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Spherical coordinates describe a vector or point in space with
a distance and two angles. The distance, * R*, is
the usual Euclidean norm. There are multiple conventions regarding
the specification of the two angles. They include:

Azimuth and elevation angles

Phi and theta angles

and*u*coordinates*v*

Phased Array System Toolbox™ software natively supports the azimuth/elevation representation. The software also provides functions for converting between the azimuth/elevation representation and the other representations. See Phi and Theta Angles and U and V Coordinates.

In Phased Array System Toolbox software, the predominant convention for spherical coordinates is as follows:

Use the azimuth angle,

, and the elevation angle,*az*, to define the location of a point on the unit sphere.*el*Specify all angles in degrees.

List coordinates in the sequence (

,*az*,*el*).*R*

The *azimuth angle* of
a vector is the angle between the * x*-axis and the
orthogonal projection of the vector onto the

^{®} and Phased Array System Toolbox products do not
use this definition. |

This figure illustrates the azimuth angle and elevation angle for a vector that appears as a green solid line. The coordinate system is relative to the center of a uniform linear array, whose elements appear as blue circles.

As an alternative to azimuth and elevation angles, you can use
angles denoted by φ and θ to express the location of a
point on the unit sphere. To convert the φ/θ representation
to and from the corresponding azimuth/elevation representation, use
coordinate conversion functions, `phitheta2azel`

and `azel2phitheta`

.

The φ angle is the angle from the positive * y*-axis
toward the positive

The figure illustrates φ and θ for a vector that appears as a green solid line. The coordinate system is relative to the center of a uniform linear array, whose elements appear as blue circles.

The coordinate transformations between φ/θ and *az/el* are
described by the following equations

$$\begin{array}{l}\mathrm{sin}(\text{el})=\mathrm{sin}\varphi \mathrm{sin}\theta \hfill \\ \mathrm{tan}(\text{az})=\mathrm{cos}\varphi \mathrm{tan}\theta \hfill \\ \hfill \\ \mathrm{cos}\theta =\mathrm{cos}(\text{el})\mathrm{cos}(\text{az})\hfill \\ \mathrm{tan}\varphi =\mathrm{tan}(\text{el})/\mathrm{sin}(\text{az})\hfill \end{array}$$

In radar applications, it is often useful to parameterize the
hemisphere x ≥ 0 using coordinates denoted by * u* and

To convert the φ/θ representation to and from the corresponding

/*u*representation, use coordinate conversion functions*v*`phitheta2uv`

and`uv2phitheta`

.To convert the azimuth/elevation representation to and from the corresponding

/*u*representation, use coordinate conversion functions*v*`azel2uv`

and`uv2azel`

.

You can define * u* and

$$\begin{array}{l}u=\mathrm{sin}\theta \mathrm{cos}\varphi \\ v=\mathrm{sin}\theta \mathrm{sin}\varphi \end{array}$$

In these expressions, φ and θ are the phi and theta angles, respectively.

In terms of azimuth and elevation, the * u* and

$$\begin{array}{l}u=\mathrm{cos}el\mathrm{sin}az\\ v=\mathrm{sin}el\end{array}$$

The values of * u* and

$$\begin{array}{l}-1\le u\le 1\\ -1\le v\le 1\\ {u}^{2}+{v}^{2}\le 1\end{array}$$

Conversely, the phi and theta angles can be written in terms
of * u* and

$$\begin{array}{l}\mathrm{tan}\varphi =u/v\\ \mathrm{sin}\theta =\sqrt{{u}^{2}+{v}^{2}}\end{array}$$

The azimuth and elevation angles can also be written in terms
of * u* and

$$\begin{array}{l}\mathrm{sin}el=v\\ \mathrm{tan}az=\frac{u}{\sqrt{1-{u}^{2}-{v}^{2}}}\end{array}$$

The following equations define the relationships between rectangular
coordinates and the (* az*,

To convert rectangular coordinates to (* az*,

$$\begin{array}{l}R=\sqrt{{x}^{2}+{y}^{2}+{z}^{2}}\\ az={\mathrm{tan}}^{-1}(y/x)\\ el={\mathrm{tan}}^{-1}(z/\sqrt{{x}^{2}+{y}^{2}})\end{array}$$

To convert (* az*,

$$\begin{array}{l}x=R\mathrm{cos}(el)\mathrm{cos}(az)\\ y=R\mathrm{cos}(el)\mathrm{sin}(az)\\ z=R\mathrm{sin}(el)\end{array}$$

When specifying a target's location with respect to a
phased array, it is common to refer to its distance and direction
from the array. The distance from the array corresponds to * R* in
spherical coordinates. The direction corresponds to the azimuth and
elevation angles.

*Broadside angles* are useful when describing
the response of a uniform linear array (ULA). The array response depends
directly on the broadside angle and not on the azimuth and elevation
angles. Start with a ULA and draw a plane orthogonal to the ULA axis
as shown in blue in the figure. The broadside angle is the angle between
the plane and the signal direction. To compute the broadside angle,
construct a line from any point on the signal path to the plane, orthogonal
to the plane. The angle between these two lines is the broadside angle
and lies in the interval * [–90°,90°]*.
The broadside angle is positive when measured toward the positive
direction of the array axis. Zero degrees indicates a signal path
orthogonal to the array axis. ±90° indicates paths along
the array axis. All signal paths having the same broadside angle form
a cone around the ULA axis.

The conversion from azimuth angle, * az*, and
elevation angle,

$$\beta ={\mathrm{sin}}^{-1}(\mathrm{sin}(az)\mathrm{cos}(el))$$

This equation shows that

For an elevation angle of zero, the broadside angle equals the azimuth angle.

Elevation angles equally above and below the

plane result in identical broadside angles.*xy*

You can convert from broadside angle to azimuth angle but you must specify the elevation angle

$$az={\mathrm{sin}}^{-1}\left(\frac{\mathrm{sin}\beta}{\mathrm{cos}(el)}\right)$$

Because the signals
paths for a given broadside angle, * β*, form
a cone around the array axis, you cannot specify the elevation angle
arbitrarily. The elevation angle and broadside angle must satisfy

$$\left|el\right|+\left|\beta \right|\le 90$$

The following figure depicts a ULA with elements spaced * d* meters
apart. The ULA is illuminated by a plane wave emitted from a point
source in the far field. For convenience, the elevation angle is zero
degrees. In this case, the signal direction lies in the

Because of the angle of arrival, the array elements are not
simultaneously illuminated by the plane wave. The additional distance
the incident wave travels between array elements is * d
sinβ* where

$$\tau =\frac{d\mathrm{sin}\beta}{c},$$

where * c* is the speed of the wave.

For broadside angles of ±90°, the signal is incident
on the array parallel to the array axis and the time delay between
sensors equals * ±d/c*. For a broadside angle
of zero, the plane wave illuminates all elements of the ULA simultaneously
and the time delay between elements is zero.

Phased Array System Toolbox software provides functions `az2broadside`

and `broadside2az`

for
converting between azimuth and broadside angles.

The following examples show how to use the `az2broadside`

and `broadside2az`

functions.

A target is located at an azimuth angle of 45° and at an elevation angle of 60° relative to a ULA. Determine the corresponding broadside angle.

bsang = az2broadside(45,60)

bsang = 20.7048

Calculate the azimuth for an incident signal arriving at a broadside angle of 45° and an elevation of 20°.

az = broadside2az(45,20)

az = 48.8063

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