Nr = |
8 |
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Elipsoida Krassowskiego |
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a= |
6378245,0 |
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e2= |
0,006693421623 |
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Bo= |
45 |
o |
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B1= |
54 |
o |
33 |
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0,9994 |
" |
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L1= |
20 |
o |
33 |
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52,1008 |
" |
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H1= |
145,243 |
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N= |
6392457,955 |
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X= |
3471375,599 |
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|
172810360,578535 |
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Y= |
1302348,262 |
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Z= |
5172717,267 |
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L= |
0 |
o |
-26 |
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-7,8992 |
" |
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20,56447 |
-26,13165 |
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3707635,30304296 |
= |
pierw(X2+Y2) |
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3707635,30304296 |
= |
(N+H)cosB |
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5207572,95696728 |
= |
Z+Ne2sinB |
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5207572,95696728 |
= |
(N+H)sinB |
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Bo= |
45 |
o |
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N0= |
6388944,93544501 |
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B2= |
54 |
o |
31 |
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34,54517 |
" |
= |
arctg(Z+Ne2sinBo/pierw(X2+Y2)) |
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54,52626 |
31,57575 |
34,54517 |
N2= |
6392449,442 |
= |
a/(pierw(1-e2sin2B2) |
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B3= |
54 |
o |
33 |
|
0,80469 |
" |
= |
arctg(Z+Ne2sinB2/pierw(X2+Y2)) |
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54,55022 |
33,01341 |
0,80469 |
N3= |
6392457,935 |
= |
a/(pierw(1-e2sin2B3) |
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dB= |
0 |
o |
1 |
|
26,25952 |
" |
= |
B2-B1 |
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0,02396 |
1,43766 |
26,25952 |
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B4= |
54 |
o |
33 |
|
0,99896 |
" |
= |
arctg(Z+Ne2sinB3/pierw(X2+Y2)) |
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54,55028 |
33,01665 |
0,99896 |
N4= |
6392457,955 |
= |
a/(pierw(1-e2sin2B4) |
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dB= |
0 |
o |
0 |
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0,19427 |
" |
= |
B4-B3 |
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0,00005 |
0,00324 |
0,19427 |
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B5= |
54 |
o |
33 |
|
0,99940 |
" |
= |
arctg(Z+Ne2sinB4/pierw(X2+Y2)) |
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|
54,55028 |
33,01666 |
0,99940 |
N5= |
6392457,955 |
= |
a/(pierw(1-e2sin2B5) |
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dB= |
0 |
o |
0 |
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0,00044 |
" |
= |
B5-B4 |
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0,00000 |
0,00001 |
0,00044 |
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B6= |
54 |
o |
33 |
|
0,99940 |
" |
= |
arctg(Z+Ne2sinB5/pierw(X2+Y2)) |
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|
54,55028 |
33,01666 |
0,99940 |
N6= |
6392457,955 |
= |
a/(pierw(1-e2sin2B6) |
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dB= |
0 |
o |
0 |
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0,00000 |
" |
= |
B6-B5 |
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H= |
-407034,344427781 |
= |
(X/(cosB6*cosL))-N6 |
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Nr |
8 |
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|
WGS 84 |
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a= |
6378137,0 |
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e2= |
0,006694379901 |
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Bo= |
50 |
o |
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B1= |
54 |
o |
33 |
|
1,0994 |
" |
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L1= |
20 |
o |
33 |
|
52,1008 |
" |
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H1= |
145,243 |
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N= |
6392351,765 |
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X= |
3471315,571 |
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Y= |
1302325,741 |
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Z= |
5172628,137 |
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L= |
0 |
o |
-26 |
|
-7,8992 |
" |
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|
20,56447 |
-26,13165 |
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|
3707571,190 |
= |
pierw(X2+Y2) |
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|
3707571,190 |
= |
(N+H)cosB |
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|
5207488,25008416 |
= |
Z+Ne2sinB |
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|
5207488,25008416 |
= |
(N+H)sinB |
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Bo= |
50 |
o |
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N0= |
