Coördinate system

Spherical coördinates

Spherical coördinates have two variants which essentially vary only in argument order. One variant is traditionally used in maths while another is used in physics. In general, the argument that occurs in all three cartesian axes and two sine functions will have the domain [0,𝜋].

See Spherical coördinates in differential geometry for a formal treatment.

Mathematical convention

Where 𝜌 is the radial distance, 𝜃 is the azimuthal angle and 𝜙 is the polar angle

⃗𝐫:\vthree𝜌𝜃𝜙↦\vthree𝜌cos⁡𝜃sin⁡𝜙𝜌sin⁡𝜃sin⁡𝜙𝜌cos⁡𝜙

with the signature ⃗𝐫 :[0,∞) ×[0,2𝜋) ×[0,𝜋] →ℝ3.

Physics convention

The physics convention (ISO 80000-2:2019) is swapped: Where 𝜌 is the radial distance, 𝜃 is the polar angle and 𝜙 is the azimuthal angle1

⃗𝐫:\vthree𝜌𝜃𝜙↦\vthree𝜌sin⁡𝜃cos⁡𝜙𝜌sin⁡𝜃sin⁡𝜙𝜌cos⁡𝜃

with the signature ⃗𝐫 :[0,∞) ×[0,𝜋] ×[0,2𝜋) →ℝ3.

This has the benefit of generating a conventionally-orientated parameterisation of a sphere's surface

⃗𝐫:\vtwo𝜃𝜙↦\vthree𝑅sin⁡𝜃cos⁡𝜙𝑅sin⁡𝜃sin⁡𝜙𝑅cos⁡𝜃:[0,𝜋]×[0,2𝜋)→ℝ3⃗𝐍:\vtwo𝜃𝜙↦\vthree𝑅2sin2⁡𝜃cos⁡𝜙𝑅2sin2⁡𝜃sin⁡𝜙𝑅2sin⁡𝜃cos⁡𝜃

Calculus

The following differential quantities may be useful2

  1. 𝑑⃗ℓ=𝑑𝑟ˆ𝐫+𝑟𝑑𝜃ˆ𝜃+𝑟sin⁡𝜃𝑑𝜙ˆ𝜙
\begin{align*}
d \tau = r^2 \sin\theta\,dr\,d\theta\,d\phi = r^2 \,dr\, d\Omega
\end{align*}
$$

3. grad⁡𝐹=𝜕𝑇𝜕𝑟ˆ𝐫+1𝑟𝜕𝑇𝜕𝜃ˆ𝜃+1𝑟sin⁡𝜃𝜕𝑇𝜕𝜙ˆ𝜙 4. ∇2𝐹=1𝑟2𝜕𝜕𝑟(𝑟2𝜕𝐹𝜕𝑟)+1𝑟2sin⁡𝜃𝜕𝜕𝜃(sin⁡𝜃𝜕𝐹𝜕𝜃)+1𝑟2sin2⁡𝜃𝜕2𝐹𝜕𝜙2 5. div⁡⃗𝐅=1𝑟2𝜕𝜕𝑟(𝑟2𝐹𝑟)+1𝑟sin⁡𝜃𝜕𝜕𝜃(sin⁡(𝜃)𝐹𝜃)+1𝑟sin⁡𝜃𝜕𝐹𝜙𝜕𝜙 6. curl⁡⃗𝐅=1𝑟sin⁡𝜃(𝜕𝜕𝜃(sin⁡(𝜃)𝐹𝜃)−𝜕𝐹𝜃𝜕𝜙)ˆ𝐫+1𝑟(1sin⁡𝜃𝜕𝐹𝑟𝜕𝜙−𝜕𝜕𝑟(𝑟𝐹𝑟))ˆ𝜃+1𝑟(𝜕𝜕𝑟(𝑟𝐹𝜃)−𝜕𝐹𝑟𝜕𝜃)ˆ𝜙


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Footnotes

  1. 2021. Covariant physics: From classical mechanics to general relativity and beyond, p. 5 ↩

  2. 2013. Introduction to electrodynamics, pp. 40, 42 (§1.4.1) ↩