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Physics · Ch 10 — Electrostatics

Electric Flux

10.7

Electric Flux

As discussed in the previous section, the intensity (magnitude) of the electric field E can be thought of as the number of lines of force crossing a unit area held perpendicular to those lines, E=number of lines of forcearea enclosing the lines.E=\frac{\text{number of lines of force}}{\text{area enclosing the lines}}. Rearranging, the total number of lines of force through a flat area equals E×(area)E\times(\text{area}).

When the area is instead INCLINED at some angle θ\theta to the direction of the field (Fig. 10.14), the number of lines actually passing through it -- the ELECTRIC FLUX -- must be calculated more carefully. If θ\theta is the angle between the field E⃗\vec{E} and the area's own AREA VECTOR dS⃗d\vec{S} (a vector of magnitude equal to the area, directed along the area's outward normal), the electric flux through the small area element dSdS is defined as the product of the COMPONENT of dS⃗d\vec{S} along E⃗\vec{E} and the field magnitude: dϕ=(component of dS along E)×(area of dS)=E(dScos⁡θ)=E dScos⁡θ,d\phi=(\text{component of }dS\text{ along }E)\times(\text{area of }dS)=E(dS\cos\theta)=E\,dS\cos\theta, which can be written compactly as the dot product dϕ=E⃗⋅dS⃗.d\phi=\vec{E}\cdot d\vec{S}. Flux is therefore maximum when the area directly FACES the field (θ=0\theta=0, area perpendicular to E) and exactly ZERO when the area lies PARALLEL to the field (θ=90∘\theta=90^\circ, so the field lines merely graze past it without actually crossing it). …

Figure 10.14Fig. 10.14: Electric flux through an inclined area S

What this figure shows. A flat area element, of vector dS⃗d\vec{S} (drawn as an arrow perpendicular to the flat area, representing its outward normal), is shown tilted at an angle θ\theta relative to a set of parallel electric field lines E⃗\vec{E} passing through the region. The figure geometrically sets up the projection used in the flux formula: only the COMPONENT of the area (or equivalently of the field) that is perpendicular to the other actually contributes to flux, giving dϕ=E dScos⁡θ=E⃗⋅dS⃗d\phi=E\,dS\cos\theta=\vec{E}\cdot d\vec{S}, visually showing why flux depends on the angle of tilt between the area and the f …