1 |
mocchiut |
1.12 |
C |
2 |
mocchiut |
1.1 |
C SHELLIG.FOR, Version 2.0, January 1992 |
3 |
|
|
C |
4 |
|
|
C 11/01/91-DKB- SHELLG: lowest starting point for B0 search is 2 |
5 |
|
|
C 1/27/92-DKB- Adopted to IGRF-91 coeffcients model |
6 |
|
|
C 2/05/92-DKB- Reduce variable-names: INTER(P)SHC,EXTRA(P)SHC,INITI(ALI)ZE |
7 |
|
|
C 8/08/95-DKB- Updated to IGRF-45-95; new coeff. DGRF90, IGRF95, IGRF95S |
8 |
|
|
C 5/31/00-DKB- Updated to IGRF-45-00; new coeff.: IGRF00, IGRF00s |
9 |
|
|
C 3/24/05-DKB- Updated to IGRF-45-10; new coeff.: IGRF05, IGRF05s |
10 |
|
|
C 4/25/05-DKB- CALL FELDI and DO 1111 I=1,7 [Alexey Petrov] |
11 |
|
|
C |
12 |
|
|
C********************************************************************* |
13 |
|
|
C SUBROUTINES FINDB0, SHELLG, STOER, FELDG, FELDCOF, GETSHC, * |
14 |
|
|
C INTERSHC, EXTRASHC, INITIZE * |
15 |
|
|
C********************************************************************* |
16 |
|
|
C********************************************************************* |
17 |
|
|
C |
18 |
|
|
C |
19 |
|
|
SUBROUTINE FINDB0(STPS,BDEL,VALUE,BEQU,RR0) |
20 |
|
|
C-------------------------------------------------------------------- |
21 |
|
|
C FINDS SMALLEST MAGNETIC FIELD STRENGTH ON FIELD LINE |
22 |
|
|
C |
23 |
|
|
C INPUT: STPS STEP SIZE FOR FIELD LINE TRACING |
24 |
|
|
C COMMON/FIDB0/ |
25 |
|
|
C SP DIPOLE ORIENTED COORDINATES FORM SHELLG; P(1,*), |
26 |
|
|
C P(2,*), P(3,*) CLOSEST TO MAGNETIC EQUATOR |
27 |
|
|
C BDEL REQUIRED ACCURACY = [ B(LAST) - BEQU ] / BEQU |
28 |
|
|
C B(LAST) IS FIELD STRENGTH BEFORE BEQU |
29 |
|
|
C |
30 |
|
|
C OUTPUT: VALUE =.FALSE., IF BEQU IS NOT MINIMAL VALUE ON FIELD LINE |
31 |
|
|
C BEQU MAGNETIC FIELD STRENGTH AT MAGNETIC EQUATOR |
32 |
|
|
C RR0 EQUATORIAL RADIUS NORMALIZED TO EARTH RADIUS |
33 |
|
|
C BDEL FINAL ACHIEVED ACCURACY |
34 |
|
|
C-------------------------------------------------------------------- |
35 |
|
|
DIMENSION P(8,4),SP(3) |
36 |
|
|
LOGICAL VALUE |
37 |
|
|
COMMON/FIDB0/ SP |
38 |
|
|
SAVE /FIDB0/ |
39 |
|
|
C |
40 |
|
|
STEP=STPS |
41 |
|
|
IRUN=0 |
42 |
|
|
7777 IRUN=IRUN+1 |
43 |
|
|
IF(IRUN.GT.5) THEN |
44 |
|
|
VALUE=.FALSE. |
45 |
|
|
GOTO 8888 |
46 |
|
|
ENDIF |
47 |
|
|
C*********************FIRST THREE POINTS |
48 |
|
|
P(1,2)=SP(1) |
49 |
|
|
P(2,2)=SP(2) |
50 |
|
|
P(3,2)=SP(3) |
51 |
|
|
STEP=-SIGN(STEP,P(3,2)) |
52 |
|
|
CALL STOER(P(1,2),BQ2,R2) |
53 |
|
|
P(1,3)=P(1,2)+0.5*STEP*P(4,2) |
54 |
|
|
P(2,3)=P(2,2)+0.5*STEP*P(5,2) |
55 |
|
|
P(3,3)=P(3,2)+0.5*STEP |
56 |
|
|
CALL STOER(P(1,3),BQ3,R3) |
57 |
|
|
P(1,1)=P(1,2)-STEP*(2.*P(4,2)-P(4,3)) |
58 |
|
|
P(2,1)=P(2,2)-STEP*(2.*P(5,2)-P(5,3)) |
59 |
|
|
P(3,1)=P(3,2)-STEP |
60 |
|
|
CALL STOER(P(1,1),BQ1,R1) |
61 |
|
|
P(1,3)=P(1,2)+STEP*(20.*P(4,3)-3.*P(4,2)+P(4,1))/18. |
62 |
|
|
P(2,3)=P(2,2)+STEP*(20.*P(5,3)-3.*P(5,2)+P(5,1))/18. |
63 |
|
|
P(3,3)=P(3,2)+STEP |
64 |
|
|
CALL STOER(P(1,3),BQ3,R3) |
65 |
|
|
C******************INVERT SENSE IF REQUIRED |
66 |
|
|
IF(BQ3.LE.BQ1) GOTO 2 |
67 |
|
|
STEP=-STEP |
68 |
|
|
R3=R1 |
69 |
|
|
BQ3=BQ1 |
70 |
|
|
DO 1 I=1,5 |
71 |
|
|
ZZ=P(I,1) |
72 |
|
|
P(I,1)=P(I,3) |
73 |
|
|
1 P(I,3)=ZZ |
74 |
|
|
C******************INITIALIZATION |
75 |
|
|
2 STEP12=STEP/12. |
76 |
|
|
VALUE=.TRUE. |
77 |
|
|
BMIN=1.E4 |
78 |
|
|
BOLD=1.E4 |
79 |
|
|
C******************CORRECTOR (FIELD LINE TRACING) |
