/[PAMELA software]/DarthVader/OrbitalInfo/src/igrf_sub.for
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Revision 1.10 - (hide annotations) (download)
Fri Aug 29 07:06:41 2014 UTC (10 years, 3 months ago) by mocchiut
Branch: MAIN
Changes since 1.9: +1 -1 lines
Small SL6 compilation bug fixed

1 mocchiut 1.8 c subroutine igrf_sub(xlat,xlong,year,height,
2     c & xl,icode,dip,dec)
3 mocchiut 1.1 c----------------------------------------------------------------
4     c INPUT:
5 mocchiut 1.4 c xlat geodatic latitude in degrees
6     c xlong geodatic longitude in degrees
7     c year decimal year (year+month/12.0-0.5 or year+day-of-year/365
8     c or 366 if leap year)
9     c height height in km
10 mocchiut 1.1 c OUTPUT:
11 mocchiut 1.4 c xl L value
12     c icode =1 L is correct; =2 L is not correct;
13     c =3 an approximation is used
14     c dip geomagnetic inclination in degrees
15     c dec geomagnetic declination in degress
16 mocchiut 1.1 c----------------------------------------------------------------
17 mocchiut 1.8 c
18     c REAL LATI,LONGI
19     c COMMON/GENER/ UMR,ERA,AQUAD,BQUAD
20     c SAVE /GENER/
21     C
22     c CALL INITIZE
23     c ibbb=0
24     c ALOG2=ALOG(2.)
25     c ISTART=1
26     c lati=xlat
27     c longi=xlong
28 mocchiut 1.1 c
29     C----------------CALCULATE PROFILES-----------------------------------
30     c
31 mocchiut 1.8 c CALL FELDCOF(YEAR,DIMO)
32     c CALL FELDG(LATI,LONGI,HEIGHT,BNORTH,BEAST,BDOWN,BABS)
33     c CALL SHELLG(LATI,LONGI,HEIGHT,DIMO,XL,ICODE,BAB1)
34     c DIP=ASIN(BDOWN/BABS)/UMR
35     c DEC=ASIN(BEAST/SQRT(BEAST*BEAST+BNORTH*BNORTH))/UMR
36     c RETURN
37     c END
38 mocchiut 1.1 c
39     c
40     C SHELLIG.FOR, Version 2.0, January 1992
41     C
42     C 11/01/91-DKB- SHELLG: lowest starting point for B0 search is 2
43     C 1/27/92-DKB- Adopted to IGRF-91 coeffcients model
44     C 2/05/92-DKB- Reduce variable-names: INTER(P)SHC,EXTRA(P)SHC,INITI(ALI)ZE
45     C 8/08/95-DKB- Updated to IGRF-45-95; new coeff. DGRF90, IGRF95, IGRF95S
46     C 5/31/00-DKB- Updated to IGRF-45-00; new coeff.: IGRF00, IGRF00s
47     C 3/24/05-DKB- Updated to IGRF-45-10; new coeff.: IGRF05, IGRF05s
48     C 4/25/05-DKB- CALL FELDI and DO 1111 I=1,7 [Alexey Petrov]
49     C
50     C*********************************************************************
51     C SUBROUTINES FINDB0, SHELLG, STOER, FELDG, FELDCOF, GETSHC, *
52     C INTERSHC, EXTRASHC, INITIZE *
53     C*********************************************************************
54     C*********************************************************************
55     C
56     C
57     SUBROUTINE FINDB0(STPS,BDEL,VALUE,BEQU,RR0)
58     C--------------------------------------------------------------------
59     C FINDS SMALLEST MAGNETIC FIELD STRENGTH ON FIELD LINE
60     C
61     C INPUT: STPS STEP SIZE FOR FIELD LINE TRACING
62     C COMMON/FIDB0/
63     C SP DIPOLE ORIENTED COORDINATES FORM SHELLG; P(1,*),
64     C P(2,*), P(3,*) CLOSEST TO MAGNETIC EQUATOR
65     C BDEL REQUIRED ACCURACY = [ B(LAST) - BEQU ] / BEQU
66     C B(LAST) IS FIELD STRENGTH BEFORE BEQU
67     C
68     C OUTPUT: VALUE =.FALSE., IF BEQU IS NOT MINIMAL VALUE ON FIELD LINE
69     C BEQU MAGNETIC FIELD STRENGTH AT MAGNETIC EQUATOR
70     C RR0 EQUATORIAL RADIUS NORMALIZED TO EARTH RADIUS
71     C BDEL FINAL ACHIEVED ACCURACY
72     C--------------------------------------------------------------------
73     DIMENSION P(8,4),SP(3)
74     LOGICAL VALUE
75     COMMON/FIDB0/ SP
76     SAVE /FIDB0/
77     C
78     STEP=STPS
79     IRUN=0
80     7777 IRUN=IRUN+1
81     IF(IRUN.GT.5) THEN
82     VALUE=.FALSE.
83     GOTO 8888
84     ENDIF
85     C*********************FIRST THREE POINTS
86     P(1,2)=SP(1)
87     P(2,2)=SP(2)
88     P(3,2)=SP(3)
89     STEP=-SIGN(STEP,P(3,2))
90     CALL STOER(P(1,2),BQ2,R2)
91     P(1,3)=P(1,2)+0.5*STEP*P(4,2)
92     P(2,3)=P(2,2)+0.5*STEP*P(5,2)
93     P(3,3)=P(3,2)+0.5*STEP
94     CALL STOER(P(1,3),BQ3,R3)
95     P(1,1)=P(1,2)-STEP*(2.*P(4,2)-P(4,3))
96     P(2,1)=P(2,2)-STEP*(2.*P(5,2)-P(5,3))
97     P(3,1)=P(3,2)-STEP
98     CALL STOER(P(1,1),BQ1,R1)
99     P(1,3)=P(1,2)+STEP*(20.*P(4,3)-3.*P(4,2)+P(4,1))/18.
100     P(2,3)=P(2,2)+STEP*(20.*P(5,3)-3.*P(5,2)+P(5,1))/18.
101     P(3,3)=P(3,2)+STEP
102     CALL STOER(P(1,3),BQ3,R3)
103     C******************INVERT SENSE IF REQUIRED
104     IF(BQ3.LE.BQ1) GOTO 2
105     STEP=-STEP
106     R3=R1
107     BQ3=BQ1
108     DO 1 I=1,5
109     ZZ=P(I,1)
110     P(I,1)=P(I,3)
111     1 P(I,3)=ZZ
112     C******************INITIALIZATION
113     2 STEP12=STEP/12.
