Pat arnott, atms 360 Radar: The Quickest Path to dbZ 1.Absorption, scattering and extinction cross sections. 2.Backscattering cross section. 3.Cross section.

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Presentation transcript:

pat arnott, atms 360 Radar: The Quickest Path to dbZ 1.Absorption, scattering and extinction cross sections. 2.Backscattering cross section. 3.Cross section in the Rayleigh limit (particle diameter is much smaller than the wavelength of the radiation.) 4.Radar cross section for a particle in the Rayleigh limit. 5.Radar cross section for N particles in the Rayleigh limit. Note: Key results are circled by a red box like this. The homework assignment is also given by a red box.

pat arnott, atms 360 Definitions: Optical Coefficients for a Flat Surface Sunlight I 0 (W/m 2 ) Arbitrary Surface Area A (m 2 ) a = albedo Absorptance=(1-a) Power Scattered, Power Absorbed P sca = I 0 A a P abs = I 0 A(1-a)  abs = (1-a) A Sunlight I 0 (W/m 2 ) Black Surface Area A (m 2 ) a = albedo = 0 Absorptance = (1-a) = 1 Power Scattered, Power Absorbed P sca = 0 P abs = I 0 A  abs = A

pat arnott, atms 360 Definitions: Optical Coefficients for a Surface and a Particle Beam of Sunlight I 0 (W/m 2 ) Power Removed From Beam I 0  ext = P ext I 0  abs = P abs I 0  sca = P sca Sunlight I 0 (W/m 2 ) Arbitrary Surface Area A (m 2 ) a = albedo Absorptance=(1-a) Power Scattered, Power Absorbed P sca = I 0 A a P abs = I 0 A(1-a)  abs = (1-a) A Thing (particle, molecule, flea, etc) Absorption, less light through thing. Scattering, light redirected by thing.  abs =(1-  )  ext

pat arnott, atms 360 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!)

pat arnott, atms 360 Monodispersons and Polydispersions N particles / volume. All of radius r. n r

pat arnott, atms 360 Radar Theory Part 1

pat arnott, atms 360 Radar Theory Part 2: Key Results!!! This is what is reported on radar graphs!!!

pat arnott, atms 360 Radar Theory Part 2: Typical Values of Z dbZ Clear air mode of NEXRAD: -28 dbZ to 28 dbZ. Precipitation mode of NEXRAD: 5 dbZ to 75 dbZ. Light rain: 20 dbZ.

pat arnott, atms 360 Rain Fall Rate for Monodispersion

pat arnott, atms 360 Radar Theory Part 3: Rainfall Rate Estimate From Radar Definition of rainfall rate and what happens after rain hits the surface. Rainfall rate depends on the mass of water droplets and their fall speed.

pat arnott, atms 360 Rainfall Rate Analogy Falling rain: Coffee is being poured at some rate. Height of coffee = H Rainfall Rate = Height of Coffee / time elapsed pouring it. Rainfall Rate = dH / dt

pat arnott, atms 360 Rain Drop Fall Speed

pat arnott, atms 360 Rain Drop Fall Speed: A balance of Forces, Drag and Gravity

pat arnott, atms 360 Fall Speed Is a Function of Size: Note the Shape in Terminal Flow

pat arnott, atms 360 Radar Theory Part 3: Rainfall Rate Estimate From Radar This is one relationship used to get rainfall rate (depth / time) from radar. Problem: People have developed many such relationships! Which is correct, if any?????

pat arnott, atms 360 W. P. Arnott, AAAR tutorial, Sept Definitions: Optical Coefficients for Particles Extinction coefficient for particle mono dispersions Extinction coefficient for particle dispersions Nebulized, dried Ammonium Sulfate 532 nm Sheridan, P. J., W. P. Arnott, J. A. Ogren, B. E. Anderson, D. B. Atkinson, D. S. Covert, H. Moosmuller, A. Petzold, B. Schmid, A. W. Strawa, R. Varma and A. Virkkula (2005). "The Reno aerosol optics study: Overview and summary of results." Aerosol Science & Technology 39: Slowik, Jay, G., Eben S. Cross, Jeong-Ho Han, Paul Davidovits,Timothy B. Onasch, John T. Jayne, Leah R. Williams, Manjula R. Canagaratna, Douglas R. Worsnop, Rajan K. Chakrabarty, Hans Moosmüller, William P. Arnott, Joshua P. Schwarz, Ru-Shan Gao, DavidW. Fahey, Gregory L. Kok, and Andreas Petzold (2007). An Inter- Comparison of Instruments Measuring Black Carbon Content of Soot Particles. Aerosol Science and Technology, 41:295–314, 2007.

pat arnott, atms 360 W. P. Arnott, AAAR tutorial, Sept Light Scattering Basics (images from Wallace and Hobbs CH4). Sphere, radius r, complex refractive index n=m r + im i x x x m r =1.5 QsQs Angular Distribution of scattered radiation (phase function) x x x Dipole scattering

pat arnott, atms 360 Polarization Diverse Radar: Coming to the NWS in the next few years. Radar sends out horizontally and vertically polarized pulses. Hydrometeors like raindrops are flattened. The horizontal cross sections are larger than the vertical. Therefore for large raindrops a the horizontal polarization backscatter amount is larger than the vertical amount. Hail stones are more symmetrical and have less polarization diversity.