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CLASS="SECT1"
><H1
CLASS="SECT1"
><A
NAME="EARTHDISTANCE"
>F.13. earthdistance</A
></H1
><P
> The <TT
CLASS="FILENAME"
>earthdistance</TT
> module provides two different approaches to
calculating great circle distances on the surface of the Earth. The one
described first depends on the <TT
CLASS="FILENAME"
>cube</TT
> module (which
<SPAN
CLASS="emphasis"
><I
CLASS="EMPHASIS"
>must</I
></SPAN
> be installed before <TT
CLASS="FILENAME"
>earthdistance</TT
> can be
installed). The second one is based on the built-in <TT
CLASS="TYPE"
>point</TT
> data type,
using longitude and latitude for the coordinates.
</P
><P
> In this module, the Earth is assumed to be perfectly spherical.
(If that's too inaccurate for you, you might want to look at the
<SPAN
CLASS="APPLICATION"
><A
HREF="http://postgis.net/"
TARGET="_top"
>PostGIS</A
></SPAN
>
project.)
</P
><DIV
CLASS="SECT2"
><H2
CLASS="SECT2"
><A
NAME="AEN148077"
>F.13.1. Cube-based Earth Distances</A
></H2
><P
> Data is stored in cubes that are points (both corners are the same) using 3
coordinates representing the x, y, and z distance from the center of the
Earth. A domain <TT
CLASS="TYPE"
>earth</TT
> over <TT
CLASS="TYPE"
>cube</TT
> is provided, which
includes constraint checks that the value meets these restrictions and
is reasonably close to the actual surface of the Earth.
</P
><P
> The radius of the Earth is obtained from the <CODE
CLASS="FUNCTION"
>earth()</CODE
>
function. It is given in meters. But by changing this one function you can
change the module to use some other units, or to use a different value of
the radius that you feel is more appropriate.
</P
><P
> This package has applications to astronomical databases as well.
Astronomers will probably want to change <CODE
CLASS="FUNCTION"
>earth()</CODE
> to return a
radius of <TT
CLASS="LITERAL"
>180/pi()</TT
> so that distances are in degrees.
</P
><P
> Functions are provided to support input in latitude and longitude (in
degrees), to support output of latitude and longitude, to calculate
the great circle distance between two points and to easily specify a
bounding box usable for index searches.
</P
><P
> The provided functions are shown
in <A
HREF="earthdistance.html#EARTHDISTANCE-CUBE-FUNCTIONS"
>Table F-6</A
>.
</P
><DIV
CLASS="TABLE"
><A
NAME="EARTHDISTANCE-CUBE-FUNCTIONS"
></A
><P
><B
>Table F-6. Cube-based Earthdistance Functions</B
></P
><TABLE
BORDER="1"
CLASS="CALSTABLE"
><COL><COL><COL><THEAD
><TR
><TH
>Function</TH
><TH
>Returns</TH
><TH
>Description</TH
></TR
></THEAD
><TBODY
><TR
><TD
><CODE
CLASS="FUNCTION"
>earth()</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Returns the assumed radius of the Earth.</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>sec_to_gc(float8)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Converts the normal straight line
(secant) distance between two points on the surface of the Earth
to the great circle distance between them.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>gc_to_sec(float8)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Converts the great circle distance between two points on the
surface of the Earth to the normal straight line (secant) distance
between them.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>ll_to_earth(float8, float8)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>earth</TT
></TD
><TD
>Returns the location of a point on the surface of the Earth given
its latitude (argument 1) and longitude (argument 2) in degrees.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>latitude(earth)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Returns the latitude in degrees of a point on the surface of the
Earth.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>longitude(earth)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Returns the longitude in degrees of a point on the surface of the
Earth.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>earth_distance(earth, earth)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Returns the great circle distance between two points on the
surface of the Earth.
</TD
></TR
><TR
><TD
><CODE
CLASS="FUNCTION"
>earth_box(earth, float8)</CODE
></TD
><TD
><TT
CLASS="TYPE"
>cube</TT
></TD
><TD
>Returns a box suitable for an indexed search using the cube
<TT
CLASS="LITERAL"
>@></TT
>
operator for points within a given great circle distance of a location.
Some points in this box are further than the specified great circle
distance from the location, so a second check using
<CODE
CLASS="FUNCTION"
>earth_distance</CODE
> should be included in the query.
</TD
></TR
></TBODY
></TABLE
></DIV
></DIV
><DIV
CLASS="SECT2"
><H2
CLASS="SECT2"
><A
NAME="AEN148149"
>F.13.2. Point-based Earth Distances</A
></H2
><P
> The second part of the module relies on representing Earth locations as
values of type <TT
CLASS="TYPE"
>point</TT
>, in which the first component is taken to
represent longitude in degrees, and the second component is taken to
represent latitude in degrees. Points are taken as (longitude, latitude)
and not vice versa because longitude is closer to the intuitive idea of
x-axis and latitude to y-axis.
</P
><P
> A single operator is provided, shown
in <A
HREF="earthdistance.html#EARTHDISTANCE-POINT-OPERATORS"
>Table F-7</A
>.
</P
><DIV
CLASS="TABLE"
><A
NAME="EARTHDISTANCE-POINT-OPERATORS"
></A
><P
><B
>Table F-7. Point-based Earthdistance Operators</B
></P
><TABLE
BORDER="1"
CLASS="CALSTABLE"
><COL><COL><COL><THEAD
><TR
><TH
>Operator</TH
><TH
>Returns</TH
><TH
>Description</TH
></TR
></THEAD
><TBODY
><TR
><TD
><TT
CLASS="TYPE"
>point</TT
> <TT
CLASS="LITERAL"
><@></TT
> <TT
CLASS="TYPE"
>point</TT
></TD
><TD
><TT
CLASS="TYPE"
>float8</TT
></TD
><TD
>Gives the distance in statute miles between
two points on the Earth's surface.
</TD
></TR
></TBODY
></TABLE
></DIV
><P
> Note that unlike the <TT
CLASS="TYPE"
>cube</TT
>-based part of the module, units
are hardwired here: changing the <CODE
CLASS="FUNCTION"
>earth()</CODE
> function will
not affect the results of this operator.
</P
><P
> One disadvantage of the longitude/latitude representation is that
you need to be careful about the edge conditions near the poles
and near +/- 180 degrees of longitude. The <TT
CLASS="TYPE"
>cube</TT
>-based
representation avoids these discontinuities.
</P
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