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Connecting atmospheric composition Connecting atmospheric composition

Connecting atmospheric composition - PowerPoint Presentation

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Connecting atmospheric composition - PPT Presentation

with climate variability and change Seminar in Atmospheric Science EESC G9910 Diagnosing ENSO from atmospheric composition ozone measured from space Ziemke et al 2010 Oman et al 2011 ID: 168367

mol atmospheric global climate atmospheric mol climate global jacob forcing ch4 air gases species radiative daniel time atmosphere burden change gas lifetime

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Slide1

Connecting atmospheric composition with climate variability and change Seminar in Atmospheric Science, EESC G9910

Diagnosing ENSO from atmospheric composition (ozone measured from space)

Ziemke

et al

., 2010;

Oman et al

., 2011

To be discussed

Week 4Slide2

Course InformationTwo motivating questions:How does climate variability (and change) influence distributions of trace species in the troposphere?How do changes in trace species alter climate?Email me by Monday Sept 10:

a) to sign up for presentation:

amfiore

@

ldeo.columbia.edu

b) Credit options:

1 point (discussion only)

2 points (discussion + presentation)

Weekly readings at

www.ldeo.columbia.edu

/~

amfiore

/eescG9910.htmlSlide3

Today’s OutlineOverview of composition-climate interactionsIntro to key concepts a. Units of atmospheric composition b. Budgets / Lifetimes c. Radiative ForcingSlide4

Big Issues in Atmospheric Chemistry

LOCAL

< 100 km

REGIONAL

100-1000 km

GLOBAL

> 1000 km

Urban smog

Point source

Disasters

Visibility

Regional smog

Acid rain

Ozone

layer

Climate

Biogeochemical cycles

Daniel JacobSlide5

From Brasseur & Jacob,Ch2, draft chapterJan 2011 version; Text in prepSlide6

Air pollutants affect climate; changes in climate affect global atmospheric chemistry (and regional air pollution)NMVOCsCO, CH4

NO

x

pollutant sources

+

O

3

+

OH

H

2

O

Black carbon

Sulfate

organic carbon

T

T

Aerosols interact with sunlight

“direct” + “indirect” effects

Surface of the Earth

Greenhouse gases

absorb infrared radiation

T

atmospheric cleanser

Smaller droplet size

clouds last longer

increase

albedo

 less precipitation

A.M. FioreSlide7

Climate (change) affects chemistry (and air quality)

sources

strong

mixing

(1)

Transport / mixing (e.g., distribution of trace species)

Exchange with stratosphere

(3) Chemistry responds to changes in temperature, humidity

NMVOCs

CO, CH

4

NO

x

+

O

3

+

OH

H

2

O

PAN

(2) Emissions (biogenic, lightning NO

x

, fires)

VOCs

Planetary boundary layer

tropopause

A.M. FioreSlide8

1.1 Mixing ratio or mole fraction CX [mol mol-1]

remains constant when air density changes

e

robust measure of atmospheric composition

SPECIES

MIXING RATIO

(dry air)

[mol

mol

-1

]

Nitrogen (N

2

)

0.78

Oxygen (O

2

)

0.21

Argon (Ar)

0.0093

Carbon dioxide (CO

2

)

380x10

-6Neon (Ne)

18x10-6

Ozone (O3)(0.01-10)x10-6

Helium (He)

5.2x10

-6

Methane (CH

4)

1.7x10-6Krypton (Kr)

1.1x10-6

Trace

gases

Air also contains variable H

2

O vapor (10

-6

-10

-2

mol mol

-1

) and aerosol particles

Trace gas concentration units:

1 ppmv = 1 µmol mol

-1

= 1x10

-6

mol mol

-1

1 ppbv = 1 nmol mol

-1

= 1x10

-9

mol mol

-1

1 pptv = 1 pmol mol

-1

= 1x10

-12

mol mol

-1

Daniel JacobSlide9

1.2 Number density nX [molecules cm-3]

Proper measure for

reaction rates

optical properties of atmosphere

Proper measure for absorption or scattering of radiation by atmosphere

n

X

and

C

X

are related

by the ideal gas law:

Also define the mass concentration (g cm

-3

):

n

a

= air density

A

v

= Avogadro

’s numberP = pressureR = Gas constantT = temperature

MX= molecular mass of XDaniel JacobSlide10

ATMOSPHERIC BUDGET TERMS GLOBAL SOURCE: emissions, in situ production (Tg yr-1)

 well-known for some (well-documented) synthetic gases

GLOBAL SINK: chemical destruction, photolysis, deposition (

Tg

yr

-1

)

ATMOSPHERIC BURDEN: total mass (

Tg

) integrated over the atmosphere  Well known (measurements) for long-lived (well-mixed) gases  Poorly constrained for short-lived species TREND: difference between sources and sinks (Tg yr-1)

