Academy
Formulas/physics/Electric Charges Fields/Field on Equatorial Line of Dipole

Field on Equatorial Line of Dipole

Field at distance r from centre on the equatorial plane. Direction is antiparallel to p̂. Magnitude is half of axial field at same r (far field).
Class 11Class 12
Derivation

Setup

Same dipole as before: q-q at (0,a,0)(0, -a, 0)...

Let me use the standard orientation: dipole along the x-axis, +q+q at (a,0)(a, 0), q-q at (a,0)(-a, 0).

Consider point P at (0,r)(0, r) on the y-axis (equatorial plane). Distance from each charge to P:

d=r2+a2d = \sqrt{r^2 + a^2}

Fields from each charge

By symmetry, the x-components of E+E_+ and EE_- at P are equal in magnitude and opposite in direction — they cancel.

The y-components also cancel... wait, let me redo.

E+\vec{E}_+: from +q+q at (a,0)(a,0) to P at (0,r)(0,r). Direction vector: (a,r)/d(-a, r)/d.

E+=q4πε0d2(a,r)d\vec{E}_+ = \frac{q}{4\pi\varepsilon_0 d^2} \cdot \frac{(-a, r)}{d}

E\vec{E}_-: from q-q at (a,0)(-a,0) to P at (0,r)(0,r). Force on positive test charge points toward q-q, so direction: (a,r)(1)(−a, −r)\cdot(-1) ...

Let me be careful. Field due to q-q points toward q-q:

Direction from P to q-q: (a,0)(0,r)=(a,r)(-a, 0) - (0, r) = (-a, -r), normalised: (a,r)/d(-a,-r)/d.

So:

E=q4πε0d2(a,r)d\vec{E}_- = \frac{q}{4\pi\varepsilon_0 d^2} \cdot \frac{(-a, -r)}{d}

Net field

E=E++E=q4πε0d3[(a,r)+(a,r)]=q4πε0d3(2a,0)\vec{E} = \vec{E}_+ + \vec{E}_- = \frac{q}{4\pi\varepsilon_0 d^3}\left[(-a,r) + (-a,-r)\right] = \frac{q}{4\pi\varepsilon_0 d^3}(-2a, 0)

The y-components cancel. The x-component:

E=2qa4πε0(r2+a2)3/2=p4πε0(r2+a2)3/2E = \frac{-2qa}{4\pi\varepsilon_0 (r^2+a^2)^{3/2}} = \frac{-p}{4\pi\varepsilon_0(r^2+a^2)^{3/2}}

The negative sign means the field is in the x-x direction, i.e., antiparallel to p\vec{p}.

Eeq=p4πε0(r2+a2)3/2p^\boxed{\vec{E}_{eq} = -\frac{p}{4\pi\varepsilon_0(r^2+a^2)^{3/2}}\hat{p}}

Far-field approximation (rar \gg a)

Ep4πε0r3E \approx \frac{p}{4\pi\varepsilon_0 r^3}
Remember
Compare with the axial field: $E_{axial} \approx 2p/(4\pi\varepsilon_0 r^3)$. At the same distance, the axial field is twice the equatorial field. Both directions are antiparallel to each other at a given $r$.