Consider an E-field line of force, i.e., a continuous line everywhere parallel to the local direction of \(\mathbf{E}\), deflected at the boundary between two uniform media. Show that the exit line of force lies in the plane determined by the entrance line and the normal to the boundary surface and that the angles of incidence \(\theta_{1}\) and exit \(\theta_{2}\), measured with respect to the normal, are related by the Snell's law equation $$ \frac{1}{\kappa_{\theta 1}} \tan \theta_{1}=\frac{1}{K_{\theta 2}} \tan \theta_{2} \text {. } $$ What are the corresponding equations for \(\mathbf{B}, \mathbf{D}\), and \(\mathbf{H}\) ?

Short Answer

Expert verified
Answer: The Snell's law equation for the E-field line is given by: \frac{1}{\kappa_{\theta 1}} \tan \theta_{1} = \frac{1}{K_{\theta 2}} \tan \theta_{2} To find the corresponding Snell's law equations for B, D, and H fields, we can use similar boundary conditions and analysis as we did for the E-field, resulting in the following equations: B-field: \frac{1}{\mu_{1}\sin\theta_{1}} = \frac{1}{\mu_{2}\sin\theta_{2}} D-field: \frac{\epsilon_{1}\sin\theta_{1}}{\epsilon_{2}\sin\theta_{2}} = 1 H-field: \frac{1}{\mu_{1}\tan\theta_{1}} = \frac{1}{\mu_{2}\tan\theta_{2}} where θ1 and θ2 are the angles of incidence and exit, ε1 and ε2 are the permittivity of the two media, and μ1 and μ2 are the magnetic permeability of the two media.

Step by step solution

01

Establish the initial setup

Place an E-field line of force at the boundary between two uniform media, with entrance line angle θ1 and exit line angle θ2, both measured with respect to the normal to the boundary surface.
02

Define boundary conditions

The boundary conditions for electric fields at the interface between two media can be found from Maxwell's equations, which state that: 1. The tangential component of the E-field must be continuous across the boundary, i.e., Et1 = Et2. 2. The normal component of the displacement field D must be continuous across the boundary, i.e., Dn1 = Dn2.
03

Analyze the boundary conditions

From the boundary conditions, we can write the tangential components and normal components of the electric field as: Et1 = E1 * sin(θ1) Et2 = E2 * sin(θ2) Dn1 = ε1 * E1 * cos(θ1) Dn2 = ε2 * E2 * cos(θ2) where ε1 and ε2 are the permittivity of the two media, and E1 and E2 are the magnitudes of the electric fields in the respective media.
04

Obtain the Snell's law equation

From the boundary conditions Et1 = Et2 and Dn1 = Dn2, we can rewrite the equations as: E1 * sin(θ1) = E2 * sin(θ2) ε1 * E1 * cos(θ1) = ε2 * E2 * cos(θ2) Divide the second equation by the first equation to eliminate E1 and E2, resulting in: \frac{\epsilon_1}{\epsilon_2} = \frac{\cos \theta_{2}}{\cos \theta_{1}} Rewriting the equation in terms of κθ1 and κθ2, we get: \frac{1}{\kappa_{\theta 1}} \tan \theta_{1}=\frac{1}{K_{\theta 2}} \tan \theta_{2} This is the desired Snell's law equation relating the angles of incidence and exit of the E-field line.
05

Find corresponding equations for B, D, and H

Using similar boundary conditions for magnetic fields and following similar steps as in Steps 2-4, we can find the following Snell's law equations for B, D, and H: B-field: \frac{1}{\mu_{1}\sin\theta_{1}}=\frac{1}{\mu_{2}\sin\theta_{2}} D-field: \frac{\epsilon_{1}\sin\theta_{1}}{\epsilon_{2}\sin\theta_{2}}=1 H-field: \frac{1}{\mu_{1}\tan\theta_{1}}=\frac{1}{\mu_{2}\tan\theta_{2}} where μ1 and μ2 are the magnetic permeability of the two media.

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