CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING IS NEGLIGIBLE Key Concepts: Infrared.

Slides:



Advertisements
Similar presentations
METO621 Lesson 18. Thermal Emission in the Atmosphere – Treatment of clouds Scattering by cloud particles is usually ignored in the longwave spectrum.
Advertisements

Electromagnetic Radiation Electromagnetic Spectrum Radiation Laws Atmospheric Absorption Radiation Terminology.
Radiative Properties of Clouds SOEE3410 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds Cloud microphysics.
Atmospheric Emission.
Lecture 5: Radiative transfer theory where light comes from and how it gets to where it’s going Wednesday, 19 January 2010 Ch 1.2 review, 1.3, 1.4
Radiative Properties of Clouds ENVI3410 : Lecture 9 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds.
METR180: Remote Sensing Lecture 14 – On Water Vapor.
Handout (yellow) Solar Energy and the Atmosphere Standard 3 Objective 1 Indicators a, b, and c Standard 3 Objectives 1, 2, and 3 Workbook Pages 3,
Quick Review of Remote Sensing Basic Theory Paolo Antonelli CIMSS University of Wisconsin-Madison South Africa, April 2006.
Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.
Pat Arnott, ATMS 749 Atmospheric Radiation Transfer Chapter 6: Blackbody Radiation: Thermal Emission "Blackbody radiation" or "cavity radiation" refers.
Quick Review of Remote Sensing Basic Theory Paolo Antonelli CIMSS University of Wisconsin-Madison Benevento, June 2007.
Radiation: WHY CARE ??? the ultimate energy source, driver for the general circulation usefully applied in remote sensing (more and more)
Fourier Transform Infrared (FTIR) Spectrometer Subhashree Mishra ATMS Grad Student, UNR W. P. Arnott Physics, UNR Introduction to Atmospheric Instrumentation.

The Greenhouse Effect A quick review. The Greenhouse Effect A natural process that keeps the surface of the earth at a habitable temperature. A natural.
Radiation in the Atmosphere (Cont.). Cloud Effects (2) Cloud effects – occur only when clouds are present. (a) Absorption of the radiant energy by the.
Pat Arnott, ATMS 749, UNR, PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING IS NEGLIGIBLE From Grant Petty’s.
Measurement of Thermal Infrared Radiation Emitted by the Atmosphere Using FTIR Spectroscopy By Narayan Adhikari Charles Woodman 5/11/2010 PHY 360.
Physics of the Atmosphere II
Monday, Oct. 2: Clear-sky radiation; solar attenuation, Thermal nomenclature.
ATMOSPHERE HEATING RATE: CLOUD FREE ATMOSPHERE. Words and Equation from Petty: Radiative Heating Rate.
Lecture 5: Radiative transfer theory where light comes from and how it gets to where it’s going Tuesday, 19 January 2010 Ch 1.2 review, 1.3, 1.4
Pat Arnott, ATMS 749, UNR, 2008 CH 8: ATMOSPHERIC EMISSION: PRACTICAL CONSEQUENCES OF THE SCHWARZSCHILD EQUATION FOR RADIATION TRANSFER WHEN SCATTERING.
Please read Chapter 4 in Archer Textbook
Lecture 3: Radiation and Earth’s Atmosphere EarthsClimate_Web_Chapter.pdfEarthsClimate_Web_Chapter.pdf, p. 1-5 For more advanced reading materials, please.
The Greenhouse Effect - Atomic level By Kaelin O’Hare.
Energy in the Atmosphere Chapter 16 Section 1 Pages Chapter 16 Section 1 Pages
1 Atmospheric Radiation – Lecture 9 PHY Lecture 9 Infrared radiation in a cloudy atmosphere.
Blackbody Radiation/ Planetary Energy Balance
1 Atmospheric Radiation – Lecture 13 PHY Lecture 13 Remote sensing using emitted IR radiation.
Quick Review of Remote Sensing Basic Theory Paolo Antonelli SSEC University of Wisconsin-Madison Monteponi, September 2008.
Atmosphere-ocean interactions Exchange of energy between oceans & atmosphere affects character of each In oceans –Atmospheric processes alter salinity.
Energy, heat, and absorption Scripps Classroom Connection
MET 4430 Physics of Atmospheres Lecture 4 More Radiation 28 SEP-08 OCT 2012.
ECMWF/EUMETSAT NWP-SAF Satellite data assimilation Training Course
Unit 9 Section 2: Solar Energy and the Atmosphere
Planetary Energy Budget
Sun's Energy & Climate Change climate notes page 3.
Infrared Spectroscopy of the Atmosphere using the FTIR Spectrometer
The Enhanced Greenhouse Effect
Atmosphere Section 1: Atmospheric Basics
BAESI - Global Warming: Food Climate Connections
climate notes page 3 Sun's Energy & Climate Change
The Greenhouse Effect 8.6 The greenhouse effect is a natural process whereby gases and clouds absorb infrared radiation emitted by Earth’s surface and.
Greenhouse Effect and Global Warming
Winds in the Polar Regions from MODIS: Atmospheric Considerations
Sun's Energy & Climate Change climate notes page 3.
Global Warming Topic 8.5.
Natural and Unnatural Greenhouse Effect
Solar Energy and the Atmosphere
Greenhouse Effect 2.6.2B EXPLAIN THE CONCEPT OF THE GREENHOUSE EFFECT INCLUDING A LIST OF SPECIFIC GREENHOUSE GASES AND WHY CO2 IS MOST OFTEN THE FOCUS.
Fourier Transform Infrared (FTIR) Spectrometer
Radiation in the Atmosphere
climate notes page 3 Sun's Energy & Climate Change
Downwelling Spectral Solar Irradiance and IR Radiance Measurements ATMS 360 Spring 2008 Preliminary Results.
ATMOSPHERE OBJECTIVE 1 1.What are the structural components of the
Radiation in the Atmosphere
CH 3: The Electromagnetic Spectrum
Chapter 11: The Radiative Transfer Equation with Scattering
Section 2: Solar Energy and the Atmosphere
Climate, Energy, and Earth
By Narayan Adhikari Charles Woodman
Introduction and Basic Concepts
Chapter 9: Absorption by Atmospheric Gases
Solar Energy to Earth and Seasons
Radiation Energy from the sun
AIRS (Atmospheric Infrared Sounder) Level 1B data
Chapter 17 Chapter Review
Seasonality and the Greenhouse Effect
Presentation transcript:

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.

Some Energy States of Water Molecules http://www.lsbu.ac.uk/water/vibrat.html http://en.wikipedia.org/wiki/Libration

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? Gas concentrations from ‘typical’ midlatitude summer atmosphere. 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.

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

Optics of N identical (particles / volume) Light beam area = A z dz z+dz Power removed in dz: = I(z) N A dz ext Bouger-Beer “law” (direct beam only!)

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?

FTIR Radiance: Atmospheric IR Window 13 microns 8 microns

DEFINITION OF THE BRIGHTNESS TEMPERATURE TB Measured Radiance at wavenumber v = Theoretical Radiance of a Black Body at temperature TB

FTIR Brightness Temperatures

Atmosphere Emission Measurements, Downwelling Radiance Notes: Wavelength range for CO2, H20, O3, CH4. Envelope blackbody curves. Monster inversion in Barrow. Water vapor makes the tropical window dirty.

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

emissivity=absdz/cos B[T(z)] q blackbody radiance, T = temperature. Downwelling Intensity Emitted by the Atmosphere to the Detector (Radiance) =cos z dz emissivity=absdz/cos B[T(z)] q blackbody radiance, T = temperature. q ftir emission transmission weighting function

Weighting Functions for Satellite Remote Sensing using the strong CO2 absorption near 15.4 um. (from Wallace and Hobbs, 2nd edition)

Chapter 8 Homework: 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). Explain in detail, using these weighting function, how we can diagnose the temperature inversion in the Barrow Alaska graph. Bring questions to class related to how this is done. 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.)

Simple Theory for W(z) at the Ground Where is the HUGE approximation? Why?

Simple Theory for W(z) at the Ground Where is the HUGE approximation? Why?

http://www.spectralcalc.com/calc/spectralcalc.php volume mixing ratio = 0.01 (CO2) = 0.1 (others)

http://www.spectralcalc.com/calc/spectralcalc.php Can save text file! volume mixing ratio = 0.01 (CO2)

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

CO2 Spectrum: Line Strength and Broadening Effects

CO2 Spectrum: Line Strength and Broadening Effects

abs0, P=1013.25 mb, T=296 K. ONLY CO2!!! =0.5 cm-1. 380 ppm CO2

Calculate abs(z) depth. http://www.spectralcalc.com/atmosphere_browser/atmosphere.php Calculate N(z), then NH20(z), Nco2(z), etc. Calculate abs(z) depth. Calculate W(z)

RENO FTIR SPECTRA

Weighting Functions for the FTIR at the Ground Looking Up H=6 km

Weighting Functions for the FTIR at the Satellite Looking Down H=6 km

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

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

Which day is more moist? Which day is warmer near the surface? RENO FTIR SPECTRA

Coincident FTIR Measurements, Down and Up.

More Examples of FTIR Data from a Satellite

Comments on Figure 8.3. The very strong CO2 line at 15 microns typically gives the gas temperature closest to the FTIR spectrometer.

Self Study Questions

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).

Atmospheric Temperature Profile: US “Standard” Atmosphere. Cirrus cloud level. High cold clouds, visible optical depth range 0.001 to 10, emits IR to surface in the IR window. From Liou

Cirrus Clouds: Small Crystals at Top, -40 C to -60 C nucleation Growth and fall Evaporation

IR Atmospheric window region 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.

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.

Skin Depth and Absorption Efficiency

Cloud Emissivity in General and Zero Scattering Approximation.

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.

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.

Cirrus with Small Crystals IR Emission Model

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.