114     VALUE=.TRUE.
115     BMIN=1.E4
116     BOLD=1.E4
117     C******************CORRECTOR (FIELD LINE TRACING)
118     N=0
119     5555 P(1,3)=P(1,2)+STEP12*(5.*P(4,3)+8.*P(4,2)-P(4,1))
120     N=N+1
121     P(2,3)=P(2,2)+STEP12*(5.*P(5,3)+8.*P(5,2)-P(5,1))
122     C******************PREDICTOR (FIELD LINE TRACING)
123     P(1,4)=P(1,3)+STEP12*(23.*P(4,3)-16.*P(4,2)+5.*P(4,1))
124     P(2,4)=P(2,3)+STEP12*(23.*P(5,3)-16.*P(5,2)+5.*P(5,1))
125     P(3,4)=P(3,3)+STEP
126     CALL STOER(P(1,4),BQ3,R3)
127     DO 1111 J=1,3
128     C DO 1111 I=1,8
129     DO 1111 I=1,7
130     1111 P(I,J)=P(I,J+1)
131     B=SQRT(BQ3)
132     IF(B.LT.BMIN) BMIN=B
133     IF(B.LE.BOLD) THEN
134     BOLD=B
135     ROLD=1./R3
136     SP(1)=P(1,4)
137     SP(2)=P(2,4)
138     SP(3)=P(3,4)
139     GOTO 5555
140     ENDIF
141     IF(BOLD.NE.BMIN) THEN
142     VALUE=.FALSE.
143     ENDIF
144     BDELTA=(B-BOLD)/BOLD
145     IF(BDELTA.GT.BDEL) THEN
146     STEP=STEP/10.
147     GOTO 7777
148     ENDIF
149     8888 RR0=ROLD
150     BEQU=BOLD
151     BDEL=BDELTA
152     RETURN
153     END
154     C
155     C
156     SUBROUTINE SHELLG(GLAT,GLON,ALT,DIMO,FL,ICODE,B0)
157     C--------------------------------------------------------------------
158     C CALCULATES L-VALUE FOR SPECIFIED GEODAETIC COORDINATES, ALTITUDE
159     C AND GEMAGNETIC FIELD MODEL.
160     C REF: G. KLUGE, EUROPEAN SPACE OPERATIONS CENTER, INTERNAL NOTE
161     C NO. 67, 1970.
162     C G. KLUGE, COMPUTER PHYSICS COMMUNICATIONS 3, 31-35, 1972
163     C--------------------------------------------------------------------
164     C CHANGES (D. BILITZA, NOV 87):
165     C - USING CORRECT DIPOL MOMENT I.E.,DIFFERENT COMMON/MODEL/
166     C - USING IGRF EARTH MAGNETIC FIELD MODELS FROM 1945 TO 1990
167     C--------------------------------------------------------------------
168     C INPUT: ENTRY POINT SHELLG
169     C GLAT GEODETIC LATITUDE IN DEGREES (NORTH)
170     C GLON GEODETIC LONGITUDE IN DEGREES (EAST)
171     C ALT ALTITUDE IN KM ABOVE SEA LEVEL
172     C
173     C ENTRY POINT SHELLC
174     C V(3) CARTESIAN COORDINATES IN EARTH RADII (6371.2 KM)
175     C X-AXIS POINTING TO EQUATOR AT 0 LONGITUDE
176     C Y-AXIS POINTING TO EQUATOR AT 90 LONG.
177     C Z-AXIS POINTING TO NORTH POLE
178     C
179     C DIMO DIPOL MOMENT IN GAUSS (NORMALIZED TO EARTH RADIUS)
180     C
181     C COMMON
182     C X(3) NOT USED
183     C H(144) FIELD MODEL COEFFICIENTS ADJUSTED FOR SHELLG
184     C-----------------------------------------------------------------------
185     C OUTPUT: FL L-VALUE
186     C ICODE =1 NORMAL COMPLETION
187     C =2 UNPHYSICAL CONJUGATE POINT (FL MEANINGLESS)
188     C =3 SHELL PARAMETER GREATER THAN LIMIT UP TO
189     C WHICH ACCURATE CALCULATION IS REQUIRED;
190     C APPROXIMATION IS USED.
191     C B0 MAGNETIC FIELD STRENGTH IN GAUSS
192     C-----------------------------------------------------------------------
193     DIMENSION V(3),U(3,3),P(8,100),SP(3)
194 mocchiut 1.6 COMMON X(3),H(196)
195 mocchiut 1.1 COMMON/FIDB0/ SP
196     SAVE /FIDB0/
197 mocchiut 1.9 COMMON/GENER/ UMR,ERA,AQUAD,BQUAD
198 mocchiut 1.1 SAVE /GENER/
199     C
200     C-- RMIN, RMAX ARE BOUNDARIES FOR IDENTIFICATION OF ICODE=2 AND 3
201     C-- STEP IS STEP SIZE FOR FIELD LINE TRACING
202     C-- STEQ IS STEP SIZE FOR INTEGRATION
203     C
204     DATA RMIN,RMAX /0.05,1.01/
205     DATA STEP,STEQ /0.20,0.03/
206     BEQU=1.E10
207     C*****ENTRY POINT SHELLG TO BE USED WITH GEODETIC CO-ORDINATES
208     RLAT=GLAT*UMR
209     CT=SIN(RLAT)
210     ST=COS(RLAT)
211     D=SQRT(AQUAD-(AQUAD-BQUAD)*CT*CT)
212     X(1)=(ALT+AQUAD/D)*ST/ERA
213     X(3)=(ALT+BQUAD/D)*CT/ERA
214     RLON=GLON*UMR
215     X(2)=X(1)*SIN(RLON)
216     X(1)=X(1)*COS(RLON)
217     GOTO9
218     ENTRY SHELLC(V,FL,B0)
219     C*****ENTRY POINT SHELLC TO BE USED WITH CARTESIAN CO-ORDINATES
220     X(1)=V(1)
221     X(2)=V(2)
222     X(3)=V(3)
223     C*****CONVERT TO DIPOL-ORIENTED CO-ORDINATES
224     DATA U/ +0.3511737,-0.9148385,-0.1993679,
225     A +0.9335804,+0.3583680,+0.0000000,
226     B +0.0714471,-0.1861260,+0.9799247/
227     9 RQ=1./(X(1)*X(1)+X(2)*X(2)+X(3)*X(3))
