Maydenberg.
Bestimmung des Azimuthes.
121
<V
Korrektion
Azimuth
Südpunkt
Azimuth
des Objektes
Objekt
bß
Uhrzeit
Kreisablesung
wegen
der
exklusive
GO
*53
ui
M
Neigung
des Sternes
Kreisteilung
Korrektion der
Kollimation
1891. Juli 1. p. m. a = l h 18 m 36 ? 5; 8 = 4-88° 43’ 22*3; a; = 4-3 m 3 ? 9;
Rapotic -<y
Polaris
]j
W
13 h 40 m 44 18 5
96° 51' 8*0
135 11 15-0
— 3*6
0° 12’ 28*1
0
42 35-5
315 12 19-5
— 3-6
13 22-8
Rapotic <>-
R
276 51 16-8
314° 58' 43-3 141° 52' 24-7
134 58 53-1 23-7
Mittel = 141° 52' 24*20
A a" = — 0-034 Aa” —0-153 AS'
1891. Juli
2.
P-
m.
a = l“
18 m 37 ? 6;
8 = 4-88° 43'
22*4;
a? = 4- 3 m 4*2;
Rapotic -<>- .. .
R
171° 52’
5*0
Polaris
O
1 l h
26 m
4 ? 0
209 7
20-1
4-
0*6
0° 52' 22*6
29°
59' 43*3
141° 52’ 21*7
w
31
30-5
29 9
27-5
4-
4-1
49 56-9
209
59 28-4
22-4
Rapotic
L
351 51
50-8
Mittel =
= 141° 52' 22*05
A a"
= — 0-030Aa’ 4- 0-701 Aô”
1891. Juli
2.
P-
m.
i h
a = 1
18 m 37 ? 6;
8 = 4-88° 43'
22*4;
x = 4-3 m 4*3 ;
Rapotic <>■.. .
R
ll h
261° 52'
46*1
Polaris
O
49 ln
48 ? 5
299 18
50-6
—
1*2
0° 41' 35*5
120°
0’ 24-9
141° 52' 21*2
w
52
10
119 19
37-9
—
0-8
40 33-9
300
0 11-0
221
Rapotic -$>•
L
81 52
33-1
Mittel =
= 141° 52' 21*65
A a’
= — 0-031 Aa’ 4- 0-568 A8”
1891. Juli 2. p. m. a = l h 18 m 37 ? 6; 8 = +88° 43’ 22*4; i * = 4-3 m 4 ? 3;
Eapotic -<>-
Polaris
L
W
ll h 58 ra 36 ? 0
36° 51’ 21*0
74 21 35-0
— 3*9
0° 37' 29*2
254° 59' 0*3
141° 52’ 20*8
0
12 1 9-0
254 22 59-6
— 2-1
36 17-2
74 59 14-7
19-1
Rapotic <>-
R
216 51 33-8
Mittel = 141° 52' 19*95
Aa’ = - 0-032 Aa’ 4-0-512 A8*
1891. Juli 2. p. m.
a = l h 18 m 37 ? 6; 8 = 4-88° 43’ 22-4; &• = 4-3 m 4‘ 3-,
Rapotic -<►
Polaris
R
O
12 h 9 m 30 ? 5
306° 51’ 0*0
344 26 26-8
- 8*5
0° 32' 19*3
164° 58’ 37*6
141° 52' 22*4
n
W
11 550
164 27 17-8
— 41
31 10-3
341 58 24-0
22-0
Rapotic -<>-
L
126 50 46-0
Mittel = 141° 52’ 22*20
Aa* = -0-032 Aa” 4-0*441 A8'
Astron.-geodät. Arbeiten. Band XX.
16
