Let U⊆RnU\subseteq\mathbb{R}^n be open. A scalar field on UU is a function f:U→R.f:U\rightarrow\mathbb{R}. A vector field on UU is a function F‾=(F1,…,Fn):U→Rn\underline{F}=\left(F_1,\ldots,F_n\right):U\rightarrow\mathbb{R}^n that assigns a vector to each point of U.U. A vector field is CkC^k if and only if each of its components is Ck.C^k.

Let x‾,y‾∈Rn.\underline{x},\underline{y}\in\mathbb{R}^n. The dot product of x‾\underline{x} and y‾\underline{y} is the sum of the products of their coordinates.

x‾⋅y‾:=∑i=1nxi yi=x‾⊺y‾\underline{x}\cdot\underline{y}:=\sum_{i=1}^{n}x_i\,y_i=\underline{x}^\intercal\underline{y}

The dot product is the standard inner product on Rn,\mathbb{R}^n, so that ∥x‾∥=x‾⋅x‾\lVert\underline{x}\rVert=\sqrt{\underline{x}\cdot\underline{x}} is the Euclidean length of x‾\underline{x} and two vectors are orthogonal if and only if their dot product is zero. The directional derivative of a differentiable scalar field is Dv‾f(x‾)=∇f(x‾)⋅v‾.D_{\underline{v}}f(\underline{x})=\nabla f(\underline{x})\cdot\underline{v}.

A curve in Rn\mathbb{R}^n is a function γ‾=(γ1,…,γn):[a,b]→Rn\underline{\gamma}=\left(\gamma_1,\ldots,\gamma_n\right):\left[a,b\right]\rightarrow\mathbb{R}^n with continuous components. The initial point of γ‾\underline{\gamma} is γ‾(a)\underline{\gamma}(a) and the terminal point of γ‾\underline{\gamma} is γ‾(b).\underline{\gamma}(b).

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a curve. The curve γ‾\underline{\gamma} is closed if and only if γ‾(a)=γ‾(b).\underline{\gamma}(a)=\underline{\gamma}(b). The curve γ‾\underline{\gamma} is simple if and only if it is injective on [a,b)\left[a,b\right) and on (a,b].\left(a,b\right].

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a C1C^1 curve. The velocity of γ‾\underline{\gamma} at tt is the vector of derivatives of its components, γ‾′(t)=(γ1′(t),…,γn′(t)).\underline{\gamma}'(t)=\left(\gamma_1'(t),\ldots,\gamma_n'(t)\right). The speed of γ‾\underline{\gamma} at tt is ∥γ‾′(t)∥.\lVert\underline{\gamma}'(t)\rVert. Where the speed is non-zero, the unit tangent vector of γ‾\underline{\gamma} at tt is the velocity divided by the speed.

T‾(t):=γ‾′(t)∥γ‾′(t)∥\underline{T}(t):=\frac{\underline{\gamma}'(t)}{\lVert\underline{\gamma}'(t)\rVert}

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a C1C^1 curve. The curve γ‾\underline{\gamma} is regular if and only if its speed is never zero.

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a curve. The curve γ‾\underline{\gamma} is piecewise C1C^1 if and only if [a,b]\left[a,b\right] is the union of finitely many intervals on each of which γ‾\underline{\gamma} is C1.C^1.

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a piecewise C1C^1 curve. The arc length of γ‾\underline{\gamma} is the integral of its speed.

L(γ‾):=∫ab∥γ‾′(t)∥ dtL\left(\underline{\gamma}\right):=\int_a^b\lVert\underline{\gamma}'(t)\rVert\,dt

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a curve and φ:[α,β]→[a,b]\varphi:\left[\alpha,\beta\right]\rightarrow\left[a,b\right] be a C1C^1 bijection with φ′≠0.\varphi'\neq 0. The curve γ‾∘φ\underline{\gamma}\circ\varphi is a reparametrisation of γ‾.\underline{\gamma}. The reparametrisation preserves orientation if and only if φ′>0\varphi'>0 and reverses orientation if and only if φ′<0.\varphi'<0. Arc length is unchanged by reparametrisation.