228     R3H=SQRT(RQ*SQRT(RQ))
229     P(1,2)=(X(1)*U(1,1)+X(2)*U(2,1)+X(3)*U(3,1))*R3H
230     P(2,2)=(X(1)*U(1,2)+X(2)*U(2,2) )*R3H
231     P(3,2)=(X(1)*U(1,3)+X(2)*U(2,3)+X(3)*U(3,3))*RQ
232     C*****FIRST THREE POINTS OF FIELD LINE
233     STEP=-SIGN(STEP,P(3,2))
234     CALL STOER(P(1,2),BQ2,R2)
235     B0=SQRT(BQ2)
236     P(1,3)=P(1,2)+0.5*STEP*P(4,2)
237     P(2,3)=P(2,2)+0.5*STEP*P(5,2)
238     P(3,3)=P(3,2)+0.5*STEP
239     CALL STOER(P(1,3),BQ3,R3)
240     P(1,1)=P(1,2)-STEP*(2.*P(4,2)-P(4,3))
241     P(2,1)=P(2,2)-STEP*(2.*P(5,2)-P(5,3))
242     P(3,1)=P(3,2)-STEP
243     CALL STOER(P(1,1),BQ1,R1)
244     P(1,3)=P(1,2)+STEP*(20.*P(4,3)-3.*P(4,2)+P(4,1))/18.
245     P(2,3)=P(2,2)+STEP*(20.*P(5,3)-3.*P(5,2)+P(5,1))/18.
246     P(3,3)=P(3,2)+STEP
247     CALL STOER(P(1,3),BQ3,R3)
248     C*****INVERT SENSE IF REQUIRED
249     IF(BQ3.LE.BQ1)GOTO2
250     STEP=-STEP
251     R3=R1
252     BQ3=BQ1
253     DO 1 I=1,7
254     ZZ=P(I,1)
255     P(I,1)=P(I,3)
256     1 P(I,3)=ZZ
257     C*****SEARCH FOR LOWEST MAGNETIC FIELD STRENGTH
258     2 IF(BQ1.LT.BEQU) THEN
259     BEQU=BQ1
260     IEQU=1
261     ENDIF
262     IF(BQ2.LT.BEQU) THEN
263     BEQU=BQ2
264     IEQU=2
265     ENDIF
266     IF(BQ3.LT.BEQU) THEN
267     BEQU=BQ3
268     IEQU=3
269     ENDIF
270     C*****INITIALIZATION OF INTEGRATION LOOPS
271     STEP12=STEP/12.
272     STEP2=STEP+STEP
273     STEQ=SIGN(STEQ,STEP)
274     FI=0.
275     ICODE=1
276     ORADIK=0.
277     OTERM=0.
278     STP=R2*STEQ
279     Z=P(3,2)+STP
280     STP=STP/0.75
281     P(8,1)=STEP2*(P(1,1)*P(4,1)+P(2,1)*P(5,1))
282     P(8,2)=STEP2*(P(1,2)*P(4,2)+P(2,2)*P(5,2))
283     C*****MAIN LOOP (FIELD LINE TRACING)
284     DO 3 N=3,3333
285     C*****CORRECTOR (FIELD LINE TRACING)
286     P(1,N)=P(1,N-1)+STEP12*(5.*P(4,N)+8.*P(4,N-1)-P(4,N-2))
287     P(2,N)=P(2,N-1)+STEP12*(5.*P(5,N)+8.*P(5,N-1)-P(5,N-2))
288     C*****PREPARE EXPANSION COEFFICIENTS FOR INTERPOLATION
289     C*****OF SLOWLY VARYING QUANTITIES
290     P(8,N)=STEP2*(P(1,N)*P(4,N)+P(2,N)*P(5,N))
291     C0=P(1,N-1)**2+P(2,N-1)**2
292     C1=P(8,N-1)
293     C2=(P(8,N)-P(8,N-2))*0.25
294     C3=(P(8,N)+P(8,N-2)-C1-C1)/6.0
295     D0=P(6,N-1)
296     D1=(P(6,N)-P(6,N-2))*0.5
297     D2=(P(6,N)+P(6,N-2)-D0-D0)*0.5
298     E0=P(7,N-1)
299     E1=(P(7,N)-P(7,N-2))*0.5
300     E2=(P(7,N)+P(7,N-2)-E0-E0)*0.5
301     C*****INNER LOOP (FOR QUADRATURE)
302     4 T=(Z-P(3,N-1))/STEP
303     IF(T.GT.1.)GOTO5
304     HLI=0.5*(((C3*T+C2)*T+C1)*T+C0)
305     ZQ=Z*Z
306     R=HLI+SQRT(HLI*HLI+ZQ)
307     IF(R.LE.RMIN)GOTO30
308     RQ=R*R
309     FF=SQRT(1.+3.*ZQ/RQ)
310     RADIK=B0-((D2*T+D1)*T+D0)*R*RQ*FF
311 mocchiut 1.3 IF((R-RMAX).le.0.) goto 44
312     IF((R-RMAX).gt.0.) goto 45
313 mocchiut 1.1 45 ICODE=2
314     RADIK=RADIK-12.*(R-RMAX)**2
315     44 IF(RADIK+RADIK.LE.ORADIK) GOTO 10
316     TERM=SQRT(RADIK)*FF*((E2*T+E1)*T+E0)/(RQ+ZQ)
317     FI=FI+STP*(OTERM+TERM)
318     ORADIK=RADIK
319     OTERM=TERM
320     STP=R*STEQ
321     Z=Z+STP
322     GOTO4
323     C*****PREDICTOR (FIELD LINE TRACING)
324     5 P(1,N+1)=P(1,N)+STEP12*(23.*P(4,N)-16.*P(4,N-1)+5.*P(4,N-2))