More detail: TAR 4.1.3 Slide11

Recent trends in well-mixed GHGshttp://www.esrl.noaa.gov/gmd/aggi/Slide12

More than half of global methane emissions

are influenced by human activities

~300 Tg CH

4

yr

-1

Anthropogenic [EDGAR 3.2 Fast-Track 2000;

Olivier et al

., 2005]

~200 Tg CH

4

yr

-1 Biogenic sources [Wang et al., 2004] >25% uncertainty in total emissions

ANIMALS

90

LANDFILLS +

WASTEWATER

50

GAS + OIL

60

COAL

30

RICE 40

TERMITES

20WETLANDS180

BIOMASS BURNING + BIOFUEL 30GLOBAL METHANE

SOURCES (Tg CH4 yr-1)

PLANTS?

60-240 Keppler et al., 2006

85 Sanderson et al., 2006

10-60 Kirschbaum et al., 2006

0-46 Ferretti et al., 2006

Clathrates?

Melting permafrost?

A.M. FioreSlide13

LifetimesAtmospheric Lifetime: Amount of time to replace burden (turnover time) t (yr) = burden (Tg

) / mean global sink (Tg yr

-1

)

for a gas in steady-state (unchanging burden; sources = sinks

Convenient scale factor:

(1) constant emissions (

Tg

/yr)  steady-state burden (Tg) (2) emission pulse (Tg)  time integrated burden of that pulse (Tg/yr)Perturbation (

e-folding) Time – can differ from the atmospheric steady-state lifetime  only equal to atmospheric lifetime for gases with constant chemical lifetime (e.g., Rn, radioactive decay)  Chemical feedbacks (e.g., CH4: more CH4, longer CH4 lifetime; N2O: more N2O, shorter lifetimeLifetimes can vary spatially and temporally -- species with lifetimes shorter than mixing time scales (< 1 year)(TAR 4.1.4)Slide14

TIME SCALES FOR HORIZONTAL TRANSPORT(TROPOSPHERE)

2 weeks

1-2 months

1-2 months

1 year

c/o Daniel JacobSlide15

TYPICAL TIME SCALES FOR VERTICAL MIXING

0 km

2 km

1 day

planetary

boundary

layer

tropopause

5 km

(10 km)

1 week

1 month

10 years

c/o Daniel JacobSlide16

Radiative Forcing (RF): A convenient metric for comparing climate responsesto various forcing agentsRF = Change in net (down-up) irradiance (radiative flux) at the tropopause

due to a perturbation to an atmospheric constituent

D

T

s

=

l *

RF

Climate

s

ensitivityparameterGlobal, annual mean change in surface T in responseto RF (equilibrium)Why is this convenient/useful ? First order estimate, best for LLGHGsRelatively easy to calculate (as opposed to climate response)Related to global mean equilibrium T change at surface:Slide17

uv

vis

near-ir

longwave

Methane

Nitrous oxide

Oxygen; Ozone

Carbon dioxide

Water vapor

Solar

blackbody

fn.

Earth’s

“effective”

blackbody fn.

CFCs

Clouds,

Aerosols

active

throughout

spectra

c/o V. RamaswamySlide18

IR Transmission/Absorption in/near atmospheric windowFrom Jan 2012 version Ch 5 of Brasseur & Jacob textbook in prepSlide19

Radiative Forcing: Analytical expressions for Well-mixed GHGsFrom IPCC TAR CH6, Table 6.2http://www.esrl.noaa.gov/gmd/aggi/Slide20

Radiative Forcing (RF): comparison of calculation methodologiesFigure 2.2, WG1 IPCC AR-4 Chapter 2, Section 2.2Slide21

Radiative forcing of climate (1750 to present):Important contributions from non-CO2 species

IPCC,

2007Slide22

Global Warming PotentialsRadiative forcing does not account for different atmospheric lifetimes of forcing agentsGWP attempts to account for this by comparing the integrated RF over a specified period (e.g. 100 years) from a unit mass pulse emission, relative to CO2.Slide23

WHAT IS THE ATMOSPHERE?

Gaesous envelope surrounding the Earth

Mixture of gases, also contains suspended solid and liquid particles (

aerosols)

Aerosol = dispersed condensed phase suspended in a gas

Aerosols are the

visible

components of the atmosphere

The atmosphere seen from space

Pollution off U.S. east coast

Dust off West Africa

California fire plumes

Daniel JacobSlide24

ATMOSPHERIC GASES ARE “VISIBLE” TOO…IF YOU LOOK IN THE UV OR IR

Nitrogen dioxide (NO

2

) observed by satellite in the UV

Daniel Jacob