Let γ‾:[a,b]→Rn\underline{\gamma}:\left[a,b\right]\rightarrow\mathbb{R}^n be a curve. The reversed curve of γ‾\underline{\gamma} is the curve γ‾−(t):=γ‾(a+b−t),\underline{\gamma}^-(t):=\underline{\gamma}(a+b-t), which traces the same image in the opposite direction.

Let a‾,b‾∈R3.\underline{a},\underline{b}\in\mathbb{R}^3. The cross product of a‾\underline{a} and b‾\underline{b} is the vector

a‾×b‾:=(a2b3−a3b2, a3b1−a1b3, a1b2−a2b1)=det⁡[e‾1e‾2e‾3a1a2a3b1b2b3]\underline{a}\times\underline{b}:=\left(a_2 b_3-a_3 b_2,\,a_3 b_1-a_1 b_3,\,a_1 b_2-a_2 b_1\right)=\det\begin{bmatrix}\underline{e}_1 & \underline{e}_2 & \underline{e}_3 \\ a_1 & a_2 & a_3 \\ b_1 & b_2 & b_3\end{bmatrix}

where the determinant is expanded along its first row of standard basis vectors. The cross product has the following properties:

  • it is bilinear;
  • it is anticommutative, b‾×a‾=−a‾×b‾,\underline{b}\times\underline{a}=-\underline{a}\times\underline{b}, so a‾×a‾=0‾;\underline{a}\times\underline{a}=\underline{0};
  • it is orthogonal to both of its arguments;
  • if θ\theta is the angle between non-zero a‾\underline{a} and b‾\underline{b} then ∥a‾×b‾∥=∥a‾∥∥b‾∥sin⁡θ,\lVert\underline{a}\times\underline{b}\rVert=\lVert\underline{a}\rVert\lVert\underline{b}\rVert\sin\theta, the area of the parallelogram spanned by a‾\underline{a} and b‾;\underline{b};
  • a‾×b‾=0‾\underline{a}\times\underline{b}=\underline{0} if and only if a‾\underline{a} and b‾\underline{b} are linearly dependent;
  • the standard basis satisfies e‾1×e‾2=e‾3,\underline{e}_1\times\underline{e}_2=\underline{e}_3, e‾2×e‾3=e‾1\underline{e}_2\times\underline{e}_3=\underline{e}_1 and e‾3×e‾1=e‾2,\underline{e}_3\times\underline{e}_1=\underline{e}_2, which fixes the direction of a‾×b‾\underline{a}\times\underline{b} by the right-hand rule.

Let a‾,b‾,c‾∈R3.\underline{a},\underline{b},\underline{c}\in\mathbb{R}^3. The scalar triple product of a‾,b‾\underline{a},\underline{b} and c‾\underline{c} is the dot product of a‾\underline{a} with the cross product of b‾\underline{b} and c‾,\underline{c}, which is the determinant of the matrix with rows a‾,b‾,c‾.\underline{a},\underline{b},\underline{c}.

a‾⋅(b‾×c‾)=det⁡[a1a2a3b1b2b3c1c2c3]=b‾⋅(c‾×a‾)=c‾⋅(a‾×b‾)\underline{a}\cdot\left(\underline{b}\times\underline{c}\right)=\det\begin{bmatrix}a_1 & a_2 & a_3 \\ b_1 & b_2 & b_3 \\ c_1 & c_2 & c_3\end{bmatrix}=\underline{b}\cdot\left(\underline{c}\times\underline{a}\right)=\underline{c}\cdot\left(\underline{a}\times\underline{b}\right)

The absolute value of the scalar triple product is the volume of the parallelepiped spanned by a‾,b‾\underline{a},\underline{b} and c‾.\underline{c}.

