Geography Reference
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E 2 A 1 ,A 2 to p
T N E 2 A 1 ,A 2 , perspective center S
Fig. 8.5. Stereographic projection of P
8-23 Equiareal Mapping
Let us postulate an equiareal mapping of the ellipsoid-of-revolution onto a tangential plane at the
North Pole by means of the measure Λ 1 Λ 2 = 1. The details of such a mapping are collected in
Box 8.7 . At first, we have to start from the canonical postulate of an equiareal mapping ,namely
Λ 1 Λ 2 =1or f ( Δ )(1
E 2 cos 2 Δ ) 1 / 2 f ( Δ )(1
E 2 cos 2 Δ ) 3 / 2 / ( A 1 sin Δ (1
E 2 )) = 1, an equation
solved for f d f = A 1 (1
E 2 cos 2 Δ ) 2 . Direct integration leads to f 2 / 2asan
integral solved by“integration-by-parts”. Four integrals leads us to the final integral f 2 / 2asa
function of (i) ln[(1 + E cos Δ ) / (1
E 2 )sin Δ d Δ/ (1
E cos Δ ), and (iii) 1 / (1 + E cos Δ ). By
the postulate f ( Δ = 0) = 0, we then gauge the integration constant c . In summary, we get the
mapping equations f ( Δ )and f ( Φ ), or (( α = A, r = f ( Δ )), or ( x = f ( Φ )cos Λ, y = f ( Φ )sin Λ ).
The left principal stretches and the left eigenvectors are collected in Box 8.7 by ( 8.73 )andby( 8.74 ).
We finally conclude with the left maximal angular distortion ( 8.75 ).
E cos Δ )], (ii) 1 / (1
Lemma 8.11 (Normal mapping: ellipsoid-of-revolution to plane, equiareal mapping).
The equiareal mapping of the ellipsoid-of-revolution to the tangential plane at the North Pole is
parameterized by
x = f ( Δ )cos Λ,
(8.65)
y = f ( Δ )sin Λ.
subject to the left Cauchy-Green eigenspace
. The radial function r = f ( Φ )
that represents an equiareal mapping is given as a four terms integral in a closed form.
{
E Λ Λ 1 ( Φ ) , E Φ Λ 2 ( Φ )
}
End of Lemma.
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