6390702,04402744 |
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B2= |
54 |
o |
32 |
|
22,02549 |
" |
= |
arctg(Z+Ne2sinBo/pierw(X2+Y2)) |
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|
54,53945 |
32,36709 |
22,02549 |
N2= |
6392347,918 |
= |
a/(pierw(1-e2sin2B2) |
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B3= |
54 |
o |
33 |
|
1,01140 |
" |
= |
arctg(Z+Ne2sinB2/pierw(X2+Y2)) |
|
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|
54,55028 |
33,01686 |
1,01140 |
N3= |
6392351,757 |
= |
a/(pierw(1-e2sin2B3) |
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dB= |
0 |
o |
0 |
|
38,98591 |
" |
= |
B2-B1 |
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|
0,01083 |
0,64977 |
38,98591 |
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B4= |
54 |
o |
33 |
|
1,09920 |
" |
= |
arctg(Z+Ne2sinB3/pierw(X2+Y2)) |
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|
54,55031 |
33,01832 |
1,09920 |
N4= |
6392351,765 |
= |
a/(pierw(1-e2sin2B4) |
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dB= |
0 |
o |
0 |
|
0,08780 |
" |
= |
B4-B3 |
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|
0,00002 |
0,00146 |
0,08780 |
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B5= |
54 |
o |
33 |
|
1,09940 |
" |
= |
arctg(Z+Ne2sinB4/pierw(X2+Y2)) |
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|
54,55031 |
33,01832 |
1,09940 |
N5= |
6392351,765 |
= |
a/(pierw(1-e2sin2B5) |
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dB= |
0 |
o |
0 |
|
0,00020 |
" |
= |
B5-B4 |
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|
0,00000 |
0,00000 |
0,00020 |
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B6= |
54 |
o |
33 |
|
1,09940 |
" |
= |
arctg(Z+Ne2sinB5/pierw(X2+Y2)) |
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|
54,55031 |
33,01832 |
1,09940 |
N6= |
6392351,765 |
= |
a/(pierw(1-e2sin2B6) |
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dB= |
0 |
o |
0 |
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0,00000 |
" |
= |
B6-B5 |
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H= |
-407027,580660489 |
= |
(X/(cosB6*cosL))-N6 |
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Nr = |
8 |
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Interpolacja liniowa na podstawie tabel. |
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|
Opis |
z zadania |
po uwzglednieniu n |
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1. |
(3)1 dla szerokości |
|
53,33017581 |
|
B1 |
53,33017573 |
Piotr:
wartości kątowe "w stopniach" zapisane w postaci np.:
53,33017573
należy zapisać
53o33'01,7573"
53,33017581 |
0,934632337952291 |
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|
dla 33' |
0,0000000025301 |
|
L1 |
21,33523634 |
21,33523626 |
0,376372314853363 |
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dla 34' |
0,0000000025301 |
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Wynik= |
0,0000000025301 |
|
A1-2 |
9,073501 |
9,073581 |
0,159289461919355 |
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2. |
(1)1 dla szerokości |
|
53,33017581 |
|
S1-2 |
22856,807 |
22857,607 |
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dla 33' |
0,032345454 |
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dla 34' |
0,032345363 |
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Wynik= |
0,032345451 |
Err:502 |
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3. |
(1)s dla szerokości |
|
Err:502 |
|
R |
6371000 |
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dla 39' |
0,032344910 |
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dla 40' |
0,032344819 |
|
Zadanie wprost - matoda Clarke'a |
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Wynik= |
Err:502 |
Err:502 |
szerokosc punktu 2 |
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4. |
(3)c dla szerokości |
|
Err:502 |
|
s12 do kw |
522470197,766449 |
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dla 45' |
0,0000000025300 |
|
CosAZ |
0,987340235810914 |
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dla 46' |
0,0000000025300 |
|
sinAZ |
0,158616703877139 |
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Wynik= |
Err:502 |
Err:502 |
E= |
0,207 |
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|
5. |
(2)c dla szerokości |
|
Err:502 |
|
E= |
MACIEJ WELNICKI:
w stopniach
0,00002070 |
MACIEJ WELNICKI:
w radianach
0,0000010036674 |
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dla 45' |
0,03226834 |
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dla 46' |
0,03226831 |
|
AZ-2/3E |
0,159288792807732 |
9,073567 |
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Wynik= |
Err:502 |
Err:502 |
AZ-1/3E |
0,159289127363544 |
9,073574 |
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cosAZ-2/3E |
0,987340342 |
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|
1. |
(1)B dla szerokości |
|
Err:502 |
|
sinAZ-1/3E |
0,158616374 |
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dla 39' |
0,0323449099 |
|
u= |
22568,238 |
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|
dla 40' |
0,0323448193 |
|
v= |
3625,591 |
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Wynik= |
Err:502 |
Err:502 |
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|
2. |
(2)B dla szerokości |
|
53,39066624 |
|
DBOc |
MACIEJ WELNICKI:
w sekundach
Err:502 |
Err:502 |
Err:502 |
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|
|
dla 39' |
0,0322685197 |
|
DBOc |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w radianach