Let a‾,b‾,c‾∈R3.\underline{a},\underline{b},\underline{c}\in\mathbb{R}^3. The vector triple product of a‾,b‾\underline{a},\underline{b} and c‾\underline{c} is a‾×(b‾×c‾),\underline{a}\times\left(\underline{b}\times\underline{c}\right), and it satisfies

a‾×(b‾×c‾)=(a‾⋅c‾)b‾−(a‾⋅b‾)c‾.\underline{a}\times\left(\underline{b}\times\underline{c}\right)=\left(\underline{a}\cdot\underline{c}\right)\underline{b}-\left(\underline{a}\cdot\underline{b}\right)\underline{c}.

The del operator is the vector of partial derivative operators.

∇:=(∂∂x1,…,∂∂xn)\nabla:=\left(\frac{\partial}{\partial x_1},\ldots,\frac{\partial}{\partial x_n}\right)

Let U⊆RnU\subseteq\mathbb{R}^n be open and f:U→Rf:U\rightarrow\mathbb{R} be a C1C^1 scalar field. The gradient ∇f\nabla f of ff is the vector field on UU whose value at each point is the gradient of ff at that point. The gradient has the following properties:

  • the gradient at x‾\underline{x} points in the direction in which ff increases fastest, since Dv‾f(x‾)=∇f(x‾)⋅v‾D_{\underline{v}}f(\underline{x})=\nabla f(\underline{x})\cdot\underline{v} is largest over unit vectors v‾\underline{v} when v‾\underline{v} is parallel to ∇f(x‾);\nabla f(\underline{x});
  • the length ∥∇f(x‾)∥\lVert\nabla f(\underline{x})\rVert is that largest rate of increase.

Let U⊆RnU\subseteq\mathbb{R}^n be open, f:U→Rf:U\rightarrow\mathbb{R} be a scalar field and c∈R.c\in\mathbb{R}. The level set of ff at cc is the set of points at which ff takes the value c.c.

{x‾∈U:f(x‾)=c}\left\{\underline{x}\in U:f(\underline{x})=c\right\}

If ff is C1C^1 and γ‾\underline{\gamma} is a C1C^1 curve in a level set of ff then the chain rule gives ∇f(γ‾(t))⋅γ‾′(t)=0,\nabla f\left(\underline{\gamma}(t)\right)\cdot\underline{\gamma}'(t)=0, so the gradient is orthogonal to level sets.

Let U⊆RnU\subseteq\mathbb{R}^n be open and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a C1C^1 vector field. The divergence of F‾\underline{F} is the scalar field given by the dot product of ∇\nabla with F‾.\underline{F}.

∇⋅F‾:=∑i=1n∂Fi∂xi=tr JF‾\nabla\cdot\underline{F}:=\sum_{i=1}^{n}\frac{\partial F_i}{\partial x_i}=\mathrm{tr}\,J_{\underline{F}}

The divergence is also written div F‾.\mathrm{div}\,\underline{F}. The vector field F‾\underline{F} is solenoidal if and only if ∇⋅F‾=0\nabla\cdot\underline{F}=0 on U.U.

Let U⊆R3U\subseteq\mathbb{R}^3 be open and F‾:U→R3\underline{F}:U\rightarrow\mathbb{R}^3 be a C1C^1 vector field. The curl of F‾\underline{F} is the vector field given by the cross product of ∇\nabla with F‾.\underline{F}.

∇×F‾:=(∂F3∂x2−∂F2∂x3, ∂F1∂x3−∂F3∂x1, ∂F2∂x1−∂F1∂x2)\nabla\times\underline{F}:=\left(\frac{\partial F_3}{\partial x_2}-\frac{\partial F_2}{\partial x_3},\,\frac{\partial F_1}{\partial x_3}-\frac{\partial F_3}{\partial x_1},\,\frac{\partial F_2}{\partial x_1}-\frac{\partial F_1}{\partial x_2}\right)

The curl is also written curl F‾.\mathrm{curl}\,\underline{F}. The vector field F‾\underline{F} is irrotational if and only if ∇×F‾=0‾\nabla\times\underline{F}=\underline{0} on U.U.

