineral dust = mineral aerosol (‘small mineral particle’) Size = 1 – 10 µm O3 NOx = NO+NO2 NOy = NO3 + N2O5 +HNO3 + => Reaction products Gas + solid reaction = heterogeneous reaction γ= number of molecules taken up total number of collision = Probability that a molecule is taken up on the solid substrate (uptake coefficient)
  • 10. Mineral dust aerosol surrogates Real event: dust storm Representative Samples Model substances such as CaCO3, Natural Limestone, Kaolinite, Arizona Test Dust, Saharan Dust Heterogeneous Reactions with trace gases Atmospheric consequences a) Reduction of the atmospheric concentration of trace gases like HNO3, NO3, N2O5, O3. b) Strong influence on the global ozone budget
  • 11. How does mineral dust affect atmospheric chemistry ? HO2 O3 N2O5 NO NO2 DUST SO2 HNO3 OH Global ∆(%) Bauer et al.2 NO3 ∆(%) Bian and Zender 3 ∆H ∆P+H ∆H ∆O3 -5.4 -0.7 -0.9 ∆HNO3 -35.3 -3.5 -3.8 ∆NO3 -17.7 -4.7 -5.9 ∆N2O5 -10.6 0.0 -2.1 ∆NO2 -1.4 +1.1 -0.3 ∆OH -6.6 -11.1 -9.6 Grey line = model simulation Black line = field measurements 1 (Monte Cimone, 2000) P. Bonasoni; et al., Atmos. Chem. Phys. 2004, 4, 1201-1215. Bauer et al., J. Geophys. Res. Atm., Vol. 109, doi:10.1029/2003JD003868, 2004. 3 Bian and Zender, J. Gephys. Res. Atm, Vol 108, doi:10.1029/2002JD003143, 2003. 1 2
  • 12. Experimental: Knudsen Flow Reactor Experimental set up …in the lab
  • 13. REMPI cell Knudsen reactor control panel pumping detection chamber
  • 14. REMPI detection of NO and NO2: λ = 252.6 nm λ = 511 nm Visible light emission Molecular excitation Pumping laser − NO 2 + 3hν 2 + hν 2 → NO + e (b) 50 40 30 2 20 1 10 + + 2 NO + 2hν 1 + 2hυ1 → NO + e (a) 3 2 − -3 60x10 4 Energy (mJ/cm ) + NO REMPI signal (Volt x s) Ions yield Molecular photoionization 0 0 445 450 wavelength (nm) 455 460
  • 15. Example: NO3 uptake experiment on 2 g of CaCO3  MS detection  NO2 REMPI detection Multi-Diagnostic Detection 1.6 F0M N 2O 5 → NO 2 + NO 3 T = 500 K MS Signal (Volt) 1.4 NO3 inlet reaction on FrM (a) 1.2 (b) 1.0 (a) 0.8 (b) (c) 0.6 0.4 0.2 (d)x10 (d)x10 0.0 200 Heterogeneous rate loss (c) 400 600 time (s) 800 1000 MS Signal: (a) = m/e 30; (b) = m/e 46; (c) = NO2 REMPI signal at λ = 511 nm; (d) = m/e 62 (NO3) F0M k ss = ( M − 1) ⋅ k esc = γ ss ⋅ ω Fr γ ss = Steady state uptake coefficient
  • 16. NO3 uptake on 200 mg of Kaolinite gas residence time τ = 1/kesc = 0.57 s (orifice = 8 mm) [NO3] = (7.0 ± 1.0) x 1011 cm-3 (30 ppb) 1.5 MS Signal (Volt) NO2 uptake on adsorbed NO3 (a) = m/e 30; (b) = m/e 46; (c) = NO2 REMPI signal; (d) = m/e 62 NO3; (e) = m/e 63 HNO3 reaction on NO3 inlet (a) (a) (b) 1.0 (b) (c) (c) 0.5 (d)x10 (d)x10 0.0 N 2 O 5(g) Determined from excess MS signal at 200 400 600 800 time (s) (e) 1000 1200 m/e 46 after correction for NO2 REMPI signal 0.14 MS Signal (Volt) NO 3(ads) + NO 2 → N 2 O 5(ads) reaction on 0.12 0.10 N 2 O 5(ads) → N 2 O 5(g) (c) 0.08 0.06 0.04 (b)x10 0.02 400 500 N 2 O5(ads) + H 2 O (ads) → 2HNO3(g) (a) x10 (d)x10 0.00 600 700 800 time (s) HNO3(g)
  • 17. Proof of adsorbed NO3: NO2 REMPI detection NO + NO 3(ads) → 2NO 2 Titration on Arizona Test Dust surface 15 Flow (molecule/s) 12 NO3 inlet reaction on NO3 stop NO admission 10 reaction on NO 2 + NO 3(ads) → 2NO 2 + 1 O 2 2 8 6 (a) 4 (b) Saharan Dust 2 0 400 600 time (s) NO2 800 1000 15 15x10 Flow (molecule/s) 14x10 10 NO3 stop NO2 admission reaction on (b) NO3 inlet reaction on 5 (a) 0 600 800 time (s) 1000 1200