80 |
|
|
N=0 |
81 |
|
|
5555 P(1,3)=P(1,2)+STEP12*(5.*P(4,3)+8.*P(4,2)-P(4,1)) |
82 |
|
|
N=N+1 |
83 |
|
|
P(2,3)=P(2,2)+STEP12*(5.*P(5,3)+8.*P(5,2)-P(5,1)) |
84 |
|
|
C******************PREDICTOR (FIELD LINE TRACING) |
85 |
|
|
P(1,4)=P(1,3)+STEP12*(23.*P(4,3)-16.*P(4,2)+5.*P(4,1)) |
86 |
|
|
P(2,4)=P(2,3)+STEP12*(23.*P(5,3)-16.*P(5,2)+5.*P(5,1)) |
87 |
|
|
P(3,4)=P(3,3)+STEP |
88 |
|
|
CALL STOER(P(1,4),BQ3,R3) |
89 |
|
|
DO 1111 J=1,3 |
90 |
|
|
C DO 1111 I=1,8 |
91 |
|
|
DO 1111 I=1,7 |
92 |
|
|
1111 P(I,J)=P(I,J+1) |
93 |
|
|
B=SQRT(BQ3) |
94 |
|
|
IF(B.LT.BMIN) BMIN=B |
95 |
|
|
IF(B.LE.BOLD) THEN |
96 |
|
|
BOLD=B |
97 |
|
|
ROLD=1./R3 |
98 |
|
|
SP(1)=P(1,4) |
99 |
|
|
SP(2)=P(2,4) |
100 |
|
|
SP(3)=P(3,4) |
101 |
|
|
GOTO 5555 |
102 |
|
|
ENDIF |
103 |
|
|
IF(BOLD.NE.BMIN) THEN |
104 |
|
|
VALUE=.FALSE. |
105 |
|
|
ENDIF |
106 |
|
|
BDELTA=(B-BOLD)/BOLD |
107 |
|
|
IF(BDELTA.GT.BDEL) THEN |
108 |
|
|
STEP=STEP/10. |
109 |
|
|
GOTO 7777 |
110 |
|
|
ENDIF |
111 |
|
|
8888 RR0=ROLD |
112 |
|
|
BEQU=BOLD |
113 |
|
|
BDEL=BDELTA |
114 |
|
|
RETURN |
115 |
|
|
END |
116 |
|
|
C |
117 |
|
|
C |
118 |
|
|
SUBROUTINE SHELLG(GLAT,GLON,ALT,DIMO,FL,ICODE,B0) |
119 |
|
|
C-------------------------------------------------------------------- |
120 |
|
|
C CALCULATES L-VALUE FOR SPECIFIED GEODAETIC COORDINATES, ALTITUDE |
121 |
|
|
C AND GEMAGNETIC FIELD MODEL. |
122 |
|
|
C REF: G. KLUGE, EUROPEAN SPACE OPERATIONS CENTER, INTERNAL NOTE |
123 |
|
|
C NO. 67, 1970. |
124 |
|
|
C G. KLUGE, COMPUTER PHYSICS COMMUNICATIONS 3, 31-35, 1972 |
125 |
|
|
C-------------------------------------------------------------------- |
126 |
|
|
C CHANGES (D. BILITZA, NOV 87): |
127 |
|
|
C - USING CORRECT DIPOL MOMENT I.E.,DIFFERENT COMMON/MODEL/ |
128 |
|
|
C - USING IGRF EARTH MAGNETIC FIELD MODELS FROM 1945 TO 1990 |
129 |
|
|
C-------------------------------------------------------------------- |
130 |
|
|
C INPUT: ENTRY POINT SHELLG |
131 |
|
|
C GLAT GEODETIC LATITUDE IN DEGREES (NORTH) |
132 |
|
|
C GLON GEODETIC LONGITUDE IN DEGREES (EAST) |
133 |
|
|
C ALT ALTITUDE IN KM ABOVE SEA LEVEL |
134 |
|
|
C |
135 |
|
|
C ENTRY POINT SHELLC |
136 |
|
|
C V(3) CARTESIAN COORDINATES IN EARTH RADII (6371.2 KM) |
137 |
|
|
C X-AXIS POINTING TO EQUATOR AT 0 LONGITUDE |
138 |
|
|
C Y-AXIS POINTING TO EQUATOR AT 90 LONG. |
139 |
|
|
C Z-AXIS POINTING TO NORTH POLE |
140 |
|
|
C |
141 |
|
|
C DIMO DIPOL MOMENT IN GAUSS (NORMALIZED TO EARTH RADIUS) |
142 |
|
|
C |
143 |
|
|
C COMMON |
144 |
|
|
C X(3) NOT USED |
145 |
|
|
C H(144) FIELD MODEL COEFFICIENTS ADJUSTED FOR SHELLG |
146 |
|
|
C----------------------------------------------------------------------- |
147 |
|
|
C OUTPUT: FL L-VALUE |
148 |
|
|
C ICODE =1 NORMAL COMPLETION |
149 |
|
|
C =2 UNPHYSICAL CONJUGATE POINT (FL MEANINGLESS) |
150 |
|
|
C =3 SHELL PARAMETER GREATER THAN LIMIT UP TO |
151 |
|
|
C WHICH ACCURATE CALCULATION IS REQUIRED; |
152 |
|
|
C APPROXIMATION IS USED. |
153 |
|
|
C B0 MAGNETIC FIELD STRENGTH IN GAUSS |
154 |
|
|
C----------------------------------------------------------------------- |
155 |
|
|
DIMENSION V(3),U(3,3),P(8,100),SP(3) |
156 |
mocchiut |
1.6 |
COMMON X(3),H(196) |
157 |
mocchiut |
1.1 |
COMMON/FIDB0/ SP |
158 |
|
|
SAVE /FIDB0/ |
159 |
mocchiut |
1.9 |
COMMON/GENER/ UMR,ERA,AQUAD,BQUAD |
