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Vector fields in cylindrical and spherical coordinates
Encyclopedia
- This page uses standard physics notation. For spherical coordinates,
is the angle between the z axis and the radius vector connecting the origin to the point in question.
is the angle between the projection of the radius vector onto the x-y plane and the x axis. Some (American mathematics) sources reverse this definition.
Vector fields
Vectors are defined in cylindrical coordinates by (r, θ, z), where- r is the length of the vector projected onto the X-Y-plane,
- θ is the angle between the projection of the vector onto the X-Y-plane (i.e. r) and the positive X-axis (0 ≤ θ < 2π),
- z is the regular z-coordinate.
(r, θ, z) is given in cartesian coordinates by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-3.gif)
or inversely by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-4.gif)
Any vector field
Vector field
In vector calculus, a vector field is an assignmentof a vector to each point in a subset of Euclidean space. A vector field in the plane for instance can be visualized as an arrow, with a given magnitude and direction, attached to each point in the plane...
can be written in terms of the unit vectors as:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-5.gif)
The cylindrical unit vectors are related to the cartesian unit vectors by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-6.gif)
- Note: the matrix is an orthogonal matrixOrthogonal matrixIn linear algebra, an orthogonal matrix , is a square matrix with real entries whose columns and rows are orthogonal unit vectors ....
, that is, its inverse is simply its transposeTransposeIn linear algebra, the transpose of a matrix A is another matrix AT created by any one of the following equivalent actions:...
.
Time derivative of a vector field
To find out how the vector field A changes in time we calculate the time derivatives.For this purpose we use Newton's notation for the time derivative (
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-7.gif)
In cartesian coordinates this is simply:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-8.gif)
However, in cylindrical coordinates this becomes:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-9.gif)
We need the time derivatives of the unit vectors.
They are given by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-10.gif)
So the time derivative simplifies to:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-11.gif)
Second time derivative of a vector field
For physical purposes we are usually interested in the second time derivative which tells us something about motions in classical mechanical systems.The second time derivative of a vector field in cylindrical coordinates is given by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-12.gif)
To understand this expression, we substitute A = P, where p is the vector (r, θ, z).
This means that
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-13.gif)
After substituting we get:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-14.gif)
People should recognize this, because we see:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-15.gif)
See also: Centripetal force
Centripetal force
Centripetal force is a force that makes a body follow a curved path: it is always directed orthogonal to the velocity of the body, toward the instantaneous center of curvature of the path. The mathematical description was derived in 1659 by Dutch physicist Christiaan Huygens...
, Angular acceleration
Angular acceleration
Angular acceleration is the rate of change of angular velocity over time. In SI units, it is measured in radians per second squared , and is usually denoted by the Greek letter alpha .- Mathematical definition :...
, Coriolis effect
Coriolis effect
In physics, the Coriolis effect is a deflection of moving objects when they are viewed in a rotating reference frame. In a reference frame with clockwise rotation, the deflection is to the left of the motion of the object; in one with counter-clockwise rotation, the deflection is to the right...
.
Vector fields
Vectors are defined in spherical coordinates by (ρ,θ,φ), where- ρ is the length of the vector,
- θ is the angle between the positive Z-axis and vector in question (0 ≤ θ ≤ π)
- φ is the angle between the projection of the vector onto the X-Y-plane and the positive X-axis (0 ≤ φ < 2π),
(ρ,θ,φ) is given in cartesian coordinates by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-16.gif)
or inversely by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-17.gif)
Any vector field can be written in terms of the unit vectors as:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-18.gif)
The spherical unit vectors are related to the cartesian unit vectors by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-19.gif)
- Note: the matrix is an orthogonal matrixOrthogonal matrixIn linear algebra, an orthogonal matrix , is a square matrix with real entries whose columns and rows are orthogonal unit vectors ....
, that is, its inverse is simply its transposeTransposeIn linear algebra, the transpose of a matrix A is another matrix AT created by any one of the following equivalent actions:...
.
Time derivative of a vector field
To find out how the vector field A changes in time we calculate the time derivatives.In cartesian coordinates this is simply:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-20.gif)
However, in spherical coordinates this becomes:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-21.gif)
We need the time derivatives of the unit vectors.
They are given by:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-22.gif)
So the time derivative becomes:
![](http://image.absoluteastronomy.com/images/formulas/9/3/1936519-23.gif)
See also
- Del in cylindrical and spherical coordinatesDel in cylindrical and spherical coordinatesThis is a list of some vector calculus formulae of general use in working with various curvilinear coordinate systems.- Note :* This page uses standard physics notation. For spherical coordinates, \theta is the angle between the z axis and the radius vector connecting the origin to the point in...
for the specification of gradientGradientIn vector calculus, the gradient of a scalar field is a vector field that points in the direction of the greatest rate of increase of the scalar field, and whose magnitude is the greatest rate of change....
, divergenceDivergenceIn vector calculus, divergence is a vector operator that measures the magnitude of a vector field's source or sink at a given point, in terms of a signed scalar. More technically, the divergence represents the volume density of the outward flux of a vector field from an infinitesimal volume around...
, curl, and laplacian in various coordinate systems.