Download presentation

1
**Microwave Interactions with the Atmosphere**

INEL 6069, Microwave Interactions with the Atmosphere Dr. Sandra Cruz Pol Microwave Remote Sensing INEL 6669 Dept. of Electrical & Computer Engineering, UPRM, Mayagüez, PR

2
**Atmosphere composition**

INEL 6069, Atmosphere composition Other components: Carbon dioxide (CO2), Neon (Ne), Helium (He), Methane (CH4), Krypton (Kr), Hydrogen (H2) and Water vapor (highly variable)

3
**Air Constituents in Troposphere and Stratosphere**

N %, O %, H2O 0-2% Inert gases 0.938% Many of the least abundant have a disproportionally large influence on atmospheric transmission. CO2 398ppm absorbs 2.8, 4.3 & 15 mm CH4 1.7ppm absorbs 3.3 & 7.8mm N2O .35ppm absorbs 4.5, 7.8 & 17mm O3 ~ absorbs UV-B, 9.6mm CFCl3, CF2CL2 … absorbs IR

4
Atm. CO2 Concentration Last 200 years

6
Methane

9
**H2O is less than 2% yet has great effect in climate & weather**

10
**Radiative Transfer in Atmosphere during Daytime**

INEL 6069, During daytime only. Nighttime is another story

11
**Atm. Gases & Electromagnetic propagation**

INEL 6069, Atm. Gases & Electromagnetic propagation Up to now, we have assumed lossless atm. For 1 GHz< f< 15 GHz ~lossless For higher frequencies, =>absorption bands H2O O2 GHz 183.3 GHz IR & visible 50-70GHz 118.7GHz IR & visible

12
**Outline I. The atmosphere: composition, profile**

INEL 6069, Outline I. The atmosphere: composition, profile II. Gases: many molecules 1. Shapes(G, VVW, L): below 100GHz, up to 300GHz we find interaction with H2O and O2 2. Total Atmospheric Absorption kg, opacity tq, and atm-losses Lq 3. TB: Downwelling Emission by Atmosphere Sky Temp= cosmic + galaxy

13
**U.S. Standard Atmosphere**

INEL 6069, U.S. Standard Atmosphere Thermosphere (or Ionosphere) oF! 95/120km Mesopause Mesosphere no aircrafts here too cold ~-90oF 50/60km Stratopause Stratosphere- no H2O or dust ozone absorption of UV warms air to ~40oF 8/15km Tropopause Troposphere – clouds, weather P= 1013 mbars = 1013 HPa T= 300K

14
**Atmospheric Profiles US Standard Atmosphere 1962**

INEL 6069, Atmospheric Profiles US Standard Atmosphere 1962 Temperature Density in kg/m3 Pressure P= nRT/V=rairRT/M or Poe-z/H3 or Rair= 2.87

15
INEL 6069, Water Vapor Profile Depends on factors like weather, seasons, time of the day. It’s a function of air temperature. Cold air can’t hold water Hot air can support higher humidities.(P dependence) rv(z)= roe-z/H [g/m3] where ro averages in mid latitudes and the total mass of water vapor in a column of unit cross section is

16
**Relative Humidity Dew point temperature (dew=rocío) Relative Humidity**

is the T below which the WV in a volume of humid air at a constant barometric P will condense into liquid water. Is the T as which fog forms Relative Humidity When Tair is close to Tdew => high %RH Absolute Humidity, the mass of water per unit volume of air.

17
Equations for RH Where e = pressure and exp means exponential ex

18
**Relative Humidity (RH) simplified equations**

T is in Celsius

19
**Relative Humidity, RH vapor in air**

INEL 6069, Relative Humidity, RH vapor in air Air Temperature T Vapor air can hold Actual Vapor in the air [gr per kg dry air] Relative humidity RH 86oF 27.6 10.83 39% 77oF 20.4 53% 68oF 14.9 72% 59oF 10.8 100%

20
**Relative Humidity, RH dew Temperature**

INEL 6069, Relative Humidity, RH dew Temperature Air Temperature T Dew Temperature Tdp Actual Vapor in the air [gr per kg dry air] Relative humidity RH 86oF 64oF 10.83 39% 77oF 60oF 53% 68oF oF 72% 59oF 100%