160 |
mocchiut |
1.1 |
SAVE /GENER/ |
161 |
mocchiut |
1.11 |
REAL FLS |
162 |
mocchiut |
1.1 |
C |
163 |
|
|
C-- RMIN, RMAX ARE BOUNDARIES FOR IDENTIFICATION OF ICODE=2 AND 3 |
164 |
|
|
C-- STEP IS STEP SIZE FOR FIELD LINE TRACING |
165 |
|
|
C-- STEQ IS STEP SIZE FOR INTEGRATION |
166 |
|
|
C |
167 |
|
|
DATA RMIN,RMAX /0.05,1.01/ |
168 |
|
|
DATA STEP,STEQ /0.20,0.03/ |
169 |
mocchiut |
1.11 |
BEQU=1.E10 |
170 |
|
|
FLS = FL |
171 |
mocchiut |
1.1 |
C*****ENTRY POINT SHELLG TO BE USED WITH GEODETIC CO-ORDINATES |
172 |
|
|
RLAT=GLAT*UMR |
173 |
|
|
CT=SIN(RLAT) |
174 |
|
|
ST=COS(RLAT) |
175 |
|
|
D=SQRT(AQUAD-(AQUAD-BQUAD)*CT*CT) |
176 |
|
|
X(1)=(ALT+AQUAD/D)*ST/ERA |
177 |
|
|
X(3)=(ALT+BQUAD/D)*CT/ERA |
178 |
|
|
RLON=GLON*UMR |
179 |
|
|
X(2)=X(1)*SIN(RLON) |
180 |
|
|
X(1)=X(1)*COS(RLON) |
181 |
|
|
GOTO9 |
182 |
|
|
ENTRY SHELLC(V,FL,B0) |
183 |
|
|
C*****ENTRY POINT SHELLC TO BE USED WITH CARTESIAN CO-ORDINATES |
184 |
|
|
X(1)=V(1) |
185 |
|
|
X(2)=V(2) |
186 |
|
|
X(3)=V(3) |
187 |
|
|
C*****CONVERT TO DIPOL-ORIENTED CO-ORDINATES |
188 |
|
|
DATA U/ +0.3511737,-0.9148385,-0.1993679, |
189 |
|
|
A +0.9335804,+0.3583680,+0.0000000, |
190 |
|
|
B +0.0714471,-0.1861260,+0.9799247/ |
191 |
|
|
9 RQ=1./(X(1)*X(1)+X(2)*X(2)+X(3)*X(3)) |
192 |
|
|
R3H=SQRT(RQ*SQRT(RQ)) |
193 |
|
|
P(1,2)=(X(1)*U(1,1)+X(2)*U(2,1)+X(3)*U(3,1))*R3H |
194 |
|
|
P(2,2)=(X(1)*U(1,2)+X(2)*U(2,2) )*R3H |
195 |
|
|
P(3,2)=(X(1)*U(1,3)+X(2)*U(2,3)+X(3)*U(3,3))*RQ |
196 |
|
|
C*****FIRST THREE POINTS OF FIELD LINE |
197 |
|
|
STEP=-SIGN(STEP,P(3,2)) |
198 |
|
|
CALL STOER(P(1,2),BQ2,R2) |
199 |
|
|
B0=SQRT(BQ2) |
200 |
|
|
P(1,3)=P(1,2)+0.5*STEP*P(4,2) |
201 |
|
|
P(2,3)=P(2,2)+0.5*STEP*P(5,2) |
202 |
|
|
P(3,3)=P(3,2)+0.5*STEP |
203 |
|
|
CALL STOER(P(1,3),BQ3,R3) |
204 |
|
|
P(1,1)=P(1,2)-STEP*(2.*P(4,2)-P(4,3)) |
205 |
|
|
P(2,1)=P(2,2)-STEP*(2.*P(5,2)-P(5,3)) |
206 |
|
|
P(3,1)=P(3,2)-STEP |
207 |
|
|
CALL STOER(P(1,1),BQ1,R1) |
208 |
|
|
P(1,3)=P(1,2)+STEP*(20.*P(4,3)-3.*P(4,2)+P(4,1))/18. |
209 |
|
|
P(2,3)=P(2,2)+STEP*(20.*P(5,3)-3.*P(5,2)+P(5,1))/18. |
210 |
|
|
P(3,3)=P(3,2)+STEP |
211 |
|
|
CALL STOER(P(1,3),BQ3,R3) |
212 |
|
|
C*****INVERT SENSE IF REQUIRED |
213 |
|
|
IF(BQ3.LE.BQ1)GOTO2 |
214 |
|
|
STEP=-STEP |
215 |
|
|
R3=R1 |
216 |
|
|
BQ3=BQ1 |
217 |
|
|
DO 1 I=1,7 |
218 |
|
|
ZZ=P(I,1) |
219 |
|
|
P(I,1)=P(I,3) |
220 |
|
|
1 P(I,3)=ZZ |
221 |
|
|
C*****SEARCH FOR LOWEST MAGNETIC FIELD STRENGTH |
222 |
|
|
2 IF(BQ1.LT.BEQU) THEN |
223 |
|
|
BEQU=BQ1 |
224 |
|
|
IEQU=1 |
225 |
|
|
ENDIF |
226 |
|
|
IF(BQ2.LT.BEQU) THEN |
227 |
|
|
BEQU=BQ2 |
228 |
|
|
IEQU=2 |
229 |
|
|
ENDIF |
230 |
|
|
IF(BQ3.LT.BEQU) THEN |
231 |
|
|
BEQU=BQ3 |
232 |
|
|
IEQU=3 |
233 |
|
|
ENDIF |
234 |
|
|
C*****INITIALIZATION OF INTEGRATION LOOPS |
235 |
|
|
STEP12=STEP/12. |
236 |
|
|
STEP2=STEP+STEP |
237 |
|
|
STEQ=SIGN(STEQ,STEP) |
238 |
|
|
FI=0. |
239 |
|
|
ICODE=1 |
240 |
|
|
ORADIK=0. |
241 |
|
|
OTERM=0. |
242 |
|
|
STP=R2*STEQ |
243 |
|
|
Z=P(3,2)+STP |
244 |
|
|
STP=STP/0.75 |
245 |
|
|
P(8,1)=STEP2*(P(1,1)*P(4,1)+P(2,1)*P(5,1)) |
246 |
|
|
P(8,2)=STEP2*(P(1,2)*P(4,2)+P(2,2)*P(5,2)) |
247 |
|
|
C*****MAIN LOOP (FIELD LINE TRACING) |
248 |
|
|
DO 3 N=3,3333 |
249 |
|
|
C*****CORRECTOR (FIELD LINE TRACING) |
250 |
|
|
P(1,N)=P(1,N-1)+STEP12*(5.*P(4,N)+8.*P(4,N-1)-P(4,N-2)) |