Let U⊆R2U\subseteq\mathbb{R}^2 be open and F‾=(F1,F2):U→R2\underline{F}=\left(F_1,F_2\right):U\rightarrow\mathbb{R}^2 be a C1C^1 vector field. The scalar curl of F‾\underline{F} is the scalar field ∂F2∂x1−∂F1∂x2,\frac{\partial F_2}{\partial x_1}-\frac{\partial F_1}{\partial x_2}, which is the third component of the curl of (F1,F2,0).\left(F_1,F_2,0\right).

The divergence and the curl of F‾\underline{F} are the trace and the antisymmetric part of its Jacobian matrix: the matrix JF‾−JF‾⊺J_{\underline{F}}-J_{\underline{F}}^\intercal has the components of ∇×F‾\nabla\times\underline{F} as its off-diagonal entries.

Let U⊆RnU\subseteq\mathbb{R}^n be open and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a vector field. The vector field F‾\underline{F} is radial if and only if F‾(x‾)=g(∥x‾∥)x‾\underline{F}(\underline{x})=g\left(\lVert\underline{x}\rVert\right)\underline{x} for some scalar function g.g. A C1C^1 radial field is irrotational.

Let U⊆RnU\subseteq\mathbb{R}^n be open and f:U→Rf:U\rightarrow\mathbb{R} be a C2C^2 scalar field. The Laplacian of ff is the divergence of its gradient, which is the sum of its unmixed second-order partial derivatives.

Δf:=∇⋅∇f=∑i=1n∂2f∂xi2=tr Hf\Delta f:=\nabla\cdot\nabla f=\sum_{i=1}^{n}\frac{\partial^2 f}{\partial x_i^2}=\mathrm{tr}\,H_f

The Laplacian is also written ∇2f.\nabla^2 f. The scalar field ff is harmonic on UU if and only if Δf=0\Delta f=0 on U.U.

Let U⊆RnU\subseteq\mathbb{R}^n be open and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a C2C^2 vector field. The vector Laplacian of F‾\underline{F} is the vector field ΔF‾\Delta\underline{F} whose components are the Laplacians of the components of F‾.\underline{F}.

Let U⊆R3U\subseteq\mathbb{R}^3 be open, f,gf,g be C2C^2 scalar fields on UU and F‾,G‾\underline{F},\underline{G} be C2C^2 vector fields on U.U. By Schwarz’s theorem the following vector identities hold:

∇(f g)=f ∇g+g ∇f\nabla\left(f\,g\right)=f\,\nabla g+g\,\nabla f ∇⋅(f F‾)=∇f⋅F‾+f ∇⋅F‾,∇×(f F‾)=∇f×F‾+f ∇×F‾\nabla\cdot\left(f\,\underline{F}\right)=\nabla f\cdot\underline{F}+f\,\nabla\cdot\underline{F},\qquad\nabla\times\left(f\,\underline{F}\right)=\nabla f\times\underline{F}+f\,\nabla\times\underline{F} ∇⋅(F‾×G‾)=G‾⋅(∇×F‾)−F‾⋅(∇×G‾)\nabla\cdot\left(\underline{F}\times\underline{G}\right)=\underline{G}\cdot\left(\nabla\times\underline{F}\right)-\underline{F}\cdot\left(\nabla\times\underline{G}\right) ∇×(∇f)=0‾,∇⋅(∇×F‾)=0\nabla\times\left(\nabla f\right)=\underline{0},\qquad\nabla\cdot\left(\nabla\times\underline{F}\right)=0 ∇×(∇×F‾)=∇(∇⋅F‾)−ΔF‾\nabla\times\left(\nabla\times\underline{F}\right)=\nabla\left(\nabla\cdot\underline{F}\right)-\Delta\underline{F}

The first identity on the fourth line states that gradient fields are irrotational, and the second states that curl fields are solenoidal. The identities on the first two lines hold in Rn\mathbb{R}^n with the curl omitted.

Let U⊆RnU\subseteq\mathbb{R}^n be open, γ‾:[a,b]→U\underline{\gamma}:\left[a,b\right]\rightarrow U be a piecewise C1C^1 curve and f:U→Rf:U\rightarrow\mathbb{R} be a continuous scalar field. The line integral of ff along γ‾\underline{\gamma} with respect to arc length is the integral of ff along the curve weighted by the speed.

