10 REM VISLIMIT.BAS Visual Limits 20 REM by Bradley E. Schaefer 30 FOR I=1 TO 5 : READ WA(I) : NEXT I 40 DATA 0.365, 0.44, 0.55, 0.7, 0.9 50 FOR I=1 TO 5 : READ MO(I) : NEXT I 60 DATA -10.93, -10.45, -11.05, -11.90, -12.70 70 RD=3.14159/180.0 80 REM Input for Moon and Sun 90 AM=180.0 : REM Moon phase (deg.; 0=FM, 90=FQ/LQ, 180=NM) 100 ZM=180.0 : REM Zenith distance of Moon (deg.) 110 RM=180.0 : REM Angular distance to Moon (deg.) 120 ZS=180.0 : REM Zenith distance of Sun (deg.) 130 RS=180.0 : REM Angular distance to Sun (deg.) 140 REM Input for the Site, Date, Observer 150 RH=40.0 : REM relative humidity (%) 160 TE=15.0 : REM Air temperature (deg. C) 170 LA=30.0 : REM Latitude (deg.) 180 AL=1000.0 : REM Altitude above sea level (m) 190 M=2.0 : REM Month (1=Jan, 12=Dec) 200 Y=1998.0 : REM Year 210 SN=1.0 : REM Snellen Ratio (20/20=1.0, good 20/10=2.0) 220 INPUT "Zenith distance (deg.): ";Z 230 GOSUB 1000 : REM Extinction 240 GOSUB 2000 : REM Sky 250 REM Visual limiting magnitude 260 BL=B(3)/1.11E-15 : REM in nanolamberts 270 IF BL>1500.0 THEN GOTO 300 280 C1=10.0^-9.8: C2=10.0^-1.9 290 GOTO 310 300 C1=10.0^-8.350001 : C2=10.0^-5.9 310 TH=C1*((1.0+SQR(C2*BL))^2.0) : REM in foot-candles 320 MN=-16.57-2.5*(LOG(TH)/LOG(10))-DM(3)+5.0*(LOG(SN)/LOG(10)) 330 PRINT : REM Write results and stop program 340 PRINT USING "Visual Sky Brightness (nL): ######"; BL 350 PRINT USING "Visual Limiting Magnitude: ###.##"; MN 360 END 1000 REM Extinction Subroutine 1010 FOR I=1 TO 5: READ OZ(I): NEXT I 1020 DATA 0.000, 0.000, 0.031, 0.008, 0.000 1030 FOR I=1 TO 5: READ WT(I): NEXT I 1040 DATA 0.074, 0.045, 0.031, 0.020, 0.015 1050 LT=LA*RD 1060 RA=(M-3)*30.0*RD 1070 SL=LA/ABS(LA) 1080 REM Airmass for each component 1090 ZZ=Z*RD 1100 XG=1/(COS(ZZ)+.0286*EXP(-10.5*COS(ZZ))) 1110 XA=1/(COS(ZZ)+.0123*EXP(-24.5*COS(ZZ))) 1120 XO=1/SQR(1.0-(SIN(ZZ)/(1.0+(20.0/6378.0)))^2) 1130 REM UBVRI extinction for each component 1140 FOR I=1 TO 5 1150 KR=.1066*EXP(-1*AL/8200)*((WA(I)/.55)^-4) 1160 KA=.1*((WA(I)/.55)^-1.3)*EXP(-1*AL/1500) 1170 KA=KA*((1-.32/LOG(RH/100.0))^1.33)*(1+0.33*SL*SIN(RA)) 1180 KO=OZ(I)*(3.0+.4*(LT*COS(RA)-COS(3*LT)))/3.0 1190 KW=WT(I)*.94*(RH/100.0)*EXP(TE/15)*EXP(-1*AL/8200) 1200 K(I)=KR+KA+KO+KW 1210 DM(I)=KR*XG+KA*XA+KO*XO+KW*XG 1220 NEXT I 1230 REM Write results and return 1240 PRINT : PRINT "Airmass (gas, aerosol, ozone): "; 1250 PRINT USING "####.