251 |
|
|
P(2,N)=P(2,N-1)+STEP12*(5.*P(5,N)+8.*P(5,N-1)-P(5,N-2)) |
252 |
|
|
C*****PREPARE EXPANSION COEFFICIENTS FOR INTERPOLATION |
253 |
|
|
C*****OF SLOWLY VARYING QUANTITIES |
254 |
|
|
P(8,N)=STEP2*(P(1,N)*P(4,N)+P(2,N)*P(5,N)) |
255 |
|
|
C0=P(1,N-1)**2+P(2,N-1)**2 |
256 |
|
|
C1=P(8,N-1) |
257 |
|
|
C2=(P(8,N)-P(8,N-2))*0.25 |
258 |
|
|
C3=(P(8,N)+P(8,N-2)-C1-C1)/6.0 |
259 |
|
|
D0=P(6,N-1) |
260 |
|
|
D1=(P(6,N)-P(6,N-2))*0.5 |
261 |
|
|
D2=(P(6,N)+P(6,N-2)-D0-D0)*0.5 |
262 |
|
|
E0=P(7,N-1) |
263 |
|
|
E1=(P(7,N)-P(7,N-2))*0.5 |
264 |
|
|
E2=(P(7,N)+P(7,N-2)-E0-E0)*0.5 |
265 |
|
|
C*****INNER LOOP (FOR QUADRATURE) |
266 |
|
|
4 T=(Z-P(3,N-1))/STEP |
267 |
|
|
IF(T.GT.1.)GOTO5 |
268 |
|
|
HLI=0.5*(((C3*T+C2)*T+C1)*T+C0) |
269 |
|
|
ZQ=Z*Z |
270 |
|
|
R=HLI+SQRT(HLI*HLI+ZQ) |
271 |
mocchiut |
1.11 |
IF(R.NE.R)THEN |
272 |
|
|
FL = FLS |
273 |
|
|
RETURN |
274 |
|
|
ENDIF |
275 |
mocchiut |
1.1 |
IF(R.LE.RMIN)GOTO30 |
276 |
|
|
RQ=R*R |
277 |
|
|
FF=SQRT(1.+3.*ZQ/RQ) |
278 |
|
|
RADIK=B0-((D2*T+D1)*T+D0)*R*RQ*FF |
279 |
mocchiut |
1.3 |
IF((R-RMAX).le.0.) goto 44 |
280 |
|
|
IF((R-RMAX).gt.0.) goto 45 |
281 |
mocchiut |
1.1 |
45 ICODE=2 |
282 |
|
|
RADIK=RADIK-12.*(R-RMAX)**2 |
283 |
|
|
44 IF(RADIK+RADIK.LE.ORADIK) GOTO 10 |
284 |
|
|
TERM=SQRT(RADIK)*FF*((E2*T+E1)*T+E0)/(RQ+ZQ) |
285 |
|
|
FI=FI+STP*(OTERM+TERM) |
286 |
|
|
ORADIK=RADIK |
287 |
|
|
OTERM=TERM |
288 |
|
|
STP=R*STEQ |
289 |
|
|
Z=Z+STP |
290 |
|
|
GOTO4 |
291 |
|
|
C*****PREDICTOR (FIELD LINE TRACING) |
292 |
|
|
5 P(1,N+1)=P(1,N)+STEP12*(23.*P(4,N)-16.*P(4,N-1)+5.*P(4,N-2)) |
293 |
|
|
P(2,N+1)=P(2,N)+STEP12*(23.*P(5,N)-16.*P(5,N-1)+5.*P(5,N-2)) |
294 |
|
|
P(3,N+1)=P(3,N)+STEP |
295 |
|
|
CALL STOER(P(1,N+1),BQ3,R3) |
296 |
|
|
C*****SEARCH FOR LOWEST MAGNETIC FIELD STRENGTH |
297 |
|
|
IF(BQ3.LT.BEQU) THEN |
298 |
|
|
IEQU=N+1 |
299 |
|
|
BEQU=BQ3 |
300 |
|
|
ENDIF |
301 |
|
|
3 CONTINUE |
302 |
|
|
10 IF(IEQU.lt.2) IEQU=2 |
303 |
|
|
SP(1)=P(1,IEQU-1) |
304 |
|
|
SP(2)=P(2,IEQU-1) |
305 |
|
|
SP(3)=P(3,IEQU-1) |
306 |
|
|
IF(ORADIK.LT.1E-15)GOTO11 |
307 |
|
|
FI=FI+STP/0.75*OTERM*ORADIK/(ORADIK-RADIK) |
308 |
|
|
C |
309 |
|
|
C-- The minimal allowable value of FI was changed from 1E-15 to 1E-12, |
310 |
|
|
C-- because 1E-38 is the minimal allowable arg. for ALOG in our envir. |
311 |
|
|
C-- D. Bilitza, Nov 87. |
312 |
|
|
C |
313 |
mocchiut |
1.4 |
11 FI=0.5*ABS(FI)/SQRT(B0)+1E-12 |
314 |
mocchiut |
1.1 |
C |
315 |
|
|
C*****COMPUTE L FROM B AND I. SAME AS CARMEL IN INVAR. |
316 |
|
|
C |
317 |
|
|
C-- Correct dipole moment is used here. D. Bilitza, Nov 87. |
318 |
|
|
C |
319 |
|
|
DIMOB0=DIMO/B0 |
320 |
mocchiut |
1.9 |
arg1=alog(FI) |
321 |
|
|
arg2=alog(DIMOB0) |
322 |
mocchiut |
1.4 |
c arg = FI*FI*FI/DIMOB0 |
323 |
|
|
c if(abs(arg).gt.88.0) arg=88.0 |
324 |
mocchiut |
1.1 |
XX=3*arg1-arg2 |
325 |
|
|
IF(XX.GT.23.0) GOTO 776 |
326 |
|
|
IF(XX.GT.11.7) GOTO 775 |
327 |
|
|
IF(XX.GT.+3.0) GOTO 774 |
328 |
|
|
IF(XX.GT.-3.0) GOTO 773 |
329 |
|
|
IF(XX.GT.-22.) GOTO 772 |
330 |
mocchiut |
1.3 |
c 771 GG=3.33338E-1*XX+3.0062102E-1 |
331 |
|
|
GG=3.33338E-1*XX+3.0062102E-1 |
332 |
mocchiut |
1.1 |
GOTO777 |
333 |
|
|
772 GG=((((((((-8.1537735E-14*XX+8.3232531E-13)*XX+1.0066362E-9)*XX+ |
334 |
|
|
18.1048663E-8)*XX+3.2916354E-6)*XX+8.2711096E-5)*XX+1.3714667E-3)* |
335 |
|