∫γ‾f ds:=∫abf(γ‾(t))∥γ‾′(t)∥ dt\int_{\underline{\gamma}}f\,ds:=\int_a^b f\left(\underline{\gamma}(t)\right)\lVert\underline{\gamma}'(t)\rVert\,dt

Let U⊆RnU\subseteq\mathbb{R}^n be open, γ‾:[a,b]→U\underline{\gamma}:\left[a,b\right]\rightarrow U be a piecewise C1C^1 curve and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a continuous vector field. The line integral of F‾\underline{F} along γ‾\underline{\gamma} is the integral of the dot product of F‾\underline{F} with the velocity of the curve.

∫γ‾F‾⋅dr‾:=∫abF‾(γ‾(t))⋅γ‾′(t) dt\int_{\underline{\gamma}}\underline{F}\cdot d\underline{r}:=\int_a^b\underline{F}\left(\underline{\gamma}(t)\right)\cdot\underline{\gamma}'(t)\,dt

The line integral of F‾\underline{F} integrates the component of F‾\underline{F} along the unit tangent vector, ∫γ‾F‾⋅dr‾=∫γ‾F‾⋅T‾ ds,\int_{\underline{\gamma}}\underline{F}\cdot d\underline{r}=\int_{\underline{\gamma}}\underline{F}\cdot\underline{T}\,ds, and is also written ∫γ‾F1 dx1+⋯+Fn dxn.\int_{\underline{\gamma}}F_1\,dx_1+\cdots+F_n\,dx_n. Line integrals have the following properties:

  • both line integrals are unchanged by orientation-preserving reparametrisation;
  • reversing the curve leaves the line integral of a scalar field unchanged and changes the sign of the line integral of a vector field.

Let U⊆RnU\subseteq\mathbb{R}^n be open, γ‾\underline{\gamma} be a closed piecewise C1C^1 curve in UU and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a continuous vector field. The circulation of F‾\underline{F} around γ‾\underline{\gamma} is the line integral of F‾\underline{F} around the closed curve, written ∮γ‾F‾⋅dr‾.\oint_{\underline{\gamma}}\underline{F}\cdot d\underline{r}.

Let U⊆RnU\subseteq\mathbb{R}^n be open and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a vector field. A potential of F‾\underline{F} is a C1C^1 scalar field φ:U→R\varphi:U\rightarrow\mathbb{R} with F‾=∇φ.\underline{F}=\nabla\varphi. The vector field F‾\underline{F} is conservative if and only if it has a potential.

Let U⊆RnU\subseteq\mathbb{R}^n be open, φ:U→R\varphi:U\rightarrow\mathbb{R} be a C1C^1 scalar field and γ‾:[a,b]→U\underline{\gamma}:\left[a,b\right]\rightarrow U be a piecewise C1C^1 curve. The gradient theorem states that the line integral of a gradient field depends only on the endpoints of the curve.

∫γ‾∇φ⋅dr‾=φ(γ‾(b))−φ(γ‾(a))\int_{\underline{\gamma}}\nabla\varphi\cdot d\underline{r}=\varphi\left(\underline{\gamma}(b)\right)-\varphi\left(\underline{\gamma}(a)\right)

Let U⊆RnU\subseteq\mathbb{R}^n be open and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a continuous vector field. The line integral of F‾\underline{F} is path independent if and only if it takes the same value along any two piecewise C1C^1 curves in UU with the same initial and terminal points.

