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en/8.1.20.md
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| + | ### Statement | ||
| + | |||
| + | $8.1.20.$ [Insert the problem statement] | ||
| + | |||
| + | ### Solution | ||
| + | |||
| + | |||
| + | Part (a): Source A (+I) and sink B (–I) | ||
| + | |||
| + | Positions: | ||
| + | |||
| + | · A at (-d/2, 0, 0) | ||
| + | · B at (+d/2, 0, 0) | ||
| + | Separation d. | ||
| + | |||
| + | Individual fields: | ||
| + | |||
| + | · Source A: \displaystyle \mathbf{J}_A = \frac{I}{4\pi r_A^3}\mathbf{r}_A | ||
| + | · Sink B (outgoing current): \displaystyle \mathbf{J}_B = -\frac{I}{4\pi r_B^3}\mathbf{r}_B | ||
| + | |||
| + | Plane of symmetry: x = 0, perpendicular to line AB at its midpoint. | ||
| + | |||
| + | By symmetry, on the plane x = 0: | ||
| + | |||
| + | · r_A = r_B = r = \sqrt{(d/2)^2 + y^2 + z^2} | ||
| + | · The transverse (y, z) components of \mathbf{J}_A and \mathbf{J}_B cancel. | ||
| + | · The x-components add constructively. | ||
| + | |||
| + | J_x(0, y, z) = \frac{I}{4\pi r^3}\left(\frac{d}{2}\right) + \frac{I}{4\pi r^3}\left(\frac{d}{2}\right) = \frac{I d}{4\pi r^3} | ||
| + | |||
| + | J_y = J_z = 0. | ||
| + | |||
| + | Thus, the volume current density in the symmetry plane is purely perpendicular to the plane: | ||
| + | |||
| + | \boxed{\mathbf{J} = \frac{I d}{4\pi \big[(d/2)^2 + \rho^2\big]^{3/2}}\;\hat{x}}, \qquad \rho = \sqrt{y^2 + z^2}. | ||
| + | |||
| + | Total current through the plane: | ||
| + | Integrate over the entire plane x = 0: | ||
| + | |||
| + | I_{\text{plane}} = \int_0^\infty J_x(\rho)\, 2\pi\rho\, d\rho | ||
| + | = \int_0^\infty \frac{I d}{4\pi (\frac{d^2}{4}+\rho^2)^{3/2}}\, 2\pi\rho\, d\rho. | ||
| + | |||
| + | With a = d/2, the integral equals 1/a = 2/d. Then: | ||
| + | |||
| + | I_{\text{plane}} = \frac{I d}{2} \cdot \frac{2}{d} = I. | ||
| + | |||
| + | \boxed{I_{\text{total}} = I} | ||
| + | |||
| + | All the current leaving A crosses the symmetry plane toward B. | ||
| + | |||
| + | If B also carries a current I (both are sources): | ||
| + | Now \mathbf{J}_B = +\frac{I}{4\pi r_B^3}\mathbf{r}_B. On the plane x = 0 the x-components oppose: | ||
| + | |||
| + | J_{Ax} = \frac{I d}{8\pi r^3},\quad J_{Bx} = -\frac{I d}{8\pi r^3}. | ||
| + | |||
| + | Result: \mathbf{J} = 0 on the plane, total current = 0. No net flow by symmetry. | ||
| + | |||
| + | --- | ||
| + | |||
| + | Part (b): Point source at depth h below the Earth's surface | ||
| + | |||
| + | Model: Conducting half-space (z > 0), insulating surface at z = 0 (no current flow into the air). Real source at (0,0,h) with current I. | ||
| + | |||
| + | Method of images: | ||
| + | To satisfy J_z = 0 at z = 0, an identical image source of current I is added at (0,0,-h), considering the full space. | ||
| + | |||
| + | Current density on the surface (z = 0): | ||
| + | |||
| + | · Vector from real source: \mathbf{r}_1 = (x, y, -h), r_1 = \sqrt{\rho^2 + h^2}. | ||
| + | · Vector from image source: \mathbf{r}_2 = (x, y, h), r_2 = r_1 = r. | ||
| + | |||
| + | \mathbf{J}_{\text{surf}} = \frac{I}{4\pi r^3}\mathbf{r}_1 + \frac{I}{4\pi r^3}\mathbf{r}_2 | ||
| + | = \frac{I}{4\pi r^3}(2x, 2y, 0) | ||
| + | = \frac{I}{2\pi (\rho^2 + h^2)^{3/2}}\,(x\hat{x} + y\hat{y}). | ||
| + | |||
| + | It is radially outward from the point directly above the source (\rho = 0). Magnitude: | ||
| + | |||
