Geography Reference
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Table 22.26 Simultaneous diagonalization of the matrix pair ( G l , G r ): distortion
characteristic equation
(22.151)
Λ 2 G 11 C 12
Λ 2 G 12
C 11
= 0
(22.152)
Λ 2 G 12 C 22
Λ 2 G 22
C 12
x L + y L
Λ 2 G 11 x L y B + x B y L
x L y B + x B y L x 2 B + y B
= 0
(22.153)
Λ 2 G 22
Λ 4 tr C l G l Λ 2 +det C l G 1
= 0
(22.154)
l
tr C l G l 2
Λ 1 , 2 = Λ 2 ± = 1
1
2
2 tr C l G 1
4det C l G 1
±
(22.155)
l
l
Hilbert invariants
J 1 := tr C l G 1
(22.156)
l
J 2 := det C l G 1
(22.157)
l
the Cayley matrixproduct
= x L + y L G 1
( x L x B + y L y B ) G 1
22
C l G 1
11
x 2 B + y B G 1
(22.158)
l
( x L x B + y L y B ) G 1
11
22
J 1 = tr C l G 1
l
= G 1
11
x L + G 1
x 2 B + G 1
y L + G 1
y B
(22.159)
22
11
22
x L + y L x 2 B + y B
( x L x B + y L y B ) 2
J 2 = G 1
G 1
22
(22.160)
11
Appendix 2
The Euler-Lagrange equation of minimal distortion energy in Gauss surface normal coordinates
Based upon the matrix pair { C l G l } of type “left Cauchy-Green deformation tensor C l ”and
“left metric tensor G l ” given for an oblate ellipsoid-of-revolution E
A 1 ,A 2 by Eqs. ( 22.18 )-( 22.20 ),
and ( 22.32 ) we aim at deriving the stationary point set of distortion energy which is based upon
the Hilbert invariant density tr C l G l of distortion energy which we already encountered in the
eigenspace analysis of the matrix pair
. Outlined in Table 22.30 ,firstwederivetheleft
surface element dS l in terms of Gauss surface normal
{
C l G l }
{
longitude L , latitude B
}
by Eqs. ( 22.191 )and( 22.192 ). Second ,Eqs.( 22.193 )and( 22.194 ) offer a representation of distor-
tion energy density tr C l G l as a Hilbert invariant. The distortion energy, the integral over the
distortion energy density with fixed boundaries ,Eq.( 22.195 ) is additively decomposed
2 ,Eq.( 22.196 ),
into an integral I proportional to
Grad x
2 ,Eq.( 22.197 )!
Such a representation is proven by computing Grad x and Grad y , respectively, in terms of
the left Cartan 2-leg
into an integral II proportional to
Grad y
2 and
2 ,
{
C 1 , C 2
|
X
}
attached to the point X ,aswellas
Grad x
Grad y
respectively, by Eqs.( 22.198 )-( 22.203 ). The first variations
• δ| =0 , Eq.( 22.204 ),
• δ|| =0 , Eq.( 22.205 )
 
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