21
Quantum of energy INEL 6069,

22
**EM interaction with Molecules**

INEL 6069, EM interaction with Molecules Total internal energy state for a molecule electronic energy corresponding to atomic level vibration of atoms about their equilibrium position rotation of atoms about center of molecule E = Ee + Ev + Er Bohr condition f lm= (El – Em ) /h Values for energy differences for electronic: 2 to 10 eV vibrational-rotational: 0.1 to 2 eV pure rotational: 10-4 to 5 x 10-2 eV ( microwaves)

23
INEL 6069, Aviris Visible and IR

24
**Line Shapes where, Slm is the line strength F(f,flm) is the line shape**

INEL 6069, Line Shapes where, Slm is the line strength F(f,flm) is the line shape LINE SHAPES Lorentz Gross Van-Vleck-Weisskopt One molecule frequency Absorption Many molecules: pressure broaden* frequency *caused by collision between molecules

25
**Line shapes Lorentz Gross Van-Vleck-Weisskopt Liebe MPM model for**

INEL 6069, Line shapes Lorentz Gross Van-Vleck-Weisskopt Liebe MPM model for Millimeter wave propagation model

26
**Absorption Bands Mainly water and oxygen for microwaves**

INEL 6069, Absorption Bands Mainly water and oxygen for microwaves Brightness Temperature [K] Frequency [GHz]

27
**Note how line width changes with height due to less pressure broadening**

29
**Total Atmospheric Absorption kg, Opacity tq, [Np] Loss factor Lq**

INEL 6069, Total Atmospheric Absorption kg, Opacity tq, [Np] Loss factor Lq [L en dB] To convert from Np/km to dB/km multiply by for 1-way propagation

30
**Atmospheric Emission For clear atmosphere where**

INEL 6069, Atmospheric Emission For clear atmosphere where Also there is some background radiation Tcos=2.7K from the Big Bang and Tgal~0 above 5GHz

31
**Latent Heat – to understand radiation budget need to monitor water content in atmosphere**

Radiative Transfer, INEL 6069,

32
**Scattering from Hydrometeors: Clouds, Snow, Rain**

33
**Outline: Clouds & Rain Single sphere (Mie vs. Rayleigh)**

Sphere of rain, snow, & ice (Hydrometeors) Find their ec, nc, sb Many spheres together : Clouds, Rain, Snow a. Drop size distribution b. Volume Extinction= Scattering+ Absorption c. Volume Backscattering Radar Equation for Meteorology TB Brightness by Clouds & Rain

34
**Clouds Types on our Atmosphere**

35
**Sizes for cloud and rain drops**

36
**Cirrus Clouds Composition**

% Cirrus Clouds Composition

37
**EM interaction with Single Spherical Particles**

Absorption Cross-Section, Qa =Pa /Si Efficiency, xa= Qa /pr2 Scattered Power, Ps Cross-section , Qs =Ps /Si Efficiency, xs= Qs /pr2 Total power removed by sphere from the incident EM wave, xe = xs+ xa Backscatter, Ss(p) = Sisb/4pR2

38
**Mie Scattering: general solution to EM scattered, absorbed by dielectric sphere.**

Uses 2 parameters (Mie parameters) Size wrt. l : Speed ratio on both media:

39
**[Index of Refraction and Refractivity]**

The Propagation constant depends on the relative complex permittivity Where the index of refraction is But n’air≅1.0003 So we define N

40
**So… Propagation in terms of N is And the attenuation and phase is**

And the power density carried by wave traveling in the z-direction is : With f in GHz

41
**Mie Solution Mie solution**

Where am & bm are the Mie coefficients given by 8.33a to 8.33b in the textbook. Probl , menos 7,9,10,13 para jueves Abr10

42
Mie coefficients

43
**Mie Regions Cambio de regiones de acuerdo a razon de e’/e”**

Rayleigh region Intermediate or Mie region Optical region Rayleigh region Intermediate region Optical region Cambio de regiones de acuerdo a razon de e’/e” Example: sphere with e =3.2(1-j) Conclusion: regiones se definen de acuerdo a c y a n

44
**Intermediate or Mie region**

Backscattering Intermediate or Mie region Optical region Rayleigh region

45
**Variations of water dielectric const. with frequency and Temperature**

46
**Non-absorbing sphere or drop (n”=0 for a perfect dielectric, which is a non-absorbing sphere)**

