This system is that which was adopted in 1803 by the "Dépôt de la
Guerre" for the map of France, and is there known by the title of
_Projection de Bonne_. It is that on which the ordnance survey map of
Scotland on the scale of 1 in. to a mile is constructed, and it is
frequently met with in ordinary atlases. It is ill-adapted for countries
having great extent in longitude, as the intersections of the meridians
and parallels become very oblique--as will be seen on examining the map
of Asia in most atlases.
If [phi]0 be taken as the latitude of the centre parallel, and
co-ordinates be measured from the intersection of this parallel with
the central meridian, then, if [rho] be the radius of the parallel of
latitude [phi], we have [rho] = cot [phi]0 + [phi]0 - [phi]. Also, if
S be a point on this parallel whose co-ordinates are x, y, so that VS
= [rho], and [theta] be the angle VS makes with the central meridian,
then [rho][theta] = [omega] cos [phi]; and x = [rho] sin [theta], y =
cot [phi]0 - [rho] cos [theta].
The projection has the property of equal areas, since each small element
bounded by two infinitely close parallels is equal in length and width
to the corresponding element on the sphere or spheroid. Also all the
meridians cross the chosen parallel (but no other) at right angles,
since in the immediate neighbourhood of that parallel the projection is
identical with the simple conical projection. Where an equal-area
projection is required for a country having no great extent in
longitude, such as France, Scotland or Madagascar, this projection is a
good one to select.
[Illustration: FIG. 19.--Sinusoidal Equal-area Projection.]
_Sinusoidal Equal-area Projection._--This projection, which is
sometimes known as Sanson's, and is also sometimes incorrectly called
Flamsteed's, is a particular case of Bonne's in which the selected
parallel is the equator. The equator is a straight line at right angles
to the central meridian which is also a straight line. Along the central
meridian the latitudes are marked off at the true rectified distances,
and from points so found the parallels are drawn as straight lines
parallel to the equator, and therefore at right angles to the central
meridian. True rectified lengths are marked along the parallels and
through corresponding points the meridians are drawn. If the earth is
treated as a sphere the meridians are clearly sine curves, and for this
reason d'Avezac has given the projection the name sinusoidal. But it is
equally easy to plot the spheroidal lengths. It is a very suitable
projection for an equal-area map of Africa.
Public-domain text, read in full here on John Shaqi.
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