MET 4410 Remote Sensing: Radar and Satellite Meteorology MET 5412 Remote Sensing in Meteorology. Lecture 9: Reflection and Refraction (Petty Ch4)

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MET 4410 Remote Sensing: Radar and Satellite Meteorology MET 5412 Remote Sensing in Meteorology Lecture 9: Reflection and Refraction (Petty Ch4)

When to use the laws of reflection and refraction? EM waves incident on a planar (flat) boundary between two homogeneous mediums. Definition of homogeneous medium: the medium is smooth and uniform on scales comparable to the wavelength of the radiation, i.e., the size and spacing of the individual molecules and other irregularities are much smaller than the wavelength. Homogeneous medium examples: water, air, glass, etc. are all effectively homogeneous to radiation in visible, IR, and microwave band. Inhomogeneous medium examples: Milk for visible light Most objects (water, glass, milk, etc.) are inhomogeneous for x-rays and gamma rays. Clouds with 10 µm diameter droplets are homogeneous in microwave band, but inhomogeneous in IR and visible bands.

The complex index of refraction of a medium Definition: N= n r +i n i From a macroscopic point of view, all the complexity between radiation and media is hidden in N. For any substance, N is a function of wavelength, temperature, pressure, etc. The real part n r controls the phase speed of the EM wave through the medium. n r is defined as the ratio of the speed of light in vacuum to the speed of EM waves through the medium: n " = $ $ % For all real substance, n r >1. n r water 1.33 at visible band n r air 1.0003 at visible band, at sea level

Imaginary part of N The imaginary part n i describes the rate of absorption. n i 0 means absorption occurs as an EM wave passes a medium n i is also called absorption index. The relationship between absorption coefficient β αλ and absorption index n i is: β (λ = 4πn + λ n r and n i are not independent. If you know one of them, you can get the other through some complicated relationships.

1.8 1.7 1.6 (a) Index of Refraction of Water and Ice (Real Part) Water (10 o C) Ice (-5 o C) 1.5 n r 1.4 1.3 1.2 1.1 n i 1 0.1 0.15 0.2 0.3 0.5 0.7 1 1.5 2 3 4 5 7 10 15 20 30 50 Wavelength [µm] (b) Index of Refraction of Water and Ice (Imag. Part) 1 0.1 0.01 0.001 0.0001 1e-05 1e-06 1e-07 Water (10 o C) 1e-08 Ice (-5 o C) 1e-09 0.1 0.15 0.2 0.3 0.5 0.7 1 1.5 2 3 4 5 7 10 15 20 30 50 Wavelength [µm]

Reflection and Refraction What causes the phenomena of reflection and refraction? The sudden change of phase speed at boundaries between media. Reflection: When an EM wave encounters a planar boundary between two homogeneous media having different indices of refraction, some of the energy of the radiation is reflected; while the remainder passes through the boundary into the second medium. Refraction: The direction of the transmitted wave in medium 2 may altered from the original direction in medium 1, a phenomenon known as Refraction.

Angle of Reflection The reflected ray lies in the same plane as the direction of incident ray and local normal, but on the opposite side from the incident ray. The reflected angle equals the incident angle: θ + = θ " The wavelength of reflected ray equals the wavelength of incident ray: λ + = λ " incident angle= 0

Angle of Refraction and Snell s Law In refraction, the transmitted ray changes direction according to Snell s Law: -+./ 0 1 % = -+./ 2 1 3, N 1 and N 2 are the indices of refraction of medium 1 and 2. θ 4 is the angle of the transmitted ray relative to local normal. If θ + = 0, then θ 4 = 0. If θ + > 0 and N 1 < N 2 (from air to water), then θ 4 < θ + and the wavelength of transmitted ray is less than the wavelength of incident ray: λ 4 < λ + incident angle θ + > 0 and N 1 < N 2

Critical Angle of Refraction If θ + > 0 and N 1 > N 2 (from water to air), then θ 4 > θ + and the wavelength of transmitted ray is greater than the wavelength of incident ray: λ 4 > λ + Under the same condition, Critical angle θ A arcsin ( 1 3 1 % ). When θ + = θ A, θ 4 =90. It s impossible to have θ + > θ A becasue it would make sinθ 4 > 1. So waves incident on the interface at an angle greater than the critical angle can t pass through the interface at all but rather experience total reflection. In the visible band, N 1 1.33 for water and N 2 for air, then θ A 49.

Applications to Meteorology The rules for reflection and refraction can be applied not only to planar boundaries, but to any surface whose radius (r) of curvature is much greater than the wavelength (λ) of the radiation. Therefore, for atmospheric particles, when r >> λ (or size parameter x > 50 ~2000, where x=2πr/ λ), we can use reflection/refraction rules (i.e. ray tracing or geometric optics) to solve scattering/absorption properties in the radiative transfer calculations. On the other hand, when r ~ λ (or size parameter 0.2 < x < 50 ~2000 ), we have to use Mie/Rayleigh scattering theory to solve scattering properties in the radiative transfer calculations.

Scattering Regimes

Use Geometric Optics to Explain Rainbow Condition: scattering (reflection and refraction) of visible sunlight (0.3 µm < λ<0.7 µm ) by large cloud ice particles (radius > 50 µm) or raindrops (100 µm to 3 mm). The path of a single incident ray: External reflection Transmitted through refraction At the back side of the drop, a fraction of energy goes direct transmission, while another fraction reflected internally Single internal reflection: the portion of the original ray that was internally reflected. It is responsible for the primary rainbow. The first internally reflected ray will be transmitted by refraction and reflected again. Double internal reflection: repeat the above process, responsible for secondary rainbow. Separation of colors in a rainbow: because n r for water increases slightly from the red end to the violet end, causing different refraction angles for different wavelengths. Petty Fig. 4.7

Transmitivity (transmittance) and Reflectivity (reflectance) Recall the definition of absorptivity (absorptance): WX-Y"XZ[ "W[+W4+Y. W4 \W]Z^Z._4` λ a λ = +.$+[Z.4 "W[+W4+Y. W4 \W]Z^Z._4` λ Similarly, reflectivity (reflectance) is defined as: "Zb^Z$4Z[ "W[+W4+Y. W4 \W]Z^Z._4` λ r λ = +.$+[Z.4 "W[+W4+Y. W4 \W]Z^Z._4` λ Transmitivity (transmittance) is defined as: t λ = 4"W.-d+44Z[ "W[+W4+Y. W4 \W]Z^Z._4` λ +.$+[Z.4 "W[+W4+Y. W4 \W]Z^Z._4` λ

Relationship between absorptivity, transmitivity, and reflectivity Case 1: sunlight incident on Earth s surface, no transmission, so: a λ + r λ = 1 Case 2: When sunlight incident on the top of a cloud layer. A photon of sunlight will experience one of the four possible fates: Direct transmitted without being scattered or absorbed: direct transmittance t λdir It may be scattered one or more times and emerge from the bottom of the cloud layer: diffuse transmittance t λdiff It may be scattered one or more times and emerge from the top of the cloud layer: reflectance r λ Whatever is neither transmitted nor reflected must be absorbed: absorptance a λ Obviously for case 2: t λdir + t λdiff + a λ + r λ = 1, where t λdir + t λdiff = t λ