| + | \boxed{J(\rho) = \frac{I}{2\pi} \frac{\rho}{(\rho^2 + h^2)^{3/2}} }. | ||
| + | |||
| + | The surface current density is purely horizontal and decreases with radial distance \rho. | ||
| + | |||
| + | #### Answer | ||
| + | |||
| + | [Insert a concise answer or boxed result] | ||
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| ### Statement | |||
| $8.1.20.$ [Insert the problem statement] | |||
| ### Solution | |||
| Part (a): Source A (+I) and sink B (–I) | |||
| Positions: | |||
| · A at (-d/2, 0, 0) | |||
| · B at (+d/2, 0, 0) | |||
| Separation d. | |||
| Individual fields: | |||
| · Source A: \displaystyle \mathbf{J}_A = \frac{I}{4\pi r_A^3}\mathbf{r}_A | |||
| · Sink B (outgoing current): \displaystyle \mathbf{J}_B = -\frac{I}{4\pi r_B^3}\mathbf{r}_B | |||
| Plane of symmetry: x = 0, perpendicular to line AB at its midpoint. | |||
| By symmetry, on the plane x = 0: | |||
| · r_A = r_B = r = \sqrt{(d/2)^2 + y^2 + z^2} | |||
| · The transverse (y, z) components of \mathbf{J}_A and \mathbf{J}_B cancel. | |||
| · The x-components add constructively. | |||
| J_x(0, y, z) = \frac{I}{4\pi r^3}\left(\frac{d}{2}\right) + \frac{I}{4\pi r^3}\left(\frac{d}{2}\right) = \frac{I d}{4\pi r^3} | |||
| J_y = J_z = 0. | |||
| Thus, the volume current density in the symmetry plane is purely perpendicular to the plane: | |||
| \boxed{\mathbf{J} = \frac{I d}{4\pi \big[(d/2)^2 + \rho^2\big]^{3/2}}\;\hat{x}}, \qquad \rho = \sqrt{y^2 + z^2}. | |||
| Total current through the plane: | |||
| Integrate over the entire plane x = 0: | |||
| I_{\text{plane}} = \int_0^\infty J_x(\rho)\, 2\pi\rho\, d\rho | |||
| = \int_0^\infty \frac{I d}{4\pi (\frac{d^2}{4}+\rho^2)^{3/2}}\, 2\pi\rho\, d\rho. | |||
| With a = d/2, the integral equals 1/a = 2/d. Then: | |||
| I_{\text{plane}} = \frac{I d}{2} \cdot \frac{2}{d} = I. | |||
| \boxed{I_{\text{total}} = I} | |||
| All the current leaving A crosses the symmetry plane toward B. | |||
| If B also carries a current I (both are sources): | |||
| Now \mathbf{J}_B = +\frac{I}{4\pi r_B^3}\mathbf{r}_B. On the plane x = 0 the x-components oppose: | |||
| J_{Ax} = \frac{I d}{8\pi r^3},\quad J_{Bx} = -\frac{I d}{8\pi r^3}. | |||
| Result: \mathbf{J} = 0 on the plane, total current = 0. No net flow by symmetry. | |||
| --- | |||
| Part (b): Point source at depth h below the Earth's surface | |||
| Model: Conducting half-space (z > 0), insulating surface at z = 0 (no current flow into the air). Real source at (0,0,h) with current I. | |||
| Method of images: | |||
| To satisfy J_z = 0 at z = 0, an identical image source of current I is added at (0,0,-h), considering the full space. | |||
| Current density on the surface (z = 0): | |||
| · Vector from real source: \mathbf{r}_1 = (x, y, -h), r_1 = \sqrt{\rho^2 + h^2}. | |||
| · Vector from image source: \mathbf{r}_2 = (x, y, h), r_2 = r_1 = r. | |||
| \mathbf{J}_{\text{surf}} = \frac{I}{4\pi r^3}\mathbf{r}_1 + \frac{I}{4\pi r^3}\mathbf{r}_2 | |||
| = \frac{I}{4\pi r^3}(2x, 2y, 0) | |||
| = \frac{I}{2\pi (\rho^2 + h^2)^{3/2}}\,(x\hat{x} + y\hat{y}). | |||
| It is radially outward from the point directly above the source (\rho = 0). Magnitude: | |||
| \boxed{J(\rho) = \frac{I}{2\pi} \frac{\rho}{(\rho^2 + h^2)^{3/2}} }. | |||
| The surface current density is purely horizontal and decreases with radial distance \rho. | |||
| #### Answer | |||
| [Insert a concise answer or boxed result] | |||