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- 10 ' Sunrise-Sunset
- 20 GOSUB 300
- 30 INPUT "Lat, Long (deg)";B5,L5
- 40 INPUT "Time zone (hrs)";H
- 50 L5=L5/360: Z0=H/24
- 60 GOSUB 1170: T=(J-2451545)+F
- 70 TT=T/36525+1: ' TT = centuries
- 80 ' from 1900.0
- 90 GOSUB 410: T=T+Z0
- 100 '
- 110 ' Get Sun's Position
- 120 GOSUB 910: A(1)=A5: D(1)=D5
- 130 T=T+1
- 140 GOSUB 910: A(2)=A5: D(2)=D5
- 150 IF A(2)<A(1) THEN A(2)=A(2)+P2
- 160 Z1=DR*90.833: ' Zenith dist.
- 170 S=SIN(B5*DR): C=COS(B5*DR)
- 180 Z=COS(Z1): M8=0: W8=0: PRINT
- 190 A0=A(1): D0=D(1)
- 200 DA=A(2)-A(1): DD=D(2)-D(1)
- 210 FOR C0=0 TO 23
- 220 P=(C0+1)/24
- 230 A2=A(1)+P*DA: D2=D(1)+P*DD
- 240 GOSUB 490
- 250 A0=A2: D0=D2: V0=V2
- 260 NEXT
- 270 GOSUB 820: ' Special msg?
- 280 END
- 290 '
- 300 ' Constants
- 310 DIM A(2),D(2)
- 320 P1=3.14159265: P2=2*P1
- 330 DR=P1/180: K1=15*DR*1.0027379
- 340 S$="Sunset at "
- 350 R$="Sunrise at "
- 360 M1$="No sunrise this date"
- 370 M2$="No sunset this date"
- 380 M3$="Sun down all day"
- 390 M4$="Sun up all day"
- 400 RETURN
- 410 ' LST at 0h zone time
- 420 T0=T/36525
- 430 S=24110.5+8640184.813*T0
- 440 S=S+86636.6*Z0+86400*L5
- 450 S=S/86400: S=S-INT(S)
- 460 T0=S*360*DR
- 470 RETURN
- 480 '
- 490 ' Test an hour for an event
- 500 L0=T0+C0*K1: L2=L0+K1
- 510 H0=L0-A0: H2=L2-A2
- 520 H1=(H2+H0)/2: ' Hour angle,
- 530 D1=(D2+D0)/2: ' declination,
- 540 ' at half hour
- 550 IF C0>0 THEN 570
- 560 V0=S*SIN(D0)+C*COS(D0)*COS(H0)-Z
- 570 V2=S*SIN(D2)+C*COS(D2)*COS(H2)-Z
- 580 IF SGN(V0)=SGN(V2) THEN 800
- 590 V1=S*SIN(D1)+C*COS(D1)*COS(H1)-Z
- 600 A=2*V2-4*V1+2*V0: B=4*V1-3*V0-V2
- 610 D=B*B-4*A*V0: IF D<0 THEN 800
- 620 D=SQR(D)
- 630 IF V0<0 AND V2>0 THEN PRINT R$;
- 640 IF V0<0 AND V2>0 THEN M8=1
- 650 IF V0>0 AND V2<0 THEN PRINT S$;
- 660 IF V0>0 AND V2<0 THEN W8=1
- 670 E=(-B+D)/(2*A)
- 680 IF E>1 OR E<0 THEN E=(-B-D)/(2*A)
- 690 T3=C0+E+1/120: ' Round off
- 700 H3=INT(T3): M3=INT((T3-H3)*60)
- 710 PRINT USING "##:##";H3;M3;
- 720 H7=H0+E*(H2-H0)
- 730 N7=-COS(D1)*SIN(H7)
- 740 D7=C*SIN(D1)-S*COS(D1)*COS(H7)
- 750 AZ=ATN(N7/D7)/DR
- 760 IF D7<0 THEN AZ=AZ+180
- 770 IF AZ<0 THEN AZ=AZ+360
- 780 IF AZ>360 THEN AZ=AZ-360
- 790 PRINT USING ", azimuth ###.#";AZ
- 800 RETURN
- 810 '
- 820 ' Special-message routine
- 830 IF M8=0 AND W8=0 THEN 870
- 840 IF M8=0 THEN PRINT M1$
- 850 IF W8=0 THEN PRINT M2$
- 860 GOTO 890
- 870 IF V2<0 THEN PRINT M3$
- 880 IF V2>0 THEN PRINT M4$
- 890 RETURN
- 900 '
- 910 ' Fundamental arguments
- 920 ' (Van Flandern &
- 930 ' Pulkkinen, 1979)
- 940 L=.779072+.00273790931*T
- 950 G=.993126+.0027377785*T
- 960 L=L-INT(L): G=G-INT(G)
- 970 L=L*P2: G=G*P2
- 980 V=.39785*SIN(L)
- 990 V=V-.01000*SIN(L-G)
- 1000 V=V+.00333*SIN(L+G)
- 1010 V=V-.00021*TT*SIN(L)
- 1020 U=1-.03349*COS(G)
- 1030 U=U-.00014*COS(2*L)
- 1040 U=U+.00008*COS(L)
- 1050 W=-.00010-.04129*SIN(2*L)
- 1060 W=W+.03211*SIN(G)
- 1070 W=W+.00104*SIN(2*L-G)
- 1080 W=W-.00035*SIN(2*L+G)
- 1090 W=W-.00008*TT*SIN(G)
- 1100 '
- 1110 ' Compute Sun's RA and Dec
- 1120 S=W/SQR(U-V*V)
- 1130 A5=L+ATN(S/SQR(1-S*S))
- 1140 S=V/SQR(U):D5=ATN(S/SQR(1-S*S))
- 1150 R5=1.00021*SQR(U)
- 1160 RETURN
- 1165 '
- 1170 ' Calendar --> JD
- 1180 INPUT "Year, Month, Day";Y,M,D
- 1190 G=1: IF Y<1583 THEN G=0
- 1200 D1=INT(D): F=D-D1-.5
- 1210 J=-INT(7*(INT((M+9)/12)+Y)/4)
- 1220 IF G=0 THEN 1260
- 1230 S=SGN(M-9): A=ABS(M-9)
- 1240 J3=INT(Y+S*INT(A/7))
- 1250 J3=-INT((INT(J3/100)+1)*3/4)
- 1260 J=J+INT(275*M/9)+D1+G*J3
- 1270 J=J+1721027+2*G+367*Y
- 1280 IF F>=0 THEN 1300
- 1290 F=F+1: J=J-1
- 1300 RETURN
- 1310 '
- 1320 ' This program by Roger W. Sinnott calculates the times of sunrise
- 1330 ' and sunset on any date, accurate to the minute within several
- 1340 ' centuries of the present. It correctly describes what happens in the
- 1350 ' arctic and antarctic regions, where the Sun may not rise or set on
- 1360 ' a given date. Enter north latitudes positive, west longitudes
- 1370 ' negative. For the time zone, enter the number of hours west of
- 1380 ' Greenwich (e.g., 5 for EST, 4 for EDT). The calculation is
- 1390 ' discussed in Sky & Telescope for August 1994, page 84.
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