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- 10 REM OBSCURED FRACTION
- 12 REM AT A SOLAR ECLIPSE
- 14 REM
- 16 P=3.14159265
- 18 INPUT "SUN'S SEMIDIAMETER ";S1
- 20 INPUT "MOON'S SEMIDIAMETER";S2
- 22 S=S2/S1
- 24 INPUT "ECLIPSE MAGNITUDE ";M
- 26 IF M>(S+1)/2 OR M<0 THEN 24
- 28 REM
- 30 W=M*2
- 32 D=1+S-W
- 34 IF M<1 AND D<>0 THEN 46
- 36 IF S>=1 THEN F=1: REM TOTAL
- 38 IF S<1 THEN F=S*S: REM ANNULAR
- 40 F=F*P
- 42 GOTO 90
- 44 REM
- 46 REM ANGLE B
- 48 B1=(D*D+1-S*S)/(2*D)
- 50 IF B1>1 THEN B1=1
- 52 IF B1<-1 THEN B1=-1
- 54 IF B1<>0 THEN 58
- 56 B=P/2: GOTO 64
- 58 B=ATN(SQR(1-B1*B1)/B1)
- 60 IF B1<0 THEN B=B+P
- 62 REM
- 64 REM ANGLE C
- 66 C1=(S*S+1-D*D)/(2*S)
- 68 IF C1>1 THEN C1=1
- 70 IF C1<-1 THEN C1=-1
- 72 IF C1<>0 THEN 76
- 74 C=P/2: GOTO 82
- 76 C=ATN(SQR(1-C1*C1)/C1)
- 78 IF C1<0 THEN C=C+P
- 80 REM
- 82 REM ANGLE A
- 84 A=P-B-C
- 86 REM
- 88 F=S*S*A+B-S*SIN(C)
- 90 PRINT "OBSCURATION: ";F/P
- 92 END
- 100 REM ***********************
- 110 REM FROM SKY & TELESCOPE'S
- 120 REM ASTRONOMICAL COMPUTING
- 130 REM DEPARTMENT, NOVEMBER,
- 140 REM 1986, PAGES 515-516.
- 150 REM ***********************
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