Let U⊆RnU\subseteq\mathbb{R}^n be an open set such that any two points of UU can be joined by a piecewise C1C^1 curve in U,U, and F‾:U→Rn\underline{F}:U\rightarrow\mathbb{R}^n be a continuous vector field. Conservative fields have the following properties:

  • two potentials of F‾\underline{F} differ by a constant;
  • the following are equivalent: F‾\underline{F} is conservative; the line integral of F‾\underline{F} is path independent; the circulation of F‾\underline{F} around every closed piecewise C1C^1 curve in UU is zero;
  • a C1C^1 conservative field on U⊆R3U\subseteq\mathbb{R}^3 is irrotational, and a C1C^1 conservative field on U⊆R2U\subseteq\mathbb{R}^2 has zero scalar curl, since gradient fields are irrotational;
  • the converse fails in general: F‾(x,y)=(−y,x)x2+y2\underline{F}(x,y)=\frac{\left(-y,x\right)}{x^2+y^2} has zero scalar curl on R2∖{0‾}\mathbb{R}^2\setminus\left\{\underline{0}\right\} but circulation 2π2\pi around the unit circle.

Let U⊆RnU\subseteq\mathbb{R}^n be open. The set UU is simply connected if and only if every closed curve in UU can be continuously shrunk within UU to a point. The sets Rn,\mathbb{R}^n, open rectangles and R3\mathbb{R}^3 with a point removed are simply connected, whereas R2\mathbb{R}^2 with a point removed is not. On a simply connected open set every C1C^1 irrotational field is conservative.

Let D⊂R2D\subset\mathbb{R}^2 be a closed bounded region of the kind over which multiple integrals are taken and r‾:D→R3\underline{r}:D\rightarrow\mathbb{R}^3 be C1.C^1. The image S=r‾(D)S=\underline{r}(D) is a parametrised surface with parameters (u,v)∈D.\left(u,v\right)\in D. The partial derivatives r‾u:=∂r‾∂u\underline{r}_u:=\frac{\partial\underline{r}}{\partial u} and r‾v:=∂r‾∂v\underline{r}_v:=\frac{\partial\underline{r}}{\partial v} are tangent to S.S.

Let S=r‾(D)S=\underline{r}(D) be a parametrised surface. The normal vector of SS at r‾(u,v)\underline{r}(u,v) is the cross product r‾u×r‾v,\underline{r}_u\times\underline{r}_v, which is orthogonal to S.S. The surface SS is regular if and only if the normal vector is never zero. The unit normal of a regular surface is the normal vector divided by its length.

n‾:=r‾u×r‾v∥r‾u×r‾v∥\underline{n}:=\frac{\underline{r}_u\times\underline{r}_v}{\lVert\underline{r}_u\times\underline{r}_v\rVert}

Let S=r‾(D)S=\underline{r}(D) be a parametrised surface and ff be a continuous scalar field on an open set containing S.S. The surface area of SS is the integral over DD of the length of the normal vector, which is the area of the parallelogram spanned by the tangent vectors. The surface integral of ff over SS is the integral of ff over the surface weighted by the length of the normal vector.

A(S):=∫D∥r‾u×r‾v∥ d(u,v),∫Sf dS:=∫Df(r‾(u,v))∥r‾u×r‾v∥ d(u,v)A\left(S\right):=\int_D\lVert\underline{r}_u\times\underline{r}_v\rVert\,d(u,v),\qquad\int_S f\,dS:=\int_D f\left(\underline{r}(u,v)\right)\lVert\underline{r}_u\times\underline{r}_v\rVert\,d(u,v)

For example, the graph r‾(u,v)=(u,v,g(u,v))\underline{r}(u,v)=\left(u,v,g(u,v)\right) of a C1C^1 function gg has ∥r‾u×r‾v∥=1+gu2+gv2,\lVert\underline{r}_u\times\underline{r}_v\rVert=\sqrt{1+g_u^2+g_v^2}, and the sphere of radius ρ\rho parametrised by r‾(θ,ϕ)=ρ(sin⁡ϕcos⁡θ,sin⁡ϕsin⁡θ,cos⁡ϕ)\underline{r}(\theta,\phi)=\rho\left(\sin\phi\cos\theta,\sin\phi\sin\theta,\cos\phi\right) on [0,2π]×[0,π]\left[0,2\pi\right]\times\left[0,\pi\right] has ∥r‾θ×r‾ϕ∥=ρ2sin⁡ϕ\lVert\underline{r}_\theta\times\underline{r}_\phi\rVert=\rho^2\sin\phi and surface area 4πρ2.4\pi\rho^2.

