
In the above two images, the scalar field is in black and white, black representing higher values, and its corresponding gradient is represented by blue arrows.
In
vector calculus, the
gradient of a
scalar field is a
vector field which points in the direction of the greatest rate of increase of the scalar field, and whose
magnitude is the greatest rate of change.
A generalization of the gradient for functions on a
Euclidean space which have values in another Euclidean space is the
Jacobian. A further generalization for a function from one
Banach space to another is the
Fréchet derivative.
Interpretations
For instance, consider a room in which the temperature is given by a scalar field
, so at each point
the temperature is
(we will assume that the temperature does not change in time). Then, at each point in the room, the gradient of
at that point will show the direction in which the temperature rises most quickly. The magnitude of the gradient will determine how fast the temperature rises in that direction.
Consider a surface whose height above sea level at a point
is
. The gradient of
at a point is a vector pointing in the direction of the steepest
slope or
grade at that point. The steepness of the slope at that point is given by the magnitude of the gradient vector.
The gradient can also be used to measure how a scalar field changes in other directions, rather than just the direction of greatest change, by taking a
dot product. Consider again the example with the hill and suppose that the steepest slope on the hill is 40%. If a road goes directly up the hill, then the steepest slope on the road will also be 40%. If, instead, the road goes around the hill at an angle (the gradient vector), then it will have a shallower slope. For example, if the angle between the road and the uphill direction, projected onto the horizontal plane, is 60°, then the steepest slope along the road will be 20%, which is 40% times the
cosine of 60°.
This observation can be mathematically stated as follows. If the hill height function
is differentiable, then the gradient of
dotted with a unit
vector gives the slope of the hill in the direction of the vector. More precisely, when
is differentiable, the dot product of the gradient of
with a given unit vector is equal to the
directional derivative of
in the direction of that unit vector.
Definition

The gradient of the function f(x,y) = −(cos2x + cos2y)2 depicted as a vector field on the bottom plane
The gradient (or gradient vector field) of a scalar function
is denoted
or
where
(the
nabla symbol) denotes the vector
differential operator,
del. The notation
is also used for the gradient. The gradient of
f is defined to be the
vector field whose components are the
partial derivatives of
. That is:
Here the gradient is written as a
row vector, but it is often taken to be a
column vector. When a function also depends on a parameter such as time, the gradient often refers simply to the vector of its spatial derivatives only.
Expressions in three dimensions
The form of the gradient depends on the coordinate system used. In
Cartesian coordinates, the above expression expands to
\left(\frac{\partial f}{\partial x},
\frac{\partial f}{\partial y},
\frac{\partial f}{\partial z}\right)
which is often written using the standard
vectors
:
\frac{\partial f}{\partial y} \hat{\mathbf{j}} +
\frac{\partial f}{\partial z} \hat{\mathbf{k}}
In
cylindrical coordinates, the gradient is given by :
\frac{\partial f}{\partial \rho}\mathbf{e}_\rho+
\frac{1}{\rho}\frac{\partial f}{\partial \theta}\mathbf{e}_\theta+
\frac{\partial f}{\partial z}\mathbf{e}_z
where
is the azimuthal angle,
is the axial coordinate, and
eρ,
eθ and
ez are unit vectors pointing along the coordinate directions.
In
spherical coordinates :
\frac{\partial f}{\partial r}\mathbf{e}_r+
\frac{1}{r}\frac{\partial f}{\partial \theta}\mathbf{e}_\theta+
\frac{1}{r \sin\theta}\frac{\partial f}{\partial \phi}\mathbf{e}_\phi
where
is the
azimuth angle and
is the
zenith angle.
Example
For example, the gradient of the function in Cartesian coordinates
is:
\frac{\partial f}{\partial x},
\frac{\partial f}{\partial y},
\frac{\partial f}{\partial z}\right)
= \left( 2, 6y, -\cos(z)\right).
Gradient and the derivative or differential
Linear approximation to a function
The gradient of a
function from the
Euclidean space to
at any particular point
x0 in
characterizes the best
linear approximation to
f at
x0. The approximation is as follows:
for
close to
, where
is the gradient of
f computed at
, and the dot denotes the
dot product on
. This equation is equivalent to the first two terms in the multi-variable
Taylor Series expansion of
f at
x0.
Differential or (exterior) derivative
The best linear approximation to a function
at a point
in
is a linear map from
to
which is often denoted by
or
and called the
differential or
(total) derivative of
at
. The gradient is therefore related to the differential by the formula
for any
. The function
, which maps
to
, is called the differential or
exterior derivative of
and is an example of a
differential 1-form.
