Blazkov.
Bestimmung des Azimuthes.
35
Object
Kreisablesung
Correction
Azimuth
des Sternes
Südpunkt
©
bf)
c3
Uhrzeit
wegen des Run
wegen
der
’S
corri giert
Neigung
Kreistheilung
HH
Azimuth
des Objectes
exclusive
Correction der
Collimation
1891. Mai 29. a.
m.
a = l h 18 m 7 ? 5-, 8 = 4- 88 c
43’ 245; *
= - I ra 10 ? 4;
Ambrozny -c>
L
84° 11' 45*4
Polaris
W
22 h 0“ 31 ? 0
316 31 5-4
H— 1 * o
1° 31' 27 v 9
314° 59' 39*0
309° 12' 6 V 4
0
22 3 16-5
136 30 7-2
4- 2-7
1 30 32-8
134 59 37-2
7-7
Ambrozny <>•
R
264 11 44-9
Mittel =
= 309° 12’ 7 -05
Aa" = + 0-022 Aa" — U209A8"
1891. Mai 29. a.
in.
0t
= l h
18 m 7*5;
8 =
= + 88 c
43'
24 ? 5;
® = - l m 10*4;
Ambrozny -5-
R
159°
11'
30'-'5
Polaris
0
22 h
10 m
43 ? 0
31
27
19-0
+
0 V 4
1° 28’ 0'-'l
29° 59' 19 ? 3
309° 12' 11*2
W
22
13
8‘5
211
26
29-2
H”
2-7
1 27 9-0
209 59 22-8
6-2 .
Ambrozny <>-
L
339
11
29-0
Mittel =
=309° 12' 8”70
Aa" =+ 0-023 Aa”—1-164 A8’
1891. Mai 29. a.
in.
a
= 1*
18 m 7*5;
8 =
= + 88 c
43'
24 "5;
X — — l m 10*4;
Ambrozny -<>-
L
69°
11'
53'-7
Polaris
W
22 ]1
19 m
24 ? 5
301
24
39-5
+
0 V 6
1° 24' 54 v 3
299° 59’ 45 7
309° 12' 8-0
O
22
21
370
121
23
45-7
3-1
1 24 5-9
119 59 42-9
11-0
Ambrozny <>-
R
249
11
53-9
Mittel =
=309° 12' 9 V 50
A a" = +0-024 Aa" — M24 A8"
1891. Mai 29. a. m.
Ambrozny •<>
Polaris
a = l h 18 m 7*5; 8 = + 88° 43’ 24*5; * = — l“ 10 ? 3;
Ambrozny ■$
R
0
22 11 28“ 59 ? 0
204° 11’ 40*4
76 20 50-3
+ 1*0
1° 21' 20*7
74° 59' 30*6
309° 12' 9*8
W
22 31 5-5
256 20 20
+ 4-1
1 20 32-5
254 59 33-6
6-6
I,
24 11 40-2
Mittel = 309° 12' 8*20
A a" = + 0 • 025 A a" — 1-075A8"
1891. Mai 29. a. m.
a — l h 18 m 7 ? 6 ; 8 = 4-88° 43' 24*5; a; = — l“ 10 ? 3;
Ambrozny -<>-
L
22 l1 37“ 41 ? 0
114° 12' 9*3
Polaris
W
346 17 59-0
+ 2*7
1° 17' 58*8
T)
Ambrozny -¡y
0
R
22 39 50-5
166 17 1-9
294 12 10-8
+ 4-8
1 17 7-6
344° 0’ 2-8 309° 12' 6*5
164 59 59-1 11-7
Mittel = 309° Í2 7 9" 10
Aa" =4-0-026 Aa” — 1-033 A3'
