| Revision as of 15:51, 25 February 2002 editConversion script (talk | contribs)10 editsm Automated conversion← Previous edit | Revision as of 16:29, 30 May 2002 edit undo209.206.138.69 (talk)No edit summaryNext edit → | ||
| Line 5: | Line 5: | ||
| === Circular Polar Coordinates === | === Circular Polar Coordinates === | ||
| A two-dimensional coordinate system, defined by an origin, <i>O</i>, and a semi-infinite line <i>L</i> leading from this point. (In terms of the ], the origin (0,0) and the positive x-axis). | A two-dimensional coordinate system, defined by an origin, <i>O</i>, and a semi-infinite line <i>L</i> leading from this point. (In terms of the ], the origin (0,0) and the positive x-axis). In other words, this axis (called the polar axis) is like the right half of the x-axis. | ||
| A point P is then located by its distance from the origin and the angle between line <i>L</i> and OP, measured anti-clockwise. The co-ordinates are typically denoted <i>r</i> and <i>θ</i> respectively: the point P is then (<i>r</i>, <i>θ</i>). | A point P is then located by its distance from the origin and the angle between line <i>L</i> and OP, measured anti-clockwise. The co-ordinates are typically denoted <i>r</i> and <i>θ</i> respectively: the point P is then (<i>r</i>, <i>θ</i>). | ||
Revision as of 16:29, 30 May 2002
Polar coordinate systems are coordinate systems in which a point is identified by a distance from some fixed feature in space and one or more subtended angles.
The principal types of polar co-ordinate systems are listed below.
Circular Polar Coordinates
A two-dimensional coordinate system, defined by an origin, O, and a semi-infinite line L leading from this point. (In terms of the Cartesian coordinate system, the origin (0,0) and the positive x-axis). In other words, this axis (called the polar axis) is like the right half of the x-axis.
A point P is then located by its distance from the origin and the angle between line L and OP, measured anti-clockwise. The co-ordinates are typically denoted r and θ respectively: the point P is then (r, θ).
Cylindrical Polar Coordinates
A three-dimensional system which essentially extends circular polar coordinates by adding a third co-ordinate (usually denoted h) which measures the height of a point above the plane.
A point is given as (r, θ, h). In terms of the Cartesian system:
- r is the distance from O to P', the projection of the point P onto the XY plane,
- θ is the angle between the positive x-axis and line OP', measured anti-clockwise
- h is the same as z.
Some mathematicians indeed use (r, θ, z), especially if working with both systems to, to emphasise this.
Spherical Polar Coordinates
This system is another way of extending the circular polar system to three dimensions, defined by a line in a plane and a line perpendicular to the plane. (The x-axis in the XY plane and the z-axis.)
For a point P, the distance co-ordinate is the distance OP, not the projection. It is sometimes notated r but often ρ (Greek letter rho) is used to emphasise that it is in general different to the r of cylindrical co-ordinates.
The remaining two co-ordinates are both angles: θ is the anti-clockwise between the x-axis and the line OP', where P' is the projection of P in the XY-axis. The angle φ, measures the angle between the vertical line and the line OP.
In this system, a point is then given as (ρ, φ, θ).
Note that r = ρ only in the XY plane, that is when φ= π/2 or h=0.
See also: