210 likes | 308 Vues
Explore the intricacies of solar radiation, thermal nomenclature, and atmospheric interactions for Earth science studies. Topics include blackbody curves, Doppler broadening, and radiative transfer equations. Enhance your knowledge of remote sensing techniques and radiative heating profiles with detailed explanations and applications.
E N D
Monday, Oct. 2: Clear-sky radiation; solar attenuation, Thermal nomenclature
Sun Earth Y-axis: Spectral radiance, aka monochromatic intensity units: watts/(m^2*ster*wavelength) Blackbody curves provide the envelope to Sun, earth emission
Sun Earth visible
Depth of penetraion into earth’s atmosphere of solar UV 1 Angstrom= 10-10 m. Photoionization @ wavelengths < 0.1 micron (1000 angstroms) Photodissociation @ wavelengths < 0.24 microns: O2 -> 2O Ozone dissociation @wavelengths < 0.31 micron Visible spectrum 0.39 to 0.76 micron
Thermal Radiation: • scattering negligible • absorption,emission is what matters • Math gets complicated: thousands of absorption lines, each • varying individually with pressure, temperature Natural Doppler broadening: Half-width goes as T1/2 Lorentz (Pressure) broadening: Half-width goes as P/T(0.5-1.0) natural absorption < 20 km, pressure broadening > 50 km Doppler broadening (Freq shift)/half-width
Continuing efforts to improve database on line absorption strengths and Halfwidths: H20 continuum, Microwave lines, are examples 16 micron 7 micron
Thermal Radiation transmits through an atmospheric layer According to: +J ds emission • I = intensity • = air density r = absorbing gas amount k =mass extinction coeff. rk = volume extinction coeff. Path length ds Inverse length unit Extinction=scattering+absorption ~ 0
Langley plot T = e-sec Ln (Iinf/I) =sec Beer’s Law used to assess solar constant in pre-satellite days, now used to calibrate instrumentation & determine aerosol&cloud optical depth from ground
Transmission through a layer, ignoring scattering and emission: dI = -I kabs sec dz After integration: T = e-sec Beer’s Law or Lambert’s Law T = transmissivity; = optical depth, or thickness Consequence: most radiation is absorbed/emitted at an optical depth of 1.
brightening Limb Effects darkening affects ALL terrestrial remote sensing
Limb Sounding as a Remote Sensing Technique: • first get the temperature from Planck function radiance • then use radiance in an absorbing/emitting wavelength • to get atmospheric concentration at that height HIRDLS
To calculate the broadband infrared emission, One simplification is to group lines together, Use spectral-band-average values for absorption - “band” models. A more elegant solution is to group lines by their absorption lines strengths, and integrate over that. Only works in infrared
Full radiative transfer equation for infrared/microwave (I.e. ignores scattering): attenuation emission Plane-parallel approximation: the earth is flat. -> the temperature, atmospheric density is a function of height (or pressure) alone. Curvature of earth ignored, atmosphere assumed to be horizontally homogeneous. Flux density with “flux transmissivity”
Radiative heating rate profiles: -or- Cooling to space approximation: Ignore all intervening layers Manabe & Strickler, 1965 Rodgers & Walshaw, 1966, QJRMS
Remote temperature sensing • CO2 particularly suited (well-mixed & emissive) (what part of the Earth is this from ?)
If scattering is also included: • 3 radiatively-important • scatterer parameters: • optical depth (how much stuff • Is there ?) • single-scattering albedo ksca/(kscat + kabs) (how much got • Scattered rather than absorbed ?) • asymmetry parameter g, or phase function P(cos : • (describe how it scatters)
Wednesday: • results from top of atmosphere radiation • Balance • questions up to 4.40 • some other aerosol, greenhouse gas, • results
Whether/how solar radiation scatters when it impacts gases,aerosols,clouds,the ocean surface depends on 1. ratio of scatterer size to wavelength: Size parameter x = 2*pi*scatterer radius/wavelength Sunlight on a flat ocean Sunlight on raindrops X large X small Scattering neglected IR scattering off of air, aerosol Microwave scattering off of clouds Microwave (cm)