34
Blazkov.
Bestimmung des Azimuthes.
O
Kreisablesung
Correction
Azimuth
Südpunkt
Azimuth
des Objectes
Object
bX)
c3
Uhrzeit
wegen des Run
wegen
des Sternes
der
exclusive
GG
*s
corrigiert
Neigung
Kreistheilung
Correction der
Collimation
1891. Mai 27. p. m.
a = l l1 18 m 5 ? 6; a = 4- 88° 43' 25*0; * =
l m 12 ? 6;
Ambrozny <>-
R
4°
10’
53*0
Polaris
0
10 h
29 m
15 ? 5
233
40
33-1
4- 1 1
1° 18
10'*3
234° 58' 44'-'4
309° 12' 8*6
IV
10
32
9-0
53
41
40-7
— 2-9
1 17
4-3
54 58 42-1
3-1
Ambrozny -<>•
I,
184
10
45-2
Mittel =
= 309° 12’ 5*85
A a' = — 0 025 Aa* 4-0-994 A8"
1891. Mai 27. p.
in.
a
= 1 U 18 m 5 ? 6;
o =
= + 88 c
43’ 25 v 0;
i m
x = — 1
12*6;
Ambrozny <>-
I,
274°
12'
4"1
Polaris
W
10 h
38 m
19 ? 0
143
45
25-6
- 5*8
1° 14
41 * 5
145° 0' 1*4
309° 12' 2*7
0
10
40
34-5
323
46
10-9
4- 13
1 13
48-4
325 0 0-6
10 7
Ambrozny <>•
R
94
12
11-3
Mittel =
=309° 12' 6*7o
A a' — — 0-026 A a” 4-0*951 A8"
1891. Mai 29. a.
in.
a
= l h 18 m 7 ? 4;
S =
= 4-88°
43’ 24*5;
X
= -l m
10*4;
•
Ambrozny -<>•
R
129°
13’
8 V 4
Polaris
0
21 11
26 m
44 ? 5
1
42
39-1
— 1*3
1° 41
32 *3
0° 1’ 5*4
309° 12' 3*0
w
21
28
58-0
181
41
59-1
4- 5-0
1 40
56-6
180 1 7-5
4-9
Ambrozny
L
309
13
12-4
Mittel =
=309° 12’ 3*95
Aa* =4-0-018 Aa* — 1-340 A8"
1891. Mai 29. a
ni.
a
= l h 18 m 7 ? 4;
8 =
= -h 88°
43’ 24*5;
X
= -l m
10 * 4 ;
Ambrozny -<>•
L
39°
11’
24 "5
Polaris
W
21 h
36 m
14 ? 0
271
38
13-4
4- 0 v 7
1° 38
55*9
269° 59' 18*2
309° 12' 6*3
0
21
38
47-0
91
37
24-9
4- 2-3
1 38
12-0
89 59 15-2
20-0
Ambrozny <>-
R
219
11
35-2
Mittel =
= 309° 12’ 13*15
Aa* = 4-0-019 Aa" — 1-306 A8"
1891. Mai 29. a.
in.
a
= l h 18
m 7 ? 4;
8 =
= + 88°
43’ 24*5;
X
= - l m
10 ? 4
Ambrozny -<>•
R
174°
11'
59-' 8
Polaris
0
21 11
47 m
19 s 5
46
35
27-1
4- 0-1
1° 35
39 *6
44° 59’ 47*6
309° 12’ 12*2
w
21
49
55'5
226
34
39-7
4- 3-7
1 34
51-5
224 59 51-9
6-2
Ambrozny <>-
L
354
11
58-1
Mittel =
= 309° 12’ 9*20
Aa" =4-0-021 Aa" — 1-263 A8"