  • 18. NO3 and N2O5 reaction on CaCO3 (powder calcium carbonate) NO 3 + NO 2 CaCO 3 Formation of an intermediate N 2 O 5(g) adsorbed gas phase N 2 O 5(ads) gas phase CaCO 3 + H 2 O → Ca(OH)(HCO 3 ) N 2 O 5(g) + Ca(OH)(HCO 3 ) → Ca(NO 3 ) 2 + H 2 O (s) + CO 2(g) Delayed formation of nitric acid Nitrate formation on the surface N 2 O 5(g) + H 2 O (ads) → 2HNO 3(g) S − OH + HNO 3(ads) → S − NO 3 + H 2 O (ads,g)
  • 19. N 2 O 5(ads) 2HNO3(g) + Fresh CaCO3 H 2 O (ads) Adsorbed water H2O Aged CaCO3
  • 20. Ozone reactivity on mineral dust: reaction or decomposition? Ozone Decomposition: CaCO3 O 3 + SS → O(SS) + O 2 O 2 + O( 3 P) → O 3 O 3 + O(SS) → O 2 + O 2 (SS) O 2 (SS) → O 2 + SS net 2O 3 → 3O 2 Ozone re-formation r = 1.5 O 3 + SS → adduct Reduction in of the Ozone troposphere budget O 3 + O(SS) → adduct Ozone Reactivity: Kaolinite, Saharan Dust; Arizona Test Dust; natural limestone
  • 21. Mineral dust and Atmospheric implications Example of the N2O5 reactivity at T= 293K; lifetime increasing cAγ k het = = 1/τ het (s −1 ) 4 Loss rate constant due to heterogeneous uptake of a gas species onto small particles (<2µ m) A = 1.5 x 10-6 cm2 cm-3 (surface area density for Saharan Dust; c = mean molecular speed; γ (NO3, N2O5) ~ 0.2 [NO2] = 10 ppb loss ←O5 N 2 O 5  k N2 het k hydr het −4 −1 = 2.25x10 s NO 2 + NO 3 k −1 [ NO 2 ] = 0.48s −1 NO k het 3 = 2.4x10 −3 s −1 loss HNO3 N2 k hetO5 = 2.0x10 −3 s −1 τ = 20s k1 (293K) = 4.6x10 −2 s −1 NO k ph 3 = 0.2s −1 −1 N τ ss 2O5 NO  N 2O5 k het 3 k1 (293)   = 8.5 min =  k het +  k -1 [ NO 2 ]    NO τ het 3 = 7 min NO τ ph 3 = 5s
  • 22. Soot production: incomplete fuel combustion Flame Type (Decane) Rich “gray” 40 Lean Flame soot Soot type “black” 20 3 Diameter soot particle [nm] Laboratory flame soot Fuel: hexane, octane, decane, toluene, Diesel  Black soot- low air/fuel ratios: soot highly agglomerated and consisted primarily of elemental C.  Grey soot-high air/fuel ratios: soot less agglomerated and consisted of volatile organic materials.
  • 23. N2O5 reaction on soot 0.7 N2O5 on 10 mg of grey soot MS Signal (Volt) 0.6 reaction on (sample exposed) plunger lowered plunger lowered 0.5 N2O5 0.4 0.3 0.2 gas phase NO production 0.1 NOy 0.0 200 400 600 time (s) 800 1000 soot renoxificatio n NOx = NO + NO2 0.7 MS Signal (Volt) NOy 0.5 plunger lowered reaction on (sample exposed) plunger lowered 0.6 N2O5 on 10 mg of grey soot N2O5 0.4 0.3 0.2 gas phase NO2 production 0.1 0.0 0 200 400 600 800 time (s) 1000 1200
  • 24. Soot is a potential source of tropospheric HONO NO 2 + soot(grey) → HONO + products NO3 reaction on soot NO + products Heterogeneous reactions (NO3 + NO2) reaction on soot (grey) HONO formation
  • 25. Heterogeneous interaction of trace gases on substrates of technological importance: inkjet print paper Samples: Polyester + AlOOH or SiO2 + Dye + additives Fading effect 5 Torr NO2 1 Torr NO2
  • 26. Acknowledgment  M.J. Rossi  Hubert Van den Bergh  MINATROC project  OFES foundation  ILFORD Imaging GmbH (CH)  Maria S.  Cristina  Flavio Comino Thanks

Editor's Notes

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