325     P(2,N+1)=P(2,N)+STEP12*(23.*P(5,N)-16.*P(5,N-1)+5.*P(5,N-2))
326     P(3,N+1)=P(3,N)+STEP
327     CALL STOER(P(1,N+1),BQ3,R3)
328     C*****SEARCH FOR LOWEST MAGNETIC FIELD STRENGTH
329     IF(BQ3.LT.BEQU) THEN
330     IEQU=N+1
331     BEQU=BQ3
332     ENDIF
333     3 CONTINUE
334     10 IF(IEQU.lt.2) IEQU=2
335     SP(1)=P(1,IEQU-1)
336     SP(2)=P(2,IEQU-1)
337     SP(3)=P(3,IEQU-1)
338     IF(ORADIK.LT.1E-15)GOTO11
339     FI=FI+STP/0.75*OTERM*ORADIK/(ORADIK-RADIK)
340     C
341     C-- The minimal allowable value of FI was changed from 1E-15 to 1E-12,
342     C-- because 1E-38 is the minimal allowable arg. for ALOG in our envir.
343     C-- D. Bilitza, Nov 87.
344     C
345 mocchiut 1.4 11 FI=0.5*ABS(FI)/SQRT(B0)+1E-12
346 mocchiut 1.1 C
347     C*****COMPUTE L FROM B AND I. SAME AS CARMEL IN INVAR.
348     C
349     C-- Correct dipole moment is used here. D. Bilitza, Nov 87.
350     C
351     DIMOB0=DIMO/B0
352 mocchiut 1.9 arg1=alog(FI)
353     arg2=alog(DIMOB0)
354 mocchiut 1.4 c arg = FI*FI*FI/DIMOB0
355     c if(abs(arg).gt.88.0) arg=88.0
356 mocchiut 1.1 XX=3*arg1-arg2
357     IF(XX.GT.23.0) GOTO 776
358     IF(XX.GT.11.7) GOTO 775
359     IF(XX.GT.+3.0) GOTO 774
360     IF(XX.GT.-3.0) GOTO 773
361     IF(XX.GT.-22.) GOTO 772
362 mocchiut 1.3 c 771 GG=3.33338E-1*XX+3.0062102E-1
363     GG=3.33338E-1*XX+3.0062102E-1
364 mocchiut 1.1 GOTO777
365     772 GG=((((((((-8.1537735E-14*XX+8.3232531E-13)*XX+1.0066362E-9)*XX+
366     18.1048663E-8)*XX+3.2916354E-6)*XX+8.2711096E-5)*XX+1.3714667E-3)*
367     2XX+1.5017245E-2)*XX+4.3432642E-1)*XX+6.2337691E-1
368     GOTO777
369     773 GG=((((((((2.6047023E-10*XX+2.3028767E-9)*XX-2.1997983E-8)*XX-
370     15.3977642E-7)*XX-3.3408822E-6)*XX+3.8379917E-5)*XX+1.1784234E-3)*
371     2XX+1.4492441E-2)*XX+4.3352788E-1)*XX+6.228644E-1
372     GOTO777
373     774 GG=((((((((6.3271665E-10*XX-3.958306E-8)*XX+9.9766148E-07)*XX-
374     11.2531932E-5)*XX+7.9451313E-5)*XX-3.2077032E-4)*XX+2.1680398E-3)*
375     2XX+1.2817956E-2)*XX+4.3510529E-1)*XX+6.222355E-1
376     GOTO777
377     775 GG=(((((2.8212095E-8*XX-3.8049276E-6)*XX+2.170224E-4)*XX-6.7310339
378     1E-3)*XX+1.2038224E-1)*XX-1.8461796E-1)*XX+2.0007187E0
379     GOTO777
380     776 GG=XX-3.0460681E0
381 mocchiut 1.9 777 FL=EXP(ALOG((1.+EXP(GG))*DIMOB0)/3.0)
382 mocchiut 1.1 RETURN
383     C*****APPROXIMATION FOR HIGH VALUES OF L.
384     30 ICODE=3
385     T=-P(3,N-1)/STEP
386     FL=1./(ABS(((C3*T+C2)*T+C1)*T+C0)+1E-15)
387     RETURN
388     END
389     C
390     C
391     SUBROUTINE STOER(P,BQ,R)
392     C*******************************************************************
393     C* SUBROUTINE USED FOR FIELD LINE TRACING IN SHELLG *
394     C* CALLS ENTRY POINT FELDI IN GEOMAGNETIC FIELD SUBROUTINE FELDG *
395     C*******************************************************************
396     DIMENSION P(7),U(3,3)
397 mocchiut 1.6 COMMON XI(3),H(196)