Rayleigh region |nc|<<1

47
**Conducting (absorbing) sphere**

Optical region Rayleigh region Intermediate or Mie region c =2.4

48
Plots of Mie xe versus c Rayleigh Intermediate Optical Four Cases of sphere in air : n=1.29 (lossless non-absorbing sphere) n=1.29-j0.47 (low loss sphere) n=1.28-j1.37 (lossy dielectric sphere) n= perfectly conducting metal sphere As n’’ increases, so does the absorption (xa), and less is the oscillatory behavior. Optical limit (r >>l) is xe =2. Crossover for Hi conducting sphere at c =2.4 Weakly conducting sphere is at c =.06

49
**Rayleigh Approximation |nc|<<1**

Scattering efficiency Extinction efficiency where K is the dielectric factor

50
**Absorption efficiency in Rayleigh region**

i.e. scattering can be neglected in Rayleigh region (small particles with respect to wavelength) |nc|<<1

51
**Scattering from Hydrometeors**

Rayleigh Scattering Mie Scattering >> particle size comparable to particle size --when rain or ice crystals are present. 95GHz (3mm) 33GHz (9mm)

52
**Rayleigh Approximation for ice crystals**

Rayleigh scattering (λ >d) Mie scattering (λ ~ d)

54
**Single Particle Cross-sections vs. c**

Scattering cross section Absorption cross section In the Rayleigh region (nc<<1) =>Qa is larger, so much more of the signal is absorbed than scattered. Therefore For small drops, almost no scattering, i.e. no bouncing from drop since it’s so small.

55
**Gas molecules = much smaller than visible l=> Rayleigh approx. is OK.**

Red 700nm Violet 400nm

56
**Mie Scattering Mie scatt. is almost independent of frequency**

[l dependent] [almost l independent] Mie scatt. is almost independent of frequency Cloud droplets ~20mm compare to 500nm Microwaves have l~cm or mm (large) – Rayleigh for most atmospheric constituents Laser have l~nm - Mie

58
**Observe scattering in Visible EM; forward scattering vs. backscattering**

Mie scattering by dust particles and aerosols Rayleigh scattering by water vapor molecules and gases.

60
**Mie forward scattering nos impide ver bien a menos que haya alto contraste.**

61
Forward scattering

63
**Rayleigh-Mie-Geometric/Optics**

Along with absorption, scattering is a major cause of the attenuation of radiation by the atmosphere for visible. Scattering varies as a function of the ratio of the particle diameter to the wavelength (d/l) of the radiation. When this ratio is less than about one-tenth (d/l<1/10), Rayleigh scattering occurs in which the scattering coefficient varies inversely as the fourth power of the wavelength. At larger values of the ratio of particle diameter to wavelength, the scattering varies in a complex fashion described by the Mie theory; at a ratio of the order of 10 (d/l>10), the laws of geometric optics begin to apply.

64
**Mie Scattering (necessary if d/l1),**

Mie theory : A complete mathematical-physical theory of the scattering of electromagnetic radiation by spherical particles, developed by G. Mie in 1908. In contrast to Rayleigh scattering, the Mie theory embraces all possible ratios of diameter to wavelength. The Mie theory is very important in meteorological optics, where diameter-to-wavelength ratios of the order of unity and larger are characteristic of many problems regarding haze and cloud scattering. When d/l neither Rayleigh or Geometric Optics Theory applies. Need to use Mie. Scattering of radar energy by raindrops constitutes another significant application of the Mie theory.

65
**Backscattering Cross-section**

From Mie solution, the backscattered field by a spherical particle is Observe that perfect dielectric (nonabsorbent) sphere exhibits large oscillations for c>1. Hi absorbing and perfect conducting spheres show regularly damped oscillations.

66
**Backscattering from metal sphere**

Rayleigh Region defined as For conducting sphere Where,

67
**Scattering by Hydrometeors**

Hydrometeors (water particles) In the case of water, the index of refraction is a function of T & f. (fig 5.16) @T=20C For ice. For snow, it’s a mixture of both above.