|
2XX+1.5017245E-2)*XX+4.3432642E-1)*XX+6.2337691E-1 |
336 |
|
|
GOTO777 |
337 |
|
|
773 GG=((((((((2.6047023E-10*XX+2.3028767E-9)*XX-2.1997983E-8)*XX- |
338 |
|
|
15.3977642E-7)*XX-3.3408822E-6)*XX+3.8379917E-5)*XX+1.1784234E-3)* |
339 |
|
|
2XX+1.4492441E-2)*XX+4.3352788E-1)*XX+6.228644E-1 |
340 |
|
|
GOTO777 |
341 |
|
|
774 GG=((((((((6.3271665E-10*XX-3.958306E-8)*XX+9.9766148E-07)*XX- |
342 |
|
|
11.2531932E-5)*XX+7.9451313E-5)*XX-3.2077032E-4)*XX+2.1680398E-3)* |
343 |
|
|
2XX+1.2817956E-2)*XX+4.3510529E-1)*XX+6.222355E-1 |
344 |
|
|
GOTO777 |
345 |
|
|
775 GG=(((((2.8212095E-8*XX-3.8049276E-6)*XX+2.170224E-4)*XX-6.7310339 |
346 |
|
|
1E-3)*XX+1.2038224E-1)*XX-1.8461796E-1)*XX+2.0007187E0 |
347 |
|
|
GOTO777 |
348 |
|
|
776 GG=XX-3.0460681E0 |
349 |
mocchiut |
1.9 |
777 FL=EXP(ALOG((1.+EXP(GG))*DIMOB0)/3.0) |
350 |
mocchiut |
1.1 |
RETURN |
351 |
|
|
C*****APPROXIMATION FOR HIGH VALUES OF L. |
352 |
|
|
30 ICODE=3 |
353 |
|
|
T=-P(3,N-1)/STEP |
354 |
|
|
FL=1./(ABS(((C3*T+C2)*T+C1)*T+C0)+1E-15) |
355 |
|
|
RETURN |
356 |
|
|
END |
357 |
|
|
C |
358 |
|
|
C |
359 |
|
|
SUBROUTINE STOER(P,BQ,R) |
360 |
|
|
C******************************************************************* |
361 |
|
|
C* SUBROUTINE USED FOR FIELD LINE TRACING IN SHELLG * |
362 |
|
|
C* CALLS ENTRY POINT FELDI IN GEOMAGNETIC FIELD SUBROUTINE FELDG * |
363 |
|
|
C******************************************************************* |
364 |
|
|
DIMENSION P(7),U(3,3) |
365 |
mocchiut |
1.6 |
COMMON XI(3),H(196) |
366 |
mocchiut |
1.1 |
C*****XM,YM,ZM ARE GEOMAGNETIC CARTESIAN INVERSE CO-ORDINATES |
367 |
|
|
ZM=P(3) |
368 |
|
|
FLI=P(1)*P(1)+P(2)*P(2)+1E-15 |
369 |
|
|
R=0.5*(FLI+SQRT(FLI*FLI+(ZM+ZM)**2)) |
370 |
|
|
RQ=R*R |
371 |
|
|
WR=SQRT(R) |
372 |
|
|
XM=P(1)*WR |
373 |
|
|
YM=P(2)*WR |
374 |
|
|
C*****TRANSFORM TO GEOGRAPHIC CO-ORDINATE SYSTEM |
375 |
|
|
DATA U/ +0.3511737,-0.9148385,-0.1993679, |
376 |
|
|
A +0.9335804,+0.3583680,+0.0000000, |
377 |
|
|
B +0.0714471,-0.1861260,+0.9799247/ |
378 |
|
|
XI(1)=XM*U(1,1)+YM*U(1,2)+ZM*U(1,3) |
379 |
|
|
XI(2)=XM*U(2,1)+YM*U(2,2)+ZM*U(2,3) |
380 |
|
|
XI(3)=XM*U(3,1) +ZM*U(3,3) |
381 |
|
|
C*****COMPUTE DERIVATIVES |
382 |
|
|
C CALL FELDI(XI,H) |
383 |
|
|
CALL FELDI |
384 |
|
|
Q=H(1)/RQ |
385 |
|
|
DX=H(3)+H(3)+Q*XI(1) |
386 |
|
|
DY=H(4)+H(4)+Q*XI(2) |
387 |
|
|
DZ=H(2)+H(2)+Q*XI(3) |
388 |
|
|
C*****TRANSFORM BACK TO GEOMAGNETIC CO-ORDINATE SYSTEM |
389 |
|
|
DXM=U(1,1)*DX+U(2,1)*DY+U(3,1)*DZ |
390 |
|
|
DYM=U(1,2)*DX+U(2,2)*DY |
391 |
|
|
DZM=U(1,3)*DX+U(2,3)*DY+U(3,3)*DZ |
392 |
|
|
DR=(XM*DXM+YM*DYM+ZM*DZM)/R |
393 |
|
|
C*****FORM SLOWLY VARYING EXPRESSIONS |
394 |
|
|
P(4)=(WR*DXM-0.5*P(1)*DR)/(R*DZM) |
395 |
|
|
P(5)=(WR*DYM-0.5*P(2)*DR)/(R*DZM) |
396 |
|
|
DSQ=RQ*(DXM*DXM+DYM*DYM+DZM*DZM) |
397 |
|
|
BQ=DSQ*RQ*RQ |
398 |
|
|
P(6)=SQRT(DSQ/(RQ+3.*ZM*ZM)) |
399 |
|
|
P(7)=P(6)*(RQ+ZM*ZM)/(RQ*DZM) |
400 |
|
|
RETURN |
401 |
|
|
END |
402 |
|
|
C |
403 |
|
|
C |
404 |
|
|
SUBROUTINE FELDG(GLAT,GLON,ALT,BNORTH,BEAST,BDOWN,BABS) |
405 |
|
|
C------------------------------------------------------------------- |
406 |
|
|
C CALCULATES EARTH MAGNETIC FIELD FROM SPHERICAL HARMONICS MODEL |
407 |
|
|
C REF: G. KLUGE, EUROPEAN SPACE OPERATIONS CENTRE, INTERNAL NOTE 61, |
408 |
|
|
C 1970. |
409 |
|
|
C-------------------------------------------------------------------- |
