656 J Gauss surface normal coordinates in geometry and gravity space
α = arctan
1 − E 2
12 tan Λ
, r = A 1
1 − E 2
12 sin
2 Λ E
⎛
⎝
E 2
13 − E 2
12 sin
2 Λ
1 − E 2
12 sin
2 Λ
,
π
2
⎞
⎠ . (J.90)
Important!
Important references are M. Bursa (1989a,b), B. Eitschberger (1978), E. Grafarend and
P. Lohse (1991), B. Heck (2002), W. Klingenberg (1982), L. P. Lee (1965), H. Merkel (1956),
B. M¨ uler (1991), G. Schliephake (1955, 1956), H. Schmehl (1927, 1930), J. P. Snyder (1985),
H. Viesel (1971), J. A. Weightman (1961) and S. C. Wu (1981).
α = arctan
1 − E 2
12 tan Λ
, r = A 1
1 − E 2
12 sin
2 Λ E
⎛
⎝
E 2
13 − E 2
12 sin
2 Λ
1 − E 2
12 sin
2 Λ
,
π
2
⎞
⎠ . (J.90)
Important!
Important references are M. Bursa (1989a,b), B. Eitschberger (1978), E. Grafarend and
P. Lohse (1991), B. Heck (2002), W. Klingenberg (1982), L. P. Lee (1965), H. Merkel (1956),
B. M¨ uler (1991), G. Schliephake (1955, 1956), H. Schmehl (1927, 1930), J. P. Snyder (1985),
H. Viesel (1971), J. A. Weightman (1961) and S. C. Wu (1981).