Kohout.
Bestimmung des Azimuthes.
G9
1
G>
Kreisablesung
Korrektion
Azimuth
Südpunkt
Azimuth
des Objektes
Objekt
jf
m
’S
W
Uhrzeit
wegen des Run
korrigiert
wegen
Neigung
des Sternes
der
Kreisteilung
exklusive
Korrektion der
Kollimation
1890. September 19. p. m. a = l h 19 m 24 ? 2; § = + 88° 43’ 18*9; : r = + 2 m 42 ? 3.
Vëternik (Heliotrop)
Polaris
L
W
16 h 29 ra 20 ? 0
75° 8' 9*9
76 23 42-4
4- 0-2
1° 25' 13*8
254° 58’ 28''8
H- 1
OD
O
O
50
1— 1
0
31 46-0
256 24 19-7
4- 5-5
26 3-2
74 58 22-0
47-9
Vëternik (Heliotrop)
R
255 8 9-9
Mittel =
Aa* = — 0-023
= 180° 9' 44*50
A a" —1-136 A3"
1890. September 19. p. m. a = l h 19 m 24 ? 2; 8 = 4- 88° 43' 18*9; * = 4-2 m 42 ? 3.
Vëternik (Heliotrop)
Polaris
R
0
16 h 36 m 44 ? 5
345° 8’ 46*7
346 26 39-8
4- 1*8
1° 27' 42*3
164° 58' 59-3
180° 9’ 47*4
W
38 59-5
166 27 28-9
4- 1-8
28 26-4
344 59 4*4
42-4
Vëternik (Heliotrop)
L
165 8 46-7
Mittel =
A a’ = — 0-022
= 180° 9’ 44*90
4 a" — 1-167 AS"
1890. September 19. p. m. a = l h 19 m 24 ? 2; §= + 88° 43' 18*9; x = 2 m 42 ? 3.
Vëternik (Heliotrop)
L
60°
8’
31*9
Polaris
W
16 h 43 m
31 ? 0
61
28
45-0
—
0*8
1° 29'
53*5
239° 58’ 50*7
180° 9’ 41*2
0
45
40-5
241
29
11-2
4-
6-0
30
34-4
59 58 42-8
45-1
Vëternik (Heliotrop)
R
240
8
27-9
Mittel =
= 180° 9 43*15
A«’ = — 0-021
A a” —1-195 A3"
1890. September 19. p
m. a = l h 19 m 24*2
8
= 4-88° 43’
18*9;
x = 4“ 2 m 42 ? 3.
Vëternik (Heliotrop)
R
330°
9’
0*8
Polaris
0
16 h 50 m
29 ? 5
331
31
17-1
4-
2*6
1° 32’
3*9
149° 59’ 15*8
180° 9’ 45*0
w
52
20-5
151
31
55-4
4-
3-3
37-7
329 59 21-0
43-1
Vëternik (Heliotrop)
L
150
9
4-1
Mittel =
= 180° 9' 44*05
Ad’ = — 0-020
A a" — 1-222 AS"
1890. September 19. p.
m.
= l h 19 m 24 ? S;
S
= 4-88° 43'
18*9;
a; = 4- 2 m
42 ? 3.
Vëternik (Heliotrop)
I,
105°
8’
39*0
Polaris
W
16 h 56 m
51 ? 5
106
32
58-4
—
0*6
1° 33’
58*7
284° 58' 59*1
180° 9' 39*9
n • *
0
58
47-5
286
33
19-0
7 0
34
32-7
104 58 53-3
47-7
Vëternik (Heliotrop)
R
285
8
41 -0
Mittel =
= 180° 9' 43*80
A a" = — 0-020
A a" —1-247 AS"