410 |
|
|
C CHANGES (D. BILITZA, NOV 87): |
411 |
|
|
C - FIELD COEFFICIENTS IN BINARY DATA FILES INSTEAD OF BLOCK DATA |
412 |
|
|
C - CALCULATES DIPOL MOMENT |
413 |
|
|
C-------------------------------------------------------------------- |
414 |
|
|
C INPUT: ENTRY POINT FELDG |
415 |
|
|
C GLAT GEODETIC LATITUDE IN DEGREES (NORTH) |
416 |
|
|
C GLON GEODETIC LONGITUDE IN DEGREES (EAST) |
417 |
|
|
C ALT ALTITUDE IN KM ABOVE SEA LEVEL |
418 |
|
|
C |
419 |
|
|
C ENTRY POINT FELDC |
420 |
|
|
C V(3) CARTESIAN COORDINATES IN EARTH RADII (6371.2 KM) |
421 |
|
|
C X-AXIS POINTING TO EQUATOR AT 0 LONGITUDE |
422 |
|
|
C Y-AXIS POINTING TO EQUATOR AT 90 LONG. |
423 |
|
|
C Z-AXIS POINTING TO NORTH POLE |
424 |
|
|
C |
425 |
|
|
C COMMON BLANK AND ENTRY POINT FELDI ARE NEEDED WHEN USED |
426 |
|
|
C IN CONNECTION WITH L-CALCULATION PROGRAM SHELLG. |
427 |
|
|
C |
428 |
|
|
C COMMON /MODEL/ AND /GENER/ |
429 |
|
|
C UMR = ATAN(1.0)*4./180. <DEGREE>*UMR=<RADIANT> |
430 |
|
|
C ERA EARTH RADIUS FOR NORMALIZATION OF CARTESIAN |
431 |
|
|
C COORDINATES (6371.2 KM) |
432 |
|
|
C AQUAD, BQUAD SQUARE OF MAJOR AND MINOR HALF AXIS FOR |
433 |
|
|
C EARTH ELLIPSOID AS RECOMMENDED BY INTERNATIONAL |
434 |
|
|
C ASTRONOMICAL UNION (6378.160, 6356.775 KM). |
435 |
|
|
C NMAX MAXIMUM ORDER OF SPHERICAL HARMONICS |
436 |
|
|
C TIME YEAR (DECIMAL: 1973.5) FOR WHICH MAGNETIC |
437 |
|
|
C FIELD IS TO BE CALCULATED |
438 |
|
|
C G(M) NORMALIZED FIELD COEFFICIENTS (SEE FELDCOF) |
439 |
|
|
C M=NMAX*(NMAX+2) |
440 |
|
|
C------------------------------------------------------------------------ |
441 |
|
|
C OUTPUT: BABS MAGNETIC FIELD STRENGTH IN GAUSS |
442 |
|
|
C BNORTH, BEAST, BDOWN COMPONENTS OF THE FIELD WITH RESPECT |
443 |
|
|
C TO THE LOCAL GEODETIC COORDINATE SYSTEM, WITH AXIS |
444 |
|
|
C POINTING IN THE TANGENTIAL PLANE TO THE NORTH, EAST |
445 |
|
|
C AND DOWNWARD. |
446 |
|
|
C----------------------------------------------------------------------- |
447 |
mocchiut |
1.6 |
DIMENSION V(3),B(3),G(196) |
448 |
mocchiut |
1.1 |
CHARACTER*258 NAME |
449 |
|
|
INTEGER NMAX |
450 |
|
|
REAL TIME |
451 |
mocchiut |
1.6 |
COMMON XI(3),H(196) |
452 |
mocchiut |
1.1 |
COMMON/MODEL/ G,NMAX,TIME,NAME |
453 |
|
|
SAVE/MODEL/ |
454 |
mocchiut |
1.9 |
COMMON/GENER/ UMR,ERA,AQUAD,BQUAD |
455 |
mocchiut |
1.1 |
SAVE/GENER/ |
456 |
|
|
C |
457 |
|
|
C-- IS RECORDS ENTRY POINT |
458 |
|
|
C |
459 |
|
|
C*****ENTRY POINT FELDG TO BE USED WITH GEODETIC CO-ORDINATES |
460 |
|
|
IS=1 |
461 |
|
|
RLAT=GLAT*UMR |
462 |
|
|
CT=SIN(RLAT) |
463 |
|
|
ST=COS(RLAT) |
464 |
|
|
D=SQRT(AQUAD-(AQUAD-BQUAD)*CT*CT) |
465 |
|
|
RLON=GLON*UMR |
466 |
|
|
CP=COS(RLON) |
467 |
|
|
SP=SIN(RLON) |
468 |
|
|
ZZZ=(ALT+BQUAD/D)*CT/ERA |
469 |
|
|
RHO=(ALT+AQUAD/D)*ST/ERA |
470 |
|
|
XXX=RHO*CP |
471 |
|
|
YYY=RHO*SP |
472 |
|
|
GOTO10 |
473 |
|
|
ENTRY FELDC(V,B) |
474 |
|
|
C*****ENTRY POINT FELDC TO BE USED WITH CARTESIAN CO-ORDINATES |
475 |
|
|
IS=2 |
476 |
|
|
XXX=V(1) |
477 |
|
|
YYY=V(2) |
478 |
|
|
ZZZ=V(3) |
479 |
|
|
10 RQ=1./(XXX*XXX+YYY*YYY+ZZZ*ZZZ) |
480 |
|
|
XI(1)=XXX*RQ |
481 |
|
|
XI(2)=YYY*RQ |
482 |
|
|
XI(3)=ZZZ*RQ |
483 |
|
|
GOTO20 |
484 |
|
|
ENTRY FELDI |
485 |
|
|
C*****ENTRY POINT FELDI USED FOR L COMPUTATION |
486 |
|
|
IS=3 |
487 |
|
|
20 IHMAX=NMAX*NMAX+1 |