Let SS be a regular parametrised surface. The surface SS is orientable if and only if it admits a continuous choice of unit normal. An orientation of an orientable surface is a choice of one of the two continuous unit normal fields ±n‾.\pm\underline{n}. The Möbius strip is not orientable.

Let SS be an oriented surface with unit normal n‾\underline{n} and F‾\underline{F} be a continuous vector field on an open set containing S.S. The flux of F‾\underline{F} through SS is the surface integral of the normal component of F‾.\underline{F}.

∫SF‾⋅n‾ dS=∫DF‾(r‾(u,v))⋅(r‾u×r‾v)d(u,v)\int_S\underline{F}\cdot\underline{n}\,dS=\int_D\underline{F}\left(\underline{r}(u,v)\right)\cdot\left(\underline{r}_u\times\underline{r}_v\right)d(u,v)

Surface area and surface integrals of scalar fields are unchanged by reparametrisation of S,S, and the flux changes sign when the orientation is reversed.

Let SS be a surface in R3.\mathbb{R}^3. The surface SS is closed if and only if it encloses a bounded region of R3,\mathbb{R}^3, such as a sphere. The outward normal of a closed surface is the unit normal that points away from the enclosed region. Flux through a closed surface is written ∮SF‾⋅n‾ dS.\oint_S\underline{F}\cdot\underline{n}\,dS.

Let γ‾\underline{\gamma} be a simple closed curve in R2.\mathbb{R}^2. The Jordan curve theorem states that γ‾\underline{\gamma} separates the plane into exactly two regions, one bounded and one unbounded, of which it is the common boundary.

Let γ‾\underline{\gamma} be a piecewise C1C^1 simple closed curve in R2\mathbb{R}^2 traversed anticlockwise, so that the bounded region DD it encloses lies to its left, and write ∂D\partial D for the curve γ‾.\underline{\gamma}. Let F‾=(F1,F2)\underline{F}=\left(F_1,F_2\right) be a C1C^1 vector field on an open set containing DD and γ‾.\underline{\gamma}. Green’s theorem states that the circulation of F‾\underline{F} around the boundary equals the integral of the scalar curl of F‾\underline{F} over the region.

∮∂DF1 dx+F2 dy=∫D(∂F2∂x−∂F1∂y)d(x,y)\oint_{\partial D}F_1\,dx+F_2\,dy=\int_D\left(\frac{\partial F_2}{\partial x}-\frac{\partial F_1}{\partial y}\right)d(x,y)

Taking F‾=12(−y,x)\underline{F}=\frac{1}{2}\left(-y,x\right) gives the area of DD as 12∮∂Dx dy−y dx.\frac{1}{2}\oint_{\partial D}x\,dy-y\,dx.

Let SS be a regular oriented parametrised surface in R3\mathbb{R}^3 with unit normal n‾.\underline{n}. The boundary curve of S,S, written ∂S,\partial S, is the image of the boundary of DD under r‾,\underline{r}, a piecewise C1C^1 closed curve oriented so that SS lies to the left when walking along ∂S\partial S with head in the direction of n‾.\underline{n}.

Let SS be a regular oriented parametrised surface in R3\mathbb{R}^3 with unit normal n‾\underline{n} and boundary curve ∂S,\partial S, and F‾\underline{F} be a C1C^1 vector field on an open set containing S.S. Stokes’ theorem states that the circulation of F‾\underline{F} around the boundary equals the flux of the curl of F‾\underline{F} through the surface.

∮∂SF‾⋅dr‾=∫S(∇×F‾)⋅n‾ dS\oint_{\partial S}\underline{F}\cdot d\underline{r}=\int_S\left(\nabla\times\underline{F}\right)\cdot\underline{n}\,dS

Green’s theorem is the case of a flat surface in the plane with n‾=e‾3.\underline{n}=\underline{e}_3. The flux of a curl through a closed surface is zero.