## "; XG, XA, XO 1260 PRINT "Extinction Coefficients (UBVRI): "; 1270 PRINT USING "####.## "; K(1), K(2), K(3), K(4), K(5) 1280 PRINT "Total Extinction (UBVRI): "; 1290 PRINT USING "####.## "; DM(1), DM(2), DM(3), DM(4), DM(5) 1300 RETURN 2000 REM SKY Subroutine 2010 FOR I=1 TO 5: READ BO(I): NEXT I 2020 DATA 8.0E-14, 7.0E-14, 1.0E-13, 1.0E-13, 3.0E-13 2030 FOR I=1 TO 5: READ CM(I): NEXT I 2040 DATA 1.36, 0.91, 0.00, -0.76, -1.17 2050 FOR I=1 TO 5: READ MS(I): NEXT I 2060 DATA -25.96, -26.09, -26.74, -27.26, -27.55 2070 X=1/(COS(ZZ)+.025*EXP(-11*COS(ZZ))) : REM air mass 2080 XM=1/(COS(ZM*RD)+.025*EXP(-11*COS(ZM*RD))) : REM air mass Moon 2090 IF ZM>90.0 THEN XM=40.0 2100 XS=1/(COS(ZS*RD)+.025*EXP(-11*COS(ZS*RD))) : REM air mass Sun 2110 IF ZS>90.0 THEN XS=40.0 2120 FOR I=1 TO 5 2130 REM Dark night sky brightness 2140 BN=BO(I)*(1+.3*COS(6.283*(Y-1992)/11)) 2150 BN=BN*(.4+.6/SQR(1.0-.96*((SIN(ZZ))^2))) 2160 BN=BN*(10^(-.4*K(I)*X)) 2170 REM Moonlight brightness 2180 MM=-12.73+.026*ABS(AM)+4E-09*(AM^4) : REM moon mag in V 2190 MM=MM+CM(I) : REM Moon mag 2200 C3=10.0^(-.4*K(I)*XM) 2210 FM=6.2E+07*(RM^-2)+(10^(6.15-RM/40)) 2220 FM=FM+(10^5.36)*(1.06+((COS(RM*RD))^2)) 2230 BM=10^(-.4*(MM-MO(I)+43.27)) 2240 BM=BM*(1-10^(-.4*K(I)*X)) 2250 BM=BM*(FM*C3+440000.0*(1-C3)) 2260 REM Twilight brightness 2270 HS=90.0-ZS : REM Height of Sun 2280 BT=10^(-.4*(MS(I)-MO(I)+32.5-HS-(Z/(360*K(I))))) 2290 BT=BT*(100/RS)*(1.0-10.0^(-.4*K(I)*X)) 2300 REM Daylight brightness 2310 C4=10.0^(-.4*K(I)*XS) 2320 FS=6.2E+07*(RS^-2)+(10^(6.15-RS/40)) 2330 FS=FS+(10^5.36)*(1.06+((COS(RS*RD))^2)) 2340 BD=10^(-.4*(MS(I)-MO(I)+43.27)) 2350 BD=BD*(1-10^(-.4*K(I)*X)) 2360 BD=BD*(FS*C4+440000.0*(1-C4)) 2370 REM Total sky brightness 2380 IF BD>BT THEN GOTO 2410 2390 B(I)=BN+BD 2400 GOTO 2420 2410 B(I)=BN+BT 2420 IF ZM<90.0 THEN B(I)=B(I)+BM 2430 NEXT I 2440 PRINT "Sky brightness (UBVRI):"; 2450 PRINT USING " ##.#^^^^"; B(1), B(2), B(3), B(4), B(5) 2460 RETURN 9991 REM ============================== 9992 REM FROM "ASTRONOMICAL COMPUTING," 9993 REM SKY & TELESCOPE, MAY 1998 9994 REM ==============================