Err:502 |
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|
dla 40' |
0,0322684896 |
|
Bs |
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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|
Wynik= |
0,0322685164 |
0,0322685160 |
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3. |
(3)B dla szerokości |
|
53,39066624 |
|
DBc |
MACIEJ WELNICKI:
w sekundach
Err:502 |
Err:502 |
Err:502 |
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|
dla 39' |
0,3143 |
|
DBc |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w radianach
Err:502 |
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dla 40' |
0,3146 |
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Wynik= |
0,31433331 |
0,3143000000 |
Bc |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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4. |
(4)B dla szerokości |
|
53,39066624 |
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dla 39' |
0,0002 |
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dla 40' |
0,0002 |
|
w |
MACIEJ WELNICKI:
w sekundach
Err:502 |
MACIEJ WELNICKI:
w sekundach
Err:502 |
MACIEJ WELNICKI:
w radianach
Err:502 |
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Wynik= |
0,0002 |
0,0002000000 |
B2= |
MACIEJ WELNICKI:
w radianach
Err:502 |
Err:502 |
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5. |
(5)B dla szerokości |
|
53,39066624 |
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dla 39' |
0,0399 |
|
dlugosc punktu 2 |
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dla 40' |
0,0399 |
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Wynik= |
0,0399 |
0,0399 |
DL |
MACIEJ WELNICKI:
w sekundach
Err:502 |
Err:502 |
Err:502 |
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6. |
(6)B dla szerokości |
|
53,39066624 |
|
DL |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w radianach
Err:502 |
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dla 39' |
0,0835 |
|
B2 + 1/3w |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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dla 40' |
0,0835 |
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Wynik= |
0,0835 |
0,0835 |
L2 |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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7. |
(7)B dla szerokości |
|
53,39066624 |
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dla 39' |
0,1252 |
|
azymut 2-1 |
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dla 40' |
0,1252 |
|
g |
MACIEJ WELNICKI:
w sekundach
Err:502 |
Err:502 |
Err:502 |
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Wynik= |
0,1252 |
0,1252 |
g |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w radianach
Err:502 |
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B2 + 2/3w |
MACIEJ WELNICKI:
w radianach
Err:502 |
Err:502 |
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AZ2-1 |
Err:502 |
Err:502 |
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Zadanie odwrotne - metoda średniej szerokości Gaussa |
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w stopniach |
w radianach |
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B1 |
53,33017581 |
0,934632337952291 |
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L1 |
21,33523626 |
0,376372314853363 |
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B2 |
Err:502 |
Err:502 |
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L2 |
Err:502 |
Err:502 |
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DB |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w sekundach
Err:502 |
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DL |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w sekundach
Err:502 |
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B |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
MACIEJ WELNICKI:
w sekundach
Err:502 |
Err:502 |
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C |
Err:502 |
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|
Err:502 |
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S |
Err:502 |
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D |
Err:502 |
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u= |
Err:502 |
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v= |
Err:502 |
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DA |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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s1-2 |
Err:502 |
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A |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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A1-2 |
MACIEJ WELNICKI:
w radianach
Err:502 |
Err:502 |
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|
a2-1 |
MACIEJ WELNICKI:
w radianach
Err:502 |
MACIEJ WELNICKI:
w stopniach
Err:502 |
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Nr = |
8 |
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1. Przeliczanie współrzędnych horyzontalnych na równikowe i odwrotnie |
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A) dane |
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na radiany |
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fi - |
53,1543 |
Piotr:
wartości kątowe "w stopniach" zapisane w postaci np.:
53,1543
należy zapisać
53o15'43"
53,1543 |
0,929596296569858 |
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|
ax- |
171,3743 |
1370,9944 |
23,9400220029999 |
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|
zx- |
68,2416 |
545,9328 |
9,53923277460572 |
