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Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING IS NEGLIGIBLE Key Concepts: • Infrared transmission and emission by the atmosphere gases. • Learn how to read meteorology in infrared spectra. • Learn about the basic concepts involved with retrieval of atmospheric temperature and humidity - weighting functions.
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Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

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Page 1: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD

EQUATION FOR RADIATION TRANSFER WHEN SCATTERING IS NEGLIGIBLE

Key Concepts:

• Infrared transmission and emission by the atmosphere gases.

• Learn how to read meteorology in infrared spectra.

• Learn about the basic concepts involved with retrieval of atmospheric temperature and humidity - weighting functions.

Page 2: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Some Energy States of Water Molecules

http://www.lsbu.ac.uk/water/vibrat.html

http://en.wikipedia.org/wiki/Libration

Page 3: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Atmospheric Transmission: Beer’s Law: I(x)=I0e(-abs x)

What are the main sources for each gas?

Which gases are infrared active and contribute to greenhouse warming?

Which gases significantly absorb solar radiation?

Nitrous oxide is emitted by bacteria in soils and oceans, and thus has been a part of Earth's atmosphere for eons. Agriculture is the main source of human-produced nitrous oxide: cultivating soil, the use of nitrogen fertilizers, and animal waste handling can all stimulate naturally occurring bacteria to produce more nitrous oxide. The livestock sector (primarily cows, chickens, and pigs) produces 65% of human-related nitrous oxide. [1] Industrial sources make up only about 20% of all anthropogenic sources, and include the production of nylon and nitric acid, and the burning of fossil fuel in internal combustion engines. Human activity is thought to account for somewhat less than 2 teragrams of nitrogen oxides per year, nature for over 15 teragrams.

Gas concentrations from ‘typical’ midlatitude summer atmosphere.

Page 4: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Clouds at Visible and IR (e.g. 10 um) Wavelengths

Page 5: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Optics of N identical (particles / volume)

Light beam area = A

dz

z

z+dz

Power removed in dz: = I(z) N A dz ext

Bouger-Beer“law”(direct beam only!)

Page 6: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD

EQUATION FOR RADIATION TRANSFER WHEN SCATTERING IS NEGLIGIBLE

What process subtracts radiation?What process adds radiation?

What equation is used to calculate optical depth for a gaseous atmosphere?

Page 7: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

FTIR Radiance: Atmospheric IR Window

13 microns 8 microns

Page 8: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

DEFINITION OF THE BRIGHTNESS TEMPERATURE

TB

Measured Radiance at wavenumber v =Theoretical Radiance of a Black Body at temperature TB

Page 9: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

FTIR Brightness Temperatures

Page 10: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Atmosphere Emission

Measurements, Downwelling

Radiance

Notes:

1. Wavelength range for CO2, H20, O3, CH4.

2. Envelope blackbody curves.

3. Monster inversion in Barrow.

4. Water vapor makes the tropical window dirty.

Page 11: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Ideal Weighting Function Wi: Where in the atmosphere the main contribution to the radiation at wavenumber i

comes from.

Page 12: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Downwelling Intensity Emitted by the Atmosphere to the Detector (Radiance)

z dz

ftir

emissivity=absdz/cos

=cos

B[T(z)]

blackbody radiance,T = temperature.

emission transmission

weightingfunction

Page 13: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Weighting Functions for Satellite Remote Sensing using the

strong CO2 absorption near 15.4 um. (from Wallace and Hobbs,

2nd edition)

Ii =B(Ts)exp−τ absAll Atmos

( ) (surface)

+ B[T(z)]exp(−τabs(z))0

∫ abs(z)dz (atmos)

or

I i =B(Ts)exp−τ absAll Atmos

( ) (surface)

+ B[T(z)]0

∫ Wi(z)dz (atmos)

TeB(Te)

Satellite with FTIR Looking Down

Page 14: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Chapter 8 Homework:

1. Calculate and plot weighting functions as in the previous slide, but for the FTIR spectrometer at the ground looking up.(500 to 850 cm-1 region).

2. Explain in detail, using these weighting function, how we can diagnose the temperature inversion in the Barrow Alaska graph.

3. Bring questions to class related to how this is done.

4. Extra credit: Calculate and plot weighting functions for the stratospheric ozone emission spectral region in the atmospheric window region (spectral region between 1000 and 1100 cm-1.)

Page 15: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Simple Theory for W(z) at the Ground

Where is theHUGEapproximation?Why?

Page 16: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Simple Theory for W(z) at the Ground

Where is theHUGEapproximation?Why?

Page 17: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

http://www.spectralcalc.com/calc/spectralcalc.php

volume mixing ratio = 0.01 (CO2) = 0.1 (others)

Page 18: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

http://www.spectralcalc.com/calc/spectralcalc.php

volume mixing ratio = 0.01 (CO2)

Can save text file!