398 mocchiut 1.1 C*****XM,YM,ZM ARE GEOMAGNETIC CARTESIAN INVERSE CO-ORDINATES
399     ZM=P(3)
400     FLI=P(1)*P(1)+P(2)*P(2)+1E-15
401     R=0.5*(FLI+SQRT(FLI*FLI+(ZM+ZM)**2))
402     RQ=R*R
403     WR=SQRT(R)
404     XM=P(1)*WR
405     YM=P(2)*WR
406     C*****TRANSFORM TO GEOGRAPHIC CO-ORDINATE SYSTEM
407     DATA U/ +0.3511737,-0.9148385,-0.1993679,
408     A +0.9335804,+0.3583680,+0.0000000,
409     B +0.0714471,-0.1861260,+0.9799247/
410     XI(1)=XM*U(1,1)+YM*U(1,2)+ZM*U(1,3)
411     XI(2)=XM*U(2,1)+YM*U(2,2)+ZM*U(2,3)
412     XI(3)=XM*U(3,1) +ZM*U(3,3)
413     C*****COMPUTE DERIVATIVES
414     C CALL FELDI(XI,H)
415     CALL FELDI
416     Q=H(1)/RQ
417     DX=H(3)+H(3)+Q*XI(1)
418     DY=H(4)+H(4)+Q*XI(2)
419     DZ=H(2)+H(2)+Q*XI(3)
420     C*****TRANSFORM BACK TO GEOMAGNETIC CO-ORDINATE SYSTEM
421     DXM=U(1,1)*DX+U(2,1)*DY+U(3,1)*DZ
422     DYM=U(1,2)*DX+U(2,2)*DY
423     DZM=U(1,3)*DX+U(2,3)*DY+U(3,3)*DZ
424     DR=(XM*DXM+YM*DYM+ZM*DZM)/R
425     C*****FORM SLOWLY VARYING EXPRESSIONS
426     P(4)=(WR*DXM-0.5*P(1)*DR)/(R*DZM)
427     P(5)=(WR*DYM-0.5*P(2)*DR)/(R*DZM)
428     DSQ=RQ*(DXM*DXM+DYM*DYM+DZM*DZM)
429     BQ=DSQ*RQ*RQ
430     P(6)=SQRT(DSQ/(RQ+3.*ZM*ZM))
431     P(7)=P(6)*(RQ+ZM*ZM)/(RQ*DZM)
432     RETURN
433     END
434     C
435     C
436     SUBROUTINE FELDG(GLAT,GLON,ALT,BNORTH,BEAST,BDOWN,BABS)
437     C-------------------------------------------------------------------
438     C CALCULATES EARTH MAGNETIC FIELD FROM SPHERICAL HARMONICS MODEL
439     C REF: G. KLUGE, EUROPEAN SPACE OPERATIONS CENTRE, INTERNAL NOTE 61,
440     C 1970.
441     C--------------------------------------------------------------------
442     C CHANGES (D. BILITZA, NOV 87):
443     C - FIELD COEFFICIENTS IN BINARY DATA FILES INSTEAD OF BLOCK DATA
444     C - CALCULATES DIPOL MOMENT
445     C--------------------------------------------------------------------
446     C INPUT: ENTRY POINT FELDG
447     C GLAT GEODETIC LATITUDE IN DEGREES (NORTH)
448     C GLON GEODETIC LONGITUDE IN DEGREES (EAST)
449     C ALT ALTITUDE IN KM ABOVE SEA LEVEL
450     C
451     C ENTRY POINT FELDC
452     C V(3) CARTESIAN COORDINATES IN EARTH RADII (6371.2 KM)
453     C X-AXIS POINTING TO EQUATOR AT 0 LONGITUDE
454     C Y-AXIS POINTING TO EQUATOR AT 90 LONG.
455     C Z-AXIS POINTING TO NORTH POLE
456     C
457     C COMMON BLANK AND ENTRY POINT FELDI ARE NEEDED WHEN USED
458     C IN CONNECTION WITH L-CALCULATION PROGRAM SHELLG.
459     C
460     C COMMON /MODEL/ AND /GENER/
461     C UMR = ATAN(1.0)*4./180. <DEGREE>*UMR=<RADIANT>
462     C ERA EARTH RADIUS FOR NORMALIZATION OF CARTESIAN
463     C COORDINATES (6371.2 KM)
464     C AQUAD, BQUAD SQUARE OF MAJOR AND MINOR HALF AXIS FOR
465     C EARTH ELLIPSOID AS RECOMMENDED BY INTERNATIONAL
466     C ASTRONOMICAL UNION (6378.160, 6356.775 KM).
467     C NMAX MAXIMUM ORDER OF SPHERICAL HARMONICS
468     C TIME YEAR (DECIMAL: 1973.5) FOR WHICH MAGNETIC
469     C FIELD IS TO BE CALCULATED
470     C G(M) NORMALIZED FIELD COEFFICIENTS (SEE FELDCOF)
471     C M=NMAX*(NMAX+2)
472     C------------------------------------------------------------------------
473     C OUTPUT: BABS MAGNETIC FIELD STRENGTH IN GAUSS
474     C BNORTH, BEAST, BDOWN COMPONENTS OF THE FIELD WITH RESPECT
475     C TO THE LOCAL GEODETIC COORDINATE SYSTEM, WITH AXIS
476     C POINTING IN THE TANGENTIAL PLANE TO THE NORTH, EAST
477     C AND DOWNWARD.
478     C-----------------------------------------------------------------------
479 mocchiut 1.6 DIMENSION V(3),B(3),G(196)
480 mocchiut 1.1 CHARACTER*258 NAME
481     INTEGER NMAX
482     REAL TIME
483 mocchiut 1.6 COMMON XI(3),H(196)
484 mocchiut 1.1 COMMON/MODEL/ G,NMAX,TIME,NAME
485     SAVE/MODEL/
486 mocchiut 1.9 COMMON/GENER/ UMR,ERA,AQUAD,BQUAD
487 mocchiut 1.1 SAVE/GENER/
488     C
489     C-- IS RECORDS ENTRY POINT
490     C
491     C*****ENTRY POINT FELDG TO BE USED WITH GEODETIC CO-ORDINATES
492     IS=1
493     RLAT=GLAT*UMR
494     CT=SIN(RLAT)
495     ST=COS(RLAT)
496     D=SQRT(AQUAD-(AQUAD-BQUAD)*CT*CT)
497     RLON=GLON*UMR
498     CP=COS(RLON)
499     SP=SIN(RLON)
500     ZZZ=(ALT+BQUAD/D)*CT/ERA
501     RHO=(ALT+AQUAD/D)*ST/ERA
502     XXX=RHO*CP
503     YYY=RHO*SP
504     GOTO10
505     ENTRY FELDC(V,B)
506     C*****ENTRY POINT FELDC TO BE USED WITH CARTESIAN CO-ORDINATES
507     IS=2
508     XXX=V(1)
509     YYY=V(2)
510     ZZZ=V(3)
511     10 RQ=1./(XXX*XXX+YYY*YYY+ZZZ*ZZZ)
512     XI(1)=XXX*RQ
513     XI(2)=YYY*RQ
514     XI(3)=ZZZ*RQ
515     GOTO20
516     ENTRY FELDI
517     C*****ENTRY POINT FELDI USED FOR L COMPUTATION
518     IS=3
519     20 IHMAX=NMAX*NMAX+1
520     LAST=IHMAX+NMAX+NMAX
521     IMAX=NMAX+NMAX-1
522     DO 8 I=IHMAX,LAST
523     8 H(I)=G(I)
524     DO 6 K=1,3,2
525     I=IMAX
526     IH=IHMAX
527     1 IL=IH-I
528     F=2./FLOAT(I-K+2)
529     X=XI(1)*F
530     Y=XI(2)*F
531     Z=XI(3)*(F+F)
532     I=I-2
533 mocchiut 1.3 c print *,' I ',I
534     IF((I-1).lt.0) goto 5
535     IF((I-1).eq.0) goto 4
536     IF((I-1).gt.0) goto 2
537 mocchiut 1.1 2 DO 3 M=3,I,2
538     H(IL+M+1)=G(IL+M+1)+Z*H(IH+M+1)+X*(H(IH+M+3)-H(IH+M-1))
539     A -Y*(H(IH+M+2)+H(IH+M-2))
540     3 H(IL+M)=G(IL+M)+Z*H(IH+M)+X*(H(IH+M+2)-H(IH+M-2))
541     A +Y*(H(IH+M+3)+H(IH+M-1))
542     4 H(IL+2)=G(IL+2)+Z*H(IH+2)+X*H(IH+4)-Y*(H(IH+3)+H(IH))
543     H(IL+1)=G(IL+1)+Z*H(IH+1)+Y*H(IH+4)+X*(H(IH+3)-H(IH))
544     5 H(IL)=G(IL)+Z*H(IH)+2.*(X*H(IH+1)+Y*H(IH+2))
545     IH=IL
546     IF(I.GE.K)GOTO1
547     6 CONTINUE
548     IF(IS.EQ.3)RETURN
549     S=.5*H(1)+2.*(H(2)*XI(3)+H(3)*XI(1)+H(4)*XI(2))
550     T=(RQ+RQ)*SQRT(RQ)
551     BXXX=T*(H(3)-S*XXX)
552     BYYY=T*(H(4)-S*YYY)
553     BZZZ=T*(H(2)-S*ZZZ)
554     IF(IS.EQ.2)GOTO7
555     BABS=SQRT(BXXX*BXXX+BYYY*BYYY+BZZZ*BZZZ)
556     BEAST=BYYY*CP-BXXX*SP
557     BRHO=BYYY*SP+BXXX*CP
558     BNORTH=BZZZ*ST-BRHO*CT
559     BDOWN=-BZZZ*CT-BRHO*ST
560     RETURN
561     7 B(1)=BXXX
562     B(2)=BYYY
563     B(3)=BZZZ
564     RETURN
565     END
566     C
567     C
568 mocchiut 1.3 SUBROUTINE FELDCOF(YEAR,DIMO)
569 mocchiut 1.1 C------------------------------------------------------------------------
