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The_Cambridge_Handbook_of_Physics_Formulas

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152 Electromagnetism<br />

7.8 Waves in and out <strong>of</strong> media<br />

Waves in lossless media<br />

Electric field<br />

Magnetic field<br />

∇ 2 E = µɛ ∂2 E<br />

∂t 2 (7.193)<br />

∇ 2 B = µɛ ∂2 B<br />

∂t 2 (7.194)<br />

E electric field<br />

µ permeability (= µ 0 µ r )<br />

ɛ permittivity (= ɛ 0 ɛ r )<br />

B magnetic flux density<br />

t time<br />

Refractive index η = √ ɛ r µ r (7.195)<br />

Wave speed v = 1 √ µɛ<br />

= c η<br />

√<br />

µ0<br />

Impedance <strong>of</strong> free space Z 0 = ≃ 376.7 Ω (7.197)<br />

ɛ 0<br />

(7.196)<br />

v<br />

η<br />

c<br />

wave phase speed<br />

refractive index<br />

speed <strong>of</strong> light<br />

Wave impedance Z = E H = Z 0<br />

√<br />

µr<br />

ɛ r<br />

(7.198)<br />

Z 0<br />

Z<br />

H<br />

impedance <strong>of</strong> free<br />

space<br />

wave impedance<br />

magnetic field strength<br />

Radiation pressure a<br />

Radiation<br />

momentum G = N<br />

density<br />

c 2 (7.199)<br />

Isotropic<br />

radiation<br />

Specular<br />

reflection<br />

G<br />

N<br />

c<br />

momentum density<br />

Poynting vector<br />

speed <strong>of</strong> light<br />

p n = 1 3 u(1+R) (7.200) u incident radiation<br />

energy density<br />

R (power) reflectance<br />

p n normal pressure<br />

coefficient<br />

p n = u(1+R)cos 2 θ i (7.201)<br />

p t = u(1−R)sinθ i cosθ i (7.202)<br />

p t<br />

θ i<br />

tangential pressure<br />

angle <strong>of</strong> incidence<br />

u<br />

θi<br />

From an<br />

extended p n = 1+R ∫∫<br />

c<br />

source b<br />

From a point<br />

source, c<br />

luminosity L<br />

p n = L(1+R)<br />

4πr 2 c<br />

I ν (θ,φ)cos 2 θ dΩ dν<br />

(7.203)<br />

(7.204)<br />

I ν<br />

ν<br />

Ω<br />

θ<br />

L<br />

r<br />

specific intensity<br />

frequency<br />

solid angle<br />

angle between dΩ<br />

and normal to plane<br />

source luminosity<br />

(i.e., radiant power)<br />

distance from source<br />

a On an opaque surface.<br />

b In spherical polar coordinates. See page 120 for the meaning <strong>of</strong> specific intensity.<br />

c Normal to the plane.<br />

z<br />

(normal)<br />

x<br />

φ<br />

θ<br />

dΩ<br />

y

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