488 |
|
|
LAST=IHMAX+NMAX+NMAX |
489 |
|
|
IMAX=NMAX+NMAX-1 |
490 |
|
|
DO 8 I=IHMAX,LAST |
491 |
|
|
8 H(I)=G(I) |
492 |
|
|
DO 6 K=1,3,2 |
493 |
|
|
I=IMAX |
494 |
|
|
IH=IHMAX |
495 |
|
|
1 IL=IH-I |
496 |
|
|
F=2./FLOAT(I-K+2) |
497 |
|
|
X=XI(1)*F |
498 |
|
|
Y=XI(2)*F |
499 |
|
|
Z=XI(3)*(F+F) |
500 |
|
|
I=I-2 |
501 |
mocchiut |
1.3 |
c print *,' I ',I |
502 |
|
|
IF((I-1).lt.0) goto 5 |
503 |
|
|
IF((I-1).eq.0) goto 4 |
504 |
|
|
IF((I-1).gt.0) goto 2 |
505 |
mocchiut |
1.1 |
2 DO 3 M=3,I,2 |
506 |
|
|
H(IL+M+1)=G(IL+M+1)+Z*H(IH+M+1)+X*(H(IH+M+3)-H(IH+M-1)) |
507 |
|
|
A -Y*(H(IH+M+2)+H(IH+M-2)) |
508 |
|
|
3 H(IL+M)=G(IL+M)+Z*H(IH+M)+X*(H(IH+M+2)-H(IH+M-2)) |
509 |
|
|
A +Y*(H(IH+M+3)+H(IH+M-1)) |
510 |
|
|
4 H(IL+2)=G(IL+2)+Z*H(IH+2)+X*H(IH+4)-Y*(H(IH+3)+H(IH)) |
511 |
|
|
H(IL+1)=G(IL+1)+Z*H(IH+1)+Y*H(IH+4)+X*(H(IH+3)-H(IH)) |
512 |
|
|
5 H(IL)=G(IL)+Z*H(IH)+2.*(X*H(IH+1)+Y*H(IH+2)) |
513 |
|
|
IH=IL |
514 |
|
|
IF(I.GE.K)GOTO1 |
515 |
|
|
6 CONTINUE |
516 |
|
|
IF(IS.EQ.3)RETURN |
517 |
|
|
S=.5*H(1)+2.*(H(2)*XI(3)+H(3)*XI(1)+H(4)*XI(2)) |
518 |
|
|
T=(RQ+RQ)*SQRT(RQ) |
519 |
|
|
BXXX=T*(H(3)-S*XXX) |
520 |
|
|
BYYY=T*(H(4)-S*YYY) |
521 |
|
|
BZZZ=T*(H(2)-S*ZZZ) |
522 |
|
|
IF(IS.EQ.2)GOTO7 |
523 |
|
|
BABS=SQRT(BXXX*BXXX+BYYY*BYYY+BZZZ*BZZZ) |
524 |
|
|
BEAST=BYYY*CP-BXXX*SP |
525 |
|
|
BRHO=BYYY*SP+BXXX*CP |
526 |
|
|
BNORTH=BZZZ*ST-BRHO*CT |
527 |
|
|
BDOWN=-BZZZ*CT-BRHO*ST |
528 |
|
|
RETURN |
529 |
|
|
7 B(1)=BXXX |
530 |
|
|
B(2)=BYYY |
531 |
|
|
B(3)=BZZZ |
532 |
|
|
RETURN |
533 |
|
|
END |
534 |
|
|
C |
535 |
|
|
C |
536 |
mocchiut |
1.3 |
SUBROUTINE FELDCOF(YEAR,DIMO) |
537 |
mocchiut |
1.1 |
C------------------------------------------------------------------------ |
538 |
mocchiut |
1.3 |
C DETERMINES COEFFICIENTS AND DIPOL MOMENT FROM IGRF MODELS |
539 |
|
|
C |
540 |
|
|
C INPUT: YEAR DECIMAL YEAR FOR WHICH GEOMAGNETIC FIELD IS TO |
541 |
|
|
C BE CALCULATED |
542 |
|
|
C OUTPUT: DIMO GEOMAGNETIC DIPOL MOMENT IN GAUSS (NORMALIZED |
543 |
|
|
C TO EARTH'S RADIUS) AT THE TIME (YEAR) |
544 |
|
|
C D. BILITZA, NSSDC, GSFC, CODE 633, GREENBELT, MD 20771, |
545 |
|
|
C (301)286-9536 NOV 1987. |
546 |
|
|
C ### updated to IGRF-2000 version -dkb- 5/31/2000 |
547 |
|
|
C ### updated to IGRF-2005 version -dkb- 3/24/2000 |
548 |
mocchiut |
1.1 |
C----------------------------------------------------------------------- |
549 |
mocchiut |
1.3 |
CHARACTER*258 FIL1, FIL2 |
550 |
|
|
CHARACTER*258 FILMOD |
551 |
mocchiut |
1.12 |
DIMENSION GH1(196),GH2(196),GHA(196),FILMOD(2) |
552 |
mocchiut |
1.3 |
DOUBLE PRECISION X,F0,F |
553 |
mocchiut |
1.12 |
INTEGER L1,L2,I1 |
554 |
mocchiut |
1.3 |
INTEGER NMAX |
555 |
|
|
REAL TIME |
556 |
mocchiut |
1.12 |
CHARACTER *258 P1,P2 |
557 |
|
|
COMMON/PPATH/ I1,L1,L2,P1,P2 |
558 |
mocchiut |
1.3 |
SAVE/PPATH/ |
559 |
|
|
COMMON/MODEL/ GH1,NMAX,TIME,FIL1 |
560 |
|
|
SAVE/MODEL/ |
561 |
mocchiut |
1.9 |
COMMON/GENER/ UMR,ERAD,AQUAD,BQUAD |
562 |
mocchiut |
1.3 |
SAVE/GENER/ |
563 |
mocchiut |
1.7 |
c print *, "qui" |
564 |
mocchiut |
1.1 |
FILMOD(1) = P1(1:L1) |
565 |
|
|
FILMOD(2) = P2(1:L2) |
566 |
mocchiut |
1.7 |
c print *, "qua" |
567 |
mocchiut |
1.3 |
C |
568 |
|
|
C IS=0 FOR SCHMIDT NORMALIZATION IS=1 GAUSS NORMALIZATION |
569 |
|
|
C IU IS INPUT UNIT NUMBER FOR IGRF COEFFICIENT SETS |
570 |
|
|
C |
571 |