570 mocchiut 1.3 C DETERMINES COEFFICIENTS AND DIPOL MOMENT FROM IGRF MODELS
571     C
572     C INPUT: YEAR DECIMAL YEAR FOR WHICH GEOMAGNETIC FIELD IS TO
573     C BE CALCULATED
574     C OUTPUT: DIMO GEOMAGNETIC DIPOL MOMENT IN GAUSS (NORMALIZED
575     C TO EARTH'S RADIUS) AT THE TIME (YEAR)
576     C D. BILITZA, NSSDC, GSFC, CODE 633, GREENBELT, MD 20771,
577     C (301)286-9536 NOV 1987.
578     C ### updated to IGRF-2000 version -dkb- 5/31/2000
579     C ### updated to IGRF-2005 version -dkb- 3/24/2000
580 mocchiut 1.1 C-----------------------------------------------------------------------
581 mocchiut 1.3 CHARACTER*258 FIL1, FIL2
582     CHARACTER*258 FILMOD
583     C ### FILMOD, DTEMOD arrays +1
584 mocchiut 1.6 c DIMENSION GH1(144),GH2(120),GHA(144),FILMOD(14),DTEMOD(14)
585     DIMENSION GH1(196),GH2(196),GHA(196),FILMOD(3),DTEMOD(3)
586 mocchiut 1.3 DOUBLE PRECISION X,F0,F
587     INTEGER L1,L2,L3
588     INTEGER NMAX
589     REAL TIME
590     CHARACTER *258 P1,P2,P3
591     COMMON/PPATH/ L1,L2,L3,P1, P2, P3
592     SAVE/PPATH/
593     COMMON/MODEL/ GH1,NMAX,TIME,FIL1
594     SAVE/MODEL/
595 mocchiut 1.9 COMMON/GENER/ UMR,ERAD,AQUAD,BQUAD
596 mocchiut 1.3 SAVE/GENER/
597     C ### updated to 2005
598     C CHARACTER COEFPATH*80, COEF1*80, COEF2*80, COEF3*80
599    
600     c COEFPATH = 'OrbitalInfo/src/'
601     c COEF1 = 'dgrf00.dat'
602     c COEF2 = 'igrf05.dat'
603     c COEF3 = 'igrf05s.dat'
604     c COEF1 = COEFPATH(1:16)//COEF1
605     c COEF2 = COEFPATH(1:16)//COEF2
606     c COEF3 = COEFPATH(1:16)//COEF3
607     c FILMOD(1) = COEF1
608     c FILMOD(2) = COEF2
609     c FILMOD(3) = COEF3
610 mocchiut 1.7 c print *, "qui"
611 mocchiut 1.1 FILMOD(1) = P1(1:L1)
612     FILMOD(2) = P2(1:L2)
613     FILMOD(3) = P3(1:L3)
614 mocchiut 1.7 c print *, "qua"
615 mocchiut 1.3 c FILMOD(1) = 'OrbitalInfo/src/dgrf00.dat'
616     c FILMOD(2) = 'OrbitalInfo/src/igrf05.dat'
617     c FILMOD(3) = 'OrbitalInfo/src/igrf05s.dat'
618 mocchiut 1.7 c WRITE(*,*) FILMOD(1)
619     c WRITE(*,*) FILMOD(2)
620     c WRITE(*,*) FILMOD(3)
621 mocchiut 1.1 c DATA FILMOD / 'dgrf00.dat', 'igrf05.dat', 'igrf05s.dat'/
622 mocchiut 1.5 DATA DTEMOD / 2005., 2010., 2015./
623 mocchiut 1.3 c
624     c DATA FILMOD /'dgrf45.dat', 'dgrf50.dat',
625 mocchiut 1.1 c 1 'dgrf55.dat', 'dgrf60.dat', 'dgrf65.dat',
626     c 2 'dgrf70.dat', 'dgrf75.dat', 'dgrf80.dat',
627     c 3 'dgrf85.dat', 'dgrf90.dat', 'dgrf95.dat',
628     c 4 'dgrf00.dat','igrf05.dat','igrf05s.dat'/
629 mocchiut 1.3 c DATA DTEMOD / 1945., 1950., 1955., 1960., 1965., 1970.,
630 mocchiut 1.1 c 1 1975., 1980., 1985., 1990., 1995., 2000.,2005.,2010./
631 mocchiut 1.3 C
632     C ### numye = numye + 1 ; is number of years represented by IGRF
633     C
634     c NUMYE=13
635     NUMYE=2
636 mocchiut 1.7 c print *, "quo"
637 mocchiut 1.3
638     C
639     C IS=0 FOR SCHMIDT NORMALIZATION IS=1 GAUSS NORMALIZATION
640     C IU IS INPUT UNIT NUMBER FOR IGRF COEFFICIENT SETS
641     C
642     IU = 10
643     IS = 0
644     C-- DETERMINE IGRF-YEARS FOR INPUT-YEAR
645     TIME = YEAR
646     IYEA = INT(YEAR/5.)*5
647     c L = (IYEA - 1945)/5 + 1
648     L = (IYEA - 2000)/5 + 1
649     IF(L.LT.1) L=1
650     IF(L.GT.NUMYE) L=NUMYE
651     DTE1 = DTEMOD(L)
652     FIL1 = FILMOD(L)
653     DTE2 = DTEMOD(L+1)
654     FIL2 = FILMOD(L+1)
655 mocchiut 1.7 c WRITE(*,*) FIL1
656     c WRITE(*,*) FIL2
657     c print *, "que"
658 mocchiut 1.3 C-- GET IGRF COEFFICIENTS FOR THE BOUNDARY YEARS
659     CALL GETSHC (IU, FIL1, NMAX1, ERAD, GH1, IER)
660     IF (IER .NE. 0) STOP
661 mocchiut 1.7 c print *, "quessss"
662 mocchiut 1.3 CALL GETSHC (IU, FIL2, NMAX2, ERAD, GH2, IER)
663     IF (IER .NE. 0) STOP
664 mocchiut 1.7 c print *, "quj"
665 mocchiut 1.3 C-- DETERMINE IGRF COEFFICIENTS FOR YEAR
666     IF (L .LE. NUMYE-1) THEN
667     CALL INTERSHC (YEAR, DTE1, NMAX1, GH1, DTE2,
668     1 NMAX2, GH2, NMAX, GHA)
669     ELSE
670     CALL EXTRASHC (YEAR, DTE1, NMAX1, GH1, NMAX2,
671     1 GH2, NMAX, GHA)
672     ENDIF
673 mocchiut 1.7 c print *, "quw"
674 mocchiut 1.3 C-- DETERMINE MAGNETIC DIPOL MOMENT AND COEFFIECIENTS G
675     F0=0.D0
676     DO 1234 J=1,3
677     F = GHA(J) * 1.D-5
678     F0 = F0 + F * F
679     1234 CONTINUE
680 mocchiut 1.9 DIMO = REAL(DSQRT(F0))