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B) dane |
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fi- |
63,1543 |
63,1543 |
1,10412922176929 |
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ax- |
269,1743 |
2153,3944 |
37,5884967535956 |
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zx- |
121,1817 |
969,4536 |
16,9255049541402 |
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A) |
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sin delta= |
***:
SIN DELTA=
-0,770919 |
-0,880282 |
Piotr:
w stopniach
-50,2611 |
=delta (w stopniach) |
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tg t = |
***:
w RADIANACH
-0,169004 |
-0,167422 |
Piotr:
w stopniach
-9,3533 |
w stopniach |
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|
stopnie |
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|
t w stopniach= |
|
|
2,974170 |
Piotr:
w stopniach
170,2427 |
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|
godziny |
minuty |
sekundy |
|
|
t w godzinach= |
|
|
11 |
21 |
38 |
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A arctg= |
-1,192719 |
-2,5177199024536 |
-68,2016 |
|
|
-2,5177199024536 |
0,106139484629534 |
a= |
1,94887342787136 |
***:
W STOPNIACH
111,3944 |
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|
-0,042156986774461 |
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cosZ= |
-0,993457 |
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z= |
3,027138 |
***:
W STOPNIACH
173,2632 |
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B) |
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sin delta= |
***:
w radianach
0,110590 |
0,1108 |
delta= |
***:
W STOPNIACH
6,2057 |
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tg t = |
-0,104783 |
-0,1044 |
***:
W STOPNIACH
-5,5854 |
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t w stopniach |
|
|
***:
w radianach
6,1787832454808 |
***:
w stopniach
354,0106 |
|
3,03719059189101 |
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godziny |
minuty |
sekundy |
|
|
t w godzinach |
|
|
23 |
36 |
4 |
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|
-0,103573281988489 |
A arctg= |
-0,123702 |
-0,124336737889465 |
-7,0515 |
|
|
-0,124336737889465 |
0,833006267870442 |
a= |
3,01789077034319 |
***:
w stopniach
172,5445 |
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cosZ= |
0,543482 |
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z= |
0,99621617100992 |
57,0444 |
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Nr = |
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8 |
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wartości, które należy odczytać |
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z tablic i samemu, ręcznie |
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A) |
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wpisać do programu |
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lPoznań= |
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1 |
h |
7 |
m |
30,99 |
s |
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x= |
|
0,0027379103 |
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data |
|
Piotr:
Jeśli ilość dni przekracz 31 to wtedy przechodzimy na następny miesiąć np.:
35.VII. = 4.VIII.
18 |
. |
VII |
. |
1998r |
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dodz |
|
Piotr:
Jeśli godz jest większa od 24h to te 24h zostały od całości odjęte np.:
30h - 24h = 6h
18 |
h |
48 |
m |
38,1244 |
s |
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TSE |
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18 |
h |
48 |
m |
38,1244 |
s |
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18 |
VII |
1998r |
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Wartości DYcose, dYcose należy samemu |
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- |
1 |
h |
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odczytać z tablic i wpisać ręcznie |
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TU |
|
17 |
h |
48 |
m |
38,1244 |
s |
|
TU = TSE - 1h |
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do programu |
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R1 |
+ |
0 |
h |
2 |
m |
55,5497 |
s |
|
R1 = x * TU |
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(TU)GW |
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17 |
h |
51 |
m |
33,6741 |
s |
|
(TU)GW = TU + R1 |
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DYcose |
dYcose |
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D |
+ |
19 |
h |
42 |
m |
24,8150 |
s |
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19 |
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17 |
-0,4248 |
-0,0097 |
u-1= |
-0,4345 |
D0= |
-0,0011 |
D3= |
0,0028 |
OGr |
|
13 |
h |
33 |
m |
58,4891 |
s |
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19 |
VII |
1998r |
18 |
-0,4241 |
-0,0115 |
u0= |
-0,4356 |
D1= |
0,0017 |
D4= |
0,0026 |
lPoznań |
+ |
1 |
h |
7 |
m |
30,9900 |
s |
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19 |
-0,4235 |
-0,0104 |
u1= |
-0,4339 |
D2= |
0,0043 |
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OT |
|
14 |
h |
41 |
m |
29,4791 |
s |
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20 |
-0,4229 |
-0,0067 |
u2= |
-0,4296 |
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u (nutacja) |
+ |
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|
-0,4346 |
s |
|
u = u0 + nD1 + ((n(n - 1)) / 4)(D3 * D4) |
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OTpr |