Let V⊂R3V\subset\mathbb{R}^3 be a bounded region enclosed by a closed, piecewise regular surface ∂V\partial V with outward normal n‾,\underline{n}, and F‾\underline{F} be a C1C^1 vector field on an open set containing VV and ∂V.\partial V. The divergence theorem states that the flux of F‾\underline{F} out of the region equals the integral of the divergence of F‾\underline{F} over the region.

∮∂VF‾⋅n‾ dS=∫V∇⋅F‾ dx‾\oint_{\partial V}\underline{F}\cdot\underline{n}\,dS=\int_V\nabla\cdot\underline{F}\,d\underline{x}

The divergence theorem holds in Rn\mathbb{R}^n with the surface integral replaced by the integral over the boundary with respect to (n−1)\left(n-1\right)-dimensional area. In R2\mathbb{R}^2 it states that ∮∂DF‾⋅n‾ ds=∫D∇⋅F‾ d(x,y),\oint_{\partial D}\underline{F}\cdot\underline{n}\,ds=\int_D\nabla\cdot\underline{F}\,d(x,y), which is Green’s theorem applied to (−F2,F1).\left(-F_2,F_1\right).

Let V⊂R3V\subset\mathbb{R}^3 be a bounded region enclosed by a closed, piecewise regular surface ∂V\partial V with outward normal n‾,\underline{n}, and f,gf,g be C2C^2 scalar fields on an open set containing VV and ∂V.\partial V. Green’s identities are the divergence theorem applied to f ∇g.f\,\nabla g.

∫V(f Δg+∇f⋅∇g)dx‾=∮∂Vf ∇g⋅n‾ dS\int_V\left(f\,\Delta g+\nabla f\cdot\nabla g\right)d\underline{x}=\oint_{\partial V}f\,\nabla g\cdot\underline{n}\,dS ∫V(f Δg−g Δf)dx‾=∮∂V(f ∇g−g ∇f)⋅n‾ dS\int_V\left(f\,\Delta g-g\,\Delta f\right)d\underline{x}=\oint_{\partial V}\left(f\,\nabla g-g\,\nabla f\right)\cdot\underline{n}\,dS

Let x‾∈R3\underline{x}\in\mathbb{R}^3 and ρ>0.\rho>0. The ball of radius ρ\rho centred at x‾\underline{x} is the set Bρ={y‾∈R3:∥y‾−x‾∥≤ρ},B_\rho=\left\{\underline{y}\in\mathbb{R}^3:\lVert\underline{y}-\underline{x}\rVert\leq\rho\right\}, with volume ∣Bρ∣=43πρ3\lvert B_\rho\rvert=\frac{4}{3}\pi\rho^3 and boundary sphere ∂Bρ.\partial B_\rho. Let v‾\underline{v} be a unit vector and γ‾ρ\underline{\gamma}_\rho be the circle of radius ρ\rho centred at x‾\underline{x} in the plane orthogonal to v‾\underline{v} and traversed anticlockwise about v‾.\underline{v}. By the divergence and Stokes’ theorems with the mean value theorem for integrals, the divergence of a C1C^1 field is its outward flux per unit volume and each component of its curl is its circulation per unit area.

∇⋅F‾(x‾)=lim⁡ρ→01∣Bρ∣∮∂BρF‾⋅n‾ dS,(∇×F‾(x‾))⋅v‾=lim⁡ρ→01πρ2∮γ‾ρF‾⋅dr‾\nabla\cdot\underline{F}(\underline{x})=\lim_{\rho\rightarrow 0}\frac{1}{\lvert B_\rho\rvert}\oint_{\partial B_\rho}\underline{F}\cdot\underline{n}\,dS,\qquad\left(\nabla\times\underline{F}(\underline{x})\right)\cdot\underline{v}=\lim_{\rho\rightarrow 0}\frac{1}{\pi\rho^2}\oint_{\underline{\gamma}_\rho}\underline{F}\cdot d\underline{r}

These limits define the divergence and curl independently of coordinates, so both are unchanged by rotations of the axes.