If
is viewed as the space of (length
) column vectors (of real numbers), then one can regard
as the row vector
so that
is given by matrix multiplication. The gradient is then the corresponding column vector, i.e.,
.
Gradient as a derivative
Let
U be an
open set in
Rn. If the function
f:
U →
R is
differentiable, then the differential of
f is the
(Fréchet) derivative of
f. Thus
is a function from
U to the space
R such that
where • is the dot product.
As a consequence, the usual properties of the derivative hold for the gradient:
Linearity
The gradient is linear in the sense that if
f and
g are two real-valued functions differentiable at the point
a∈
Rn, and α and β are two constants, then α
f+β
g is differentiable at
a, and moreover
Product rule
If
f and
g are real-valued functions differentiable at a point
a∈
Rn, then the
product rule asserts that the product (
fg)(
x) =
f(
x)
g(
x) of the functions
f and
g is differentiable at
a, and
Chain rule
Suppose that
f:
A→
R is a real-valued function defined on a subset
A of
Rn, and that
f is differentiable at a point
a. There are two forms of the chain rule applying to the gradient. First, suppose that the function
g is a
parametric curve; that is, a function
g :
I →
Rn maps a subset
I ⊂
R into
Rn. If
g is differentiable at a point
c ∈
I such that
g(
c) =
a, then
More generally, if instead
I⊂
Rk, then the following holds:
where (
Dg)
T denotes the transpose
Jacobian matrix.
For the second form of the chain rule, suppose that
h :
I →
R is a real valued function on a subset
I of
R, and that
h is differentiable at the point
c =
f(
a) ∈
I. Then
Transformation properties
Although the gradient is defined in term of coordinates, it is
contravariant under the application of an
orthogonal matrix to the coordinates. This is true in the sense that if
A is an orthogonal matrix, then
which follows by the chain rule above. A vector transforming in this way is known as a
contravariant vector, and so the gradient is a special type of
tensor.
The differential is more natural than the gradient because it is invariant under all coordinate transformations (or
diffeomorphisms), whereas the gradient is only invariant under orthogonal transformations (because of the implicit use of the dot product in its definition). Because of this, it is common to blur the distinction between the two concepts using the notion of
covariant and contravariant vectors. From this point of view, the components of the gradient transform covariantly under changes of coordinates, so it is called a covariant vector field, whereas the components of a vector field in the usual sense transform contravariantly. In this language the gradient
is the differential, as a covariant vector field is the same thing as a differential 1-form.
Further properties and applications
Level sets
If the partial derivatives of
f are continuous, then the
dot product of the gradient at a point
x with a vector
v gives the
directional derivative of
f at
x in the direction
v. It follows that in this case the gradient of
f is
orthogonal to the
level sets of
f. For example, a level surface in three-dimensional space is defined by an equation of the form
F(
x,
y,
z) =
c. The gradient of
F is then normal to the surface.
More generally, any
embedded hypersurface in a Riemannian manifold can be cut out by an equation of the form
F(
P) = 0 such that
dF is nowhere zero. The gradient of
F is then normal to the hypersurface.
Conservative vector fields
The gradient of a function is called a gradient field. A (continuous) gradient field is always a
conservative vector field: its
line integral along any path depends only on the endpoints of the path, and can be evaluated by the
gradient theorem (the fundamental theorem of calculus for line integrals). Conversely, a (continuous) conservative vector field is always the gradient of a function.
Riemannian manifolds
For any smooth function f on a
Riemannian manifold (
M,
g), the gradient of
f is the
vector field such that for any vector field
,
where
denotes the
inner product of tangent vectors at
x defined by the metric
g and
(sometimes denoted
X(
f)) is the function that takes any point
x∈
M to the
directional derivative of
f in the direction
X, evaluated at
x. In other words, in a
coordinate chart from an open subset of
M to an open subset of
Rn,
is given by:
where
Xj denotes the
jth component of
X in this coordinate chart.
So, the local form of the gradient takes the form:
Generalizing the case
M=
Rn, the gradient of a function is related to its
exterior derivative, since
. More precisely, the gradient
is the vector field associated to the differential 1-form d
f using the
musical isomorphism (called "sharp") defined by the metric
g. The relation between the exterior derivative and the gradient of a function on
Rn is a special case of this in which the metric is the flat metric given by the dot product.
See also