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14 |
h |
41 |
m |
29,0445 |
s |
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n= |
|
0,742108 |
|
n=TU"/86400" |
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Czas środkowoeuropejski |
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18 |
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VII |
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1998r |
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18 |
h |
48 |
m |
38,1244 |
s |
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w średnim i prawdziwym czasie gwiazdowym południka Poznań wyraża się |
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19 |
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VII |
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1998r |
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14 |
h |
41 |
m |
29,4790732114203 |
s |
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19 |
|
VII |
|
1998r |
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14 |
h |
41 |
m |
29,0444764268189 |
s |
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B) |
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lPoznań= |
|
1 |
h |
7 |
m |
30,99 |
s |
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y= |
|
0,0027304346 |
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data |
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Piotr:
Jeśli ilość dni przekracz 31 to wtedy przechodzimy na następny miesiąć np.:
35.VII. = 4.VIII.
23 |
. |
VII |
. |
1998r |
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dodz |
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Piotr:
Jeśli godz jest większa od 24h to te 24h zostały od całości odjęte np.:
30h - 24h = 6h
18 |
h |
48 |
m |
38,1244 |
s |
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Przybliżone |
Prawdziwe |
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Wartości DYcose, dYcose należy samemu |
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OTpr |
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18 |
h |
48 |
m |
38,1244 |
s |
18 |
h |
48 |
m |
38,1244 |
s |
23 |
VII |
1998r |
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odczytać z tablic i wpisać ręcznie |
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u (nutacja) |
- |
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-0,4082 |
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do programu |
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OT |
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18 |
h |
48 |
m |
38,5326 |
s |
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lPoznań |
- |
1 |
h |
7 |
m |
30,9900 |
s |
1 |
h |
7 |
m |
30,9900 |
s |
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DYcose |
dYcose |
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OGr |
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17 |
h |
41 |
m |
7,1344 |
s |
17 |
h |
41 |
m |
7,5426 |
s |
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22 |
-0,4220 |
0,0050 |
u-1= |
-0,4170 |
D0= |
0,0055 |
D3= |
-0,0019 |
D |
- |
20 |
h |
2 |
m |
7,5919 |
s |
20 |
h |
2 |
m |
7,5919 |
s |
22 |
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23 |
-0,4217 |
0,0102 |
u0= |
-0,4115 |
D1= |
0,0036 |
D4= |
-0,0025 |
(TU)GW |
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21 |
h |
38 |
m |
59,5425 |
s |
21 |
h |
38 |
m |
59,9507 |
s |
22 |
VIII |
1998r |
24 |
-0,4214 |
0,0135 |
u1= |
-0,4079 |
D2= |
0,0011 |
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R2 |
- |
0 |
h |
3 |
m |
32,8088 |
s |
0 |
h |
3 |
m |
32,8099 |
s |
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25 |
-0,4212 |
0,0144 |
u2= |
-0,4068 |
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TU |
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21 |
h |
35 |
m |
26,7337 |
s |
21 |
h |
35 |
m |
27,1407 |
s |
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+ |
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2 |
h |
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TSE |
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23 |
h |
35 |
m |
27,1407 |
s |
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R2Prz = |
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0 |
h |
3 |
m |
32,8088 |
s |
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R2Prz = y * TUGwPrz |
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n = |
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0,899615 |
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n=TU"/86400" |
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R2Pr = |
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0 |
h |
3 |
m |
32,8099 |
s |
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R2Pr = y * TUGwPr |
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Prawdziwy czas gwiazdowy południka Poznań |
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23 |
|
VII |
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1998r |
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18 |
h |
48 |
m |
38,1244 |
s |
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w czasie wschodnioeuropejskim wyraża się |
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22 |
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VIII |
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1998r |
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23 |
h |
35 |
m |
27,1407240375012 |
s |
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