681 mocchiut 1.3
682     GH1(1) = 0.0
683     I=2
684     F0=1.D-5
685     IF(IS.EQ.0) F0=-F0
686     SQRT2=SQRT(2.)
687 mocchiut 1.1
688 mocchiut 1.3 c print *, "quq"
689    
690 mocchiut 1.1 DO 9 N=1,NMAX
691 mocchiut 1.3 X = N
692     F0 = F0 * X * X / (4.D0 * X - 2.D0)
693     IF(IS.EQ.0) F0 = F0 * (2.D0 * X - 1.D0) / X
694     F = F0 * 0.5D0
695     IF(IS.EQ.0) F = F * SQRT2
696 mocchiut 1.9 GH1(I) = GHA(I-1) * REAL(F0)
697 mocchiut 1.3 I = I+1
698     DO 9 M=1,N
699     F = F * (X + M) / (X - M + 1.D0)
700     IF(IS.EQ.0) F = F * DSQRT((X - M + 1.D0) / (X + M))
701 mocchiut 1.9 GH1(I) = GHA(I-1) * REAL(F)
702     GH1(I+1) = GHA(I) * REAL(F)
703 mocchiut 1.3 I=I+2
704     9 CONTINUE
705     RETURN
706     END
707     C
708     C
709     SUBROUTINE GETSHC (IU, FSPEC, NMAX, ERAD, GH, IER)
710 mocchiut 1.9
711 mocchiut 1.1 C ===============================================================
712     C
713 mocchiut 1.3 C Version 1.01
714     C
715     C Reads spherical harmonic coefficients from the specified
716     C file into an array.
717     C
718     C Input:
719     C IU - Logical unit number
720     C FSPEC - File specification
721     C
722     C Output:
723     C NMAX - Maximum degree and order of model
724     C ERAD - Earth's radius associated with the spherical
725     C harmonic coefficients, in the same units as
726     C elevation
727     C GH - Schmidt quasi-normal internal spherical
728     C harmonic coefficients
729     C IER - Error number: = 0, no error
730     C = -2, records out of order
731     C = FORTRAN run-time error number
732     C
733     C A. Zunde
734     C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225
735     C
736     C ===============================================================
737    
738     CHARACTER FSPEC*(*), FOUT*258
739     DIMENSION GH(*)
740     C ---------------------------------------------------------------
741     C Open coefficient file. Read past first header record.
742     C Read degree and order of model and Earth's radius.
743     C ---------------------------------------------------------------
744 mocchiut 1.1 WRITE(FOUT,667) FSPEC
745 mocchiut 1.3 c 667 FORMAT('/usr/local/etc/httpd/cgi-bin/natasha/IRI/',A12)
746     667 FORMAT(A258)
747 mocchiut 1.7 c print *," gui"
748 mocchiut 1.1 OPEN (IU, FILE=FOUT, STATUS='OLD', IOSTAT=IER, ERR=999)
749 mocchiut 1.7 c print *," gua"
750 mocchiut 1.1 READ (IU, *, IOSTAT=IER, ERR=999)
751 mocchiut 1.7 c print *," gue"
752 mocchiut 1.1 READ (IU, *, IOSTAT=IER, ERR=999) NMAX, ERAD
753 mocchiut 1.7 c print *," guo"
754 mocchiut 1.1 C ---------------------------------------------------------------
755     C Read the coefficient file, arranged as follows:
756     C
757     C N M G H
758     C ----------------------
759     C / 1 0 GH(1) -
760     C / 1 1 GH(2) GH(3)
761     C / 2 0 GH(4) -
762     C / 2 1 GH(5) GH(6)
763     C NMAX*(NMAX+3)/2 / 2 2 GH(7) GH(8)
764     C records \ 3 0 GH(9) -
765     C \ . . . .
766     C \ . . . .
767     C NMAX*(NMAX+2) \ . . . .
768     C elements in GH \ NMAX NMAX . .
769     C
770     C N and M are, respectively, the degree and order of the
771     C coefficient.
772     C ---------------------------------------------------------------
773    
774     I = 0
775 mocchiut 1.3 DO 2211 NN = 1, NMAX
776     DO 2233 MM = 0, NN
777 mocchiut 1.1 READ (IU, *, IOSTAT=IER, ERR=999) N, M, G, H
778     IF (NN .NE. N .OR. MM .NE. M) THEN
779     IER = -2
780     GOTO 999
781     ENDIF
782     I = I + 1
783     GH(I) = G
784     IF (M .NE. 0) THEN
785     I = I + 1
786     GH(I) = H
787     ENDIF
788     2233 CONTINUE
789     2211 CONTINUE
790 mocchiut 1.7 c print *," guj"
791 mocchiut 1.1
792     999 CLOSE (IU)
793 mocchiut 1.7 c print *," guw IER",IER
794 mocchiut 1.3 if ( IER .eq. -1 ) IER = 0 ! gfortran 4.1.2 bug workaround... hoping not to create problems with other versions
795 mocchiut 1.1
796     RETURN
797     END
798     C
799     C
800     SUBROUTINE INTERSHC (DATE, DTE1, NMAX1, GH1, DTE2,
801     1 NMAX2, GH2, NMAX, GH)
802 mocchiut 1.9
803 mocchiut 1.1 C ===============================================================
