Now if [sigma][sigma]´ = 1 the areas are correctly represented, then

h[rho] d[rho] = sin z dz, and integrating ½h[rho]² = C - cos z; (i.)

this gives the whole group of _equal-area conical projections_.

As a special case let the pole be the centre of the projected

parallels, then when

z = 0, [rho] = 0, and const = 1, we have p = 2 sin ½z/[delta]h (ii.)

Let z1 be the co-latitude of some parallel which is to be correctly

represented, then 2h sin ½z1/[delta]h = sin z1, and h = cos² ½z1;

putting this value of h in equation (ii.) the radius of any parallel

= [rho] = 2 sin ½z sec ½z1 (iii.)

This is Lambert's _conical equal-area projection with one standard

parallel_, the pole being the centre of the parallels.

If we put z1 = [theta], then h = 1, and the meridians are inclined at

their true angles, also the scale at the pole becomes correct, and

equation (iii.) becomes

[rho] = 2 sin ½z; (iv.)

this is the _zenithal equal-area projection_.

Encyclopaedia Britannica, 11th Edition, "Map" to "Mars" Volume 17, Slice 6 · 第 19 / 41 题