68
**Liquid water refractivity, n’**

69
**Liquid water refractivity, n”**

70
Sphere pol signature Co-pol Cross-pol

71
**Mie Efficiency at 3GHz and 30GHz**

72
At 300GHz

74
**Snowflakes Snow is mixture of ice crystals and air**

The relative permittivity of dry snow The Kds factor for dry snow

75
**Volume Scattering Two assumptions:**

particles randomly distributed in volume-- incoherent scattering theory. Concentration is small-- ignore shadowing. Volume Scattering coefficient is the total scattering cross section per unit volume. [Np/m]

76
**Total number of drops per unit volume**

in units of mm-3 Drop size distribution in terms of radius or diameter Disdrometer- measures DSD

77
**pn(r) for Various Hydrometeors**

78
**Volume Scattering It’s also expressed as or in dB/km units, Using...**

[Np/m] [s,e,b stand for scattering, extinction and backscattering.] [dB/km]

79
**For Rayleigh approximation**

Substitute eqs. 41, 44 and 46 into definitions of the cross sectional areas of a scatterer. D=2r =diameter

80
**Noise in Stratus cloud image -scanning Ka-band radar**

81
**Volume extinction from clouds**

Total attenuation is due to gases,cloud, and rain cloud volume extinction is (eq.8.69) Liquid Water Content LWC or mv ) water density = 106 g/m3

82
**Relation with Cloud water content**

This means extinction increases with cloud water content. where and wavelength is in cm.

83
**Volume backscattering from Clouds**

Many applications require the modeling of the radar return. For a single drop [Eq and 8.78] For many drops (cloud)

84
**Reflectivity Factor, Z Is defined as so that**

and sometimes expressed in dBZ to cover a wider dynamic range of weather conditions. Z is also used for rain and ice measurements.

85
**Reflectivity in other books**

86
**Reflectivity & Reflectivity Factor**

h Z (in dB) Reflectivity, h [cm-1] dBZ for 1g/m3 Reflectivity and reflectivity factor produced by 1g/m3 liquid water Divided into drops of same diameter. (from Lhermitte, 2002).

87
**Cloud detection vs. frequency**

S Ka W

88
**Rain drops A) Raindrops are not tear-shaped, as most people think.**

B) Very small raindrops are almost spherical in shape. C) Larger raindrops become flattened at the bottom, like that of a hamburger bun, due to air resistance. D) Large raindrops have a large amount of air resistance, which makes them begin to become unstable. E) Very large raindrops split into smaller raindrops due to air resistance.

89
**Precipitation (Rain) Volume extinction [eq. 8.85-87]**

where Rr is rain rate in mm/hr [dB/km] and b are given by various model can depend on polarization since large drops are not spherical but ~oblong. [dB/km] Mie coefficients

90
**ke= specific extinction coeff.**

91
**W-band UMass CPRS radar**

92
Rain Rate [mm/hr] If know the rain drop size distribution, each drop has a liquid water mass of total mass per unit area and time rainfall rate is depth of water per unit time a useful formula

93
**Volume Backscattering for Rain**

For many drops in a volume, if we use Rayleigh approximation Marshall and Palmer developed but need Mie for f>10GHz.

94
**Rain retrieval Algorithms**

Several types of algorithms used to retrieve rainfall rate with polarimetric radars; mainly R(Zh), R(Zh, Zdr) R(Kdp) R(Kdp, Zdr) where R is rain rate, Zh is the horizontal co-polar radar reflectivity factor, Zdr is the differential reflectivity Kdp is the differential specific phase shift a.k.a. differential propagation phase, defined as

95
Raindrops symmetry Differential Reflectivity Zdr

96
**Snow extinction coefficient**

Both scattering and absorption ( for f < 20GHz --Rayleigh) for snowfall rates in the range of a few mm/hr, the scattering is negligible. At higher frequencies,the Mie formulation should be used. The is smaller that rain for the same R, but is higher for melting snow.

97
**Snow Volume Backscattering**

Similar to rain

98
**Radar equation for Meteorology**

For weather applications for a volume

99
Radar Equation For power distribution in the main lobe assumed to be Gaussian function.

100
**Radar Equation For calibrated target**

RcdB=radar constant (including atmospheric attenuation)

101
**These data sets provided information on the structure of precipitation systems.**

This was from Hurricane Georges passing over the Dominican Rep. while being ripped apart by tall mountains. Extremely strong convection is noted over the mountains that produced huge amounts of rainfall. EDOP flew in conjunction with radiometers. The combined radar/radiometer data sets was used to develop rain estimation algorithms for the Tropical Rainfall Measuring Mission (TRMM). The ER-2 Doppler Radar (EDOP) aboard the high-altitude ER-2 aircraft is a dual-beam 9.6 GHz radar to measure reflectivity and wind structure in precipitation systems.

Similar presentations

© 2019 SlidePlayer.com Inc.

All rights reserved.

To make this website work, we log user data and share it with processors. To use this website, you must agree to our Privacy Policy, including cookie policy.

Ads by Google