804     C
805     C Version 1.01
806     C
807     C Interpolates linearly, in time, between two spherical
808     C harmonic models.
809     C
810     C Input:
811     C DATE - Date of resulting model (in decimal year)
812     C DTE1 - Date of earlier model
813     C NMAX1 - Maximum degree and order of earlier model
814     C GH1 - Schmidt quasi-normal internal spherical
815     C harmonic coefficients of earlier model
816     C DTE2 - Date of later model
817     C NMAX2 - Maximum degree and order of later model
818     C GH2 - Schmidt quasi-normal internal spherical
819     C harmonic coefficients of later model
820     C
821     C Output:
822     C GH - Coefficients of resulting model
823     C NMAX - Maximum degree and order of resulting model
824     C
825     C A. Zunde
826     C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225
827     C
828     C ===============================================================
829    
830     DIMENSION GH1(*), GH2(*), GH(*)
831    
832     C ---------------------------------------------------------------
833     C The coefficients (GH) of the resulting model, at date
834     C DATE, are computed by linearly interpolating between the
835     C coefficients of the earlier model (GH1), at date DTE1,
836     C and those of the later model (GH2), at date DTE2. If one
837     C model is smaller than the other, the interpolation is
838     C performed with the missing coefficients assumed to be 0.
839     C ---------------------------------------------------------------
840    
841     FACTOR = (DATE - DTE1) / (DTE2 - DTE1)
842    
843     IF (NMAX1 .EQ. NMAX2) THEN
844     K = NMAX1 * (NMAX1 + 2)
845     NMAX = NMAX1
846     ELSE IF (NMAX1 .GT. NMAX2) THEN
847     K = NMAX2 * (NMAX2 + 2)
848     L = NMAX1 * (NMAX1 + 2)
849 mocchiut 1.3 DO 1122 I = K + 1, L
850 mocchiut 1.1 1122 GH(I) = GH1(I) + FACTOR * (-GH1(I))
851     NMAX = NMAX1
852     ELSE
853     K = NMAX1 * (NMAX1 + 2)
854     L = NMAX2 * (NMAX2 + 2)
855 mocchiut 1.3 DO 1133 I = K + 1, L
856 mocchiut 1.1 1133 GH(I) = FACTOR * GH2(I)
857     NMAX = NMAX2
858     ENDIF
859    
860 mocchiut 1.3 DO 1144 I = 1, K
861 mocchiut 1.1 1144 GH(I) = GH1(I) + FACTOR * (GH2(I) - GH1(I))
862    
863     RETURN
864     END
865     C
866     C
867     SUBROUTINE EXTRASHC (DATE, DTE1, NMAX1, GH1, NMAX2,
868     1 GH2, NMAX, GH)
869    
870     C ===============================================================
871     C
872     C Version 1.01
873     C
874     C Extrapolates linearly a spherical harmonic model with a
875     C rate-of-change model.
876     C
877     C Input:
878     C DATE - Date of resulting model (in decimal year)
879     C DTE1 - Date of base model
880     C NMAX1 - Maximum degree and order of base model
881     C GH1 - Schmidt quasi-normal internal spherical
882     C harmonic coefficients of base model
883     C NMAX2 - Maximum degree and order of rate-of-change
884     C model
885     C GH2 - Schmidt quasi-normal internal spherical
886     C harmonic coefficients of rate-of-change model
887     C
888     C Output:
889     C GH - Coefficients of resulting model
890     C NMAX - Maximum degree and order of resulting model
891     C
892     C A. Zunde
893     C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225
894     C
895     C ===============================================================
896    
897     DIMENSION GH1(*), GH2(*), GH(*)
898    
899     C ---------------------------------------------------------------
900     C The coefficients (GH) of the resulting model, at date
901     C DATE, are computed by linearly extrapolating the coef-
902     C ficients of the base model (GH1), at date DTE1, using
903     C those of the rate-of-change model (GH2), at date DTE2. If
904     C one model is smaller than the other, the extrapolation is
905     C performed with the missing coefficients assumed to be 0.
906     C ---------------------------------------------------------------
907    
908     FACTOR = (DATE - DTE1)
909    
910     IF (NMAX1 .EQ. NMAX2) THEN
911     K = NMAX1 * (NMAX1 + 2)
912     NMAX = NMAX1
913     ELSE IF (NMAX1 .GT. NMAX2) THEN
914     K = NMAX2 * (NMAX2 + 2)
915     L = NMAX1 * (NMAX1 + 2)
916 mocchiut 1.3 DO 1155 I = K + 1, L
917 mocchiut 1.1 1155 GH(I) = GH1(I)
918     NMAX = NMAX1
919     ELSE
920     K = NMAX1 * (NMAX1 + 2)
921     L = NMAX2 * (NMAX2 + 2)
922 mocchiut 1.3 DO 1166 I = K + 1, L
923 mocchiut 1.1 1166 GH(I) = FACTOR * GH2(I)
924     NMAX = NMAX2
925     ENDIF
926    
927 mocchiut 1.3 DO 1177 I = 1, K
928 mocchiut 1.1 1177 GH(I) = GH1(I) + FACTOR * GH2(I)
929    
930     RETURN
931     END
932     C
933     C
934     SUBROUTINE INITIZE(TP1,TL1,TP2,TL2,TP3,TL3)
935     C----------------------------------------------------------------
936     C Initializes the parameters in COMMON/GENER/
937     C
938     C UMR = ATAN(1.0)*4./180. <DEGREE>*UMR=<RADIANT>
939     C ERA EARTH RADIUS FOR NORMALIZATION OF CARTESIAN
940     C COORDINATES (6371.2 KM)
941     C EREQU MAJOR HALF AXIS FOR EARTH ELLIPSOID (6378.160 KM)
942     C ERPOL MINOR HALF AXIS FOR EARTH ELLIPSOID (6356.775 KM)
943     C AQUAD SQUARE OF MAJOR HALF AXIS FOR EARTH ELLIPSOID
944     C BQUAD SQUARE OF MINOR HALF AXIS FOR EARTH ELLIPSOID
945     C
946     C ERA, EREQU and ERPOL as recommended by the INTERNATIONAL
947     C ASTRONOMICAL UNION .
948     C-----------------------------------------------------------------
949     INTEGER TL1,TL2,TL3
950 mocchiut 1.10 CHARACTER (len=*) :: TP1,TP2,TP3
951 mocchiut 1.1 INTEGER L1,L2,L3
952     CHARACTER *258 P1,P2,P3
953     COMMON/PPATH/ L1,L2,L3,P1, P2, P3
954     SAVE/PPATH/
955    
956 mocchiut 1.9 COMMON/GENER/UMR,ERA,AQUAD,BQUAD
957 mocchiut 1.1 SAVE/GENER/
958    
959     L1 = TL1
960     L2 = TL2
961     L3 = TL3
962 mocchiut 1.2 P1 = TP1(1:L1)
963     P2 = TP2(1:L2)
964     P3 = TP3(1:L3)
965 mocchiut 1.1
966     ERA=6371.2
967     EREQU=6378.16
968     ERPOL=6356.775
969     AQUAD=EREQU*EREQU
970     BQUAD=ERPOL*ERPOL
971     UMR=ATAN(1.0)*4./180.
972     RETURN
973     END

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