Page 19: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Calculate the absorption cross section per molecule from the transmittance calculations and this theory.

Page 20: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

CO2 Spectrum: Line Strength and Broadening Effects

Page 21: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

CO2 Spectrum: Line Strength and Broadening Effects

Page 22: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

abs0, P=1013.25 mb, T=296 K. ONLY CO2!!! =0.5 cm-1.

380 ppm CO2

Page 23: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

http://www.spectralcalc.com/atmosphere_browser/atmosphere.php

Calculate N(z), thenNH20(z), Nco2(z), etc.

Calculate abs(z) depth.

Calculate W(z)

Page 24: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

RENO FTIR SPECTRA

Page 25: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Weighting Functions for the FTIR at the Ground Looking Up

H=6 km

Page 26: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Weighting Functions for the FTIR at the Satellite Looking Down

H=6 km

Page 27: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Theoretical Absorption Cross Sections for the indicated gases, averaged to 1 cm -1 resolution for clarity.

Page 28: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Theoretical Absorption Cross Sections for the indicated gases, averaged to 1 cm -1 resolution for clarity.

Page 29: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

RENO FTIR SPECTRA

Which day is more moist?

Which day is warmer near the surface?

Page 30: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Coincident FTIR Measurements, Down

and Up.

Page 31: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

More Examples of FTIR Data from a Satellite

Page 32: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Comments on Figure 8.3.

The very strong CO2 line at 15 microns typically gives the gas temperature closest to the FTIR spectrometer.

Page 33: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Self Study Questions

Page 34: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

FTIR Data from the NASA ER2 with Responsible Gases labeled.

IR Window 8-13 microns. IR radiation from

the Earth’s surface escapes

to space (cooling the

Earth). Absorption by

O3 near 9 microns ‘dirties’

the window.

(From Liou, pg 120).

Page 35: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Atmospheric Temperature Profile: US “Standard” Atmosphere.

From Liou

Cirrus cloud level.High cold clouds, visible optical depth range0.001 to 10, emits IR to surface in the IR window.

Page 36: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Cirrus Clouds: Small Crystals at Top, -40 C to -60 C

nucleation

Growth and fall

Evaporation

Page 37: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

FTIR Data from the NASA ER2, Clear and Cloudy Sky. (From Liou’s book). The ice cloud with small ice crystals has emissivity << 1, so the

ground below is partially seen. Clouds reduce the IR making it to space in the atmospheric

window region.

IR Atmospheric window region

Page 38: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Ice Refractive

Index

Red shows the atmospheric window region. The resonance in the window region is useful for remote sensing. The real part goes close to 1, making anomalous diffraction theory a fairly reasonable approach for cross sections.

Page 39: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Skin Depth and Absorption Efficiency

Page 40: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Cloud Emissivity in General and Zero Scattering Approximation.

CLOU

CLOUD

I0 Incident Irradiance

I0 tTransmittedIrradiance

L=

DirectBeam

Diffuse+

1 D ideas....

I0 rReflectedIrradiance

GENERAL CLOUD MODELTRANSMITTED≡I0 tTRANSMITTED=Direct+DiffuseDirectBeam=I0exp(−extL)

Diffuse=I0 t−exp(−extL)⎡

⎢⎢

⎥⎥

REFLECTED≡I0 r

Absorptivity(a)=Emissivity(e)e=1−t−r=a

ZeroScattering(gas)CloudModelt=exp(−absL)e=1−t

Page 41: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Cirrus with Small Crystals IR Transmission Model

Message: Curve has basic shape of the IR spectrum for small cirrus, primarily a transmission problem of ground radiance through the cloud, with a small emission correction. ASSUMES ZERO SCATTERING.

Page 42: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Cirrus with Small Crystals IR Emission Model

Message: Curve has basic shape of the IR spectrum for small cirrus, primarily a transmission problem of ground radiance through the cloud, with a small emission correction.

Te

B(Te)

Cirrus Cloud

Satellite with FTIR Looking Down

B(Te) tc B(Tc) (1-tc)

Page 43: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

Cirrus with Small Crystals IR Emission Model

Te=300 KTcirrus=213 KCrystal D= 10 umCrystal Conc=10,000 / LiCloud Thickness = 1 km

Te

B(Te)

Cirrus Cloud

Satellite with FTIR Looking Down

B(Te) tc B(Tc) (1-tc)

Page 44: Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.

Pat Arnott, ATMS 749, UNR, 2008

IR Cooling Rates(from Liou)

Message:

Clouds are good absorbers and emitters of IR radiation. MLS is a moist midlatitude profile, SAW is a dry subarctic winter profile.

Cooling rate is from the vertical divergence of the net irradiance absorbed and emitted.

ρcp ∂T∂t=−dFnetdz