|
|
IU = 10 |
572 |
|
|
IS = 0 |
573 |
|
|
C-- DETERMINE IGRF-YEARS FOR INPUT-YEAR |
574 |
|
|
TIME = YEAR |
575 |
|
|
IYEA = INT(YEAR/5.)*5 |
576 |
mocchiut |
1.12 |
L = IYEA + 5 |
577 |
|
|
C |
578 |
|
|
DTE1 = REAL(IYEA) |
579 |
|
|
FIL1 = FILMOD(1) |
580 |
|
|
DTE2 = REAL(L) |
581 |
|
|
FIL2 = FILMOD(2) |
582 |
|
|
c print *,'IYEA ',IYEA,' L ',L |
583 |
mocchiut |
1.7 |
c WRITE(*,*) FIL1 |
584 |
|
|
c WRITE(*,*) FIL2 |
585 |
|
|
c print *, "que" |
586 |
mocchiut |
1.3 |
C-- GET IGRF COEFFICIENTS FOR THE BOUNDARY YEARS |
587 |
|
|
CALL GETSHC (IU, FIL1, NMAX1, ERAD, GH1, IER) |
588 |
|
|
IF (IER .NE. 0) STOP |
589 |
mocchiut |
1.7 |
c print *, "quessss" |
590 |
mocchiut |
1.3 |
CALL GETSHC (IU, FIL2, NMAX2, ERAD, GH2, IER) |
591 |
|
|
IF (IER .NE. 0) STOP |
592 |
mocchiut |
1.7 |
c print *, "quj" |
593 |
mocchiut |
1.3 |
C-- DETERMINE IGRF COEFFICIENTS FOR YEAR |
594 |
mocchiut |
1.12 |
IF (I1.EQ.0) THEN |
595 |
mocchiut |
1.3 |
CALL INTERSHC (YEAR, DTE1, NMAX1, GH1, DTE2, |
596 |
|
|
1 NMAX2, GH2, NMAX, GHA) |
597 |
|
|
ELSE |
598 |
|
|
CALL EXTRASHC (YEAR, DTE1, NMAX1, GH1, NMAX2, |
599 |
|
|
1 GH2, NMAX, GHA) |
600 |
|
|
ENDIF |
601 |
mocchiut |
1.7 |
c print *, "quw" |
602 |
mocchiut |
1.3 |
C-- DETERMINE MAGNETIC DIPOL MOMENT AND COEFFIECIENTS G |
603 |
|
|
F0=0.D0 |
604 |
|
|
DO 1234 J=1,3 |
605 |
|
|
F = GHA(J) * 1.D-5 |
606 |
|
|
F0 = F0 + F * F |
607 |
|
|
1234 CONTINUE |
608 |
mocchiut |
1.9 |
DIMO = REAL(DSQRT(F0)) |
609 |
mocchiut |
1.3 |
|
610 |
|
|
GH1(1) = 0.0 |
611 |
|
|
I=2 |
612 |
|
|
F0=1.D-5 |
613 |
|
|
IF(IS.EQ.0) F0=-F0 |
614 |
|
|
SQRT2=SQRT(2.) |
615 |
mocchiut |
1.1 |
|
616 |
mocchiut |
1.3 |
c print *, "quq" |
617 |
|
|
|
618 |
mocchiut |
1.1 |
DO 9 N=1,NMAX |
619 |
mocchiut |
1.3 |
X = N |
620 |
|
|
F0 = F0 * X * X / (4.D0 * X - 2.D0) |
621 |
|
|
IF(IS.EQ.0) F0 = F0 * (2.D0 * X - 1.D0) / X |
622 |
|
|
F = F0 * 0.5D0 |
623 |
|
|
IF(IS.EQ.0) F = F * SQRT2 |
624 |
mocchiut |
1.9 |
GH1(I) = GHA(I-1) * REAL(F0) |
625 |
mocchiut |
1.3 |
I = I+1 |
626 |
|
|
DO 9 M=1,N |
627 |
|
|
F = F * (X + M) / (X - M + 1.D0) |
628 |
|
|
IF(IS.EQ.0) F = F * DSQRT((X - M + 1.D0) / (X + M)) |
629 |
mocchiut |
1.9 |
GH1(I) = GHA(I-1) * REAL(F) |
630 |
|
|
GH1(I+1) = GHA(I) * REAL(F) |
631 |
mocchiut |
1.3 |
I=I+2 |
632 |
|
|
9 CONTINUE |
633 |
|
|
RETURN |
634 |
|
|
END |
635 |
|
|
C |
636 |
|
|
C |
637 |
|
|
SUBROUTINE GETSHC (IU, FSPEC, NMAX, ERAD, GH, IER) |
638 |
mocchiut |
1.9 |
|
639 |
mocchiut |
1.1 |
C =============================================================== |
640 |
|
|
C |
641 |
mocchiut |
1.3 |
C Version 1.01 |
642 |
|
|
C |
643 |
|
|
C Reads spherical harmonic coefficients from the specified |
644 |
|
|
C file into an array. |
645 |
|
|
C |
646 |
|
|
C Input: |
647 |
|
|
C IU - Logical unit number |
648 |
|
|
C FSPEC - File specification |
649 |
|
|
C |
650 |
|
|
C Output: |
651 |
|
|
C NMAX - Maximum degree and order of model |
652 |
|
|
C ERAD - Earth's radius associated with the spherical |
653 |
|
|
C harmonic coefficients, in the same units as |
654 |
|
|
C elevation |
655 |
|
|
C GH - Schmidt quasi-normal internal spherical |
656 |
|
|
C harmonic coefficients |
657 |
|
|
C IER - Error number: = 0, no error |
658 |
|
|
C = -2, records out of order |
659 |
|
|
C = FORTRAN run-time error number |
660 |
|
|
C |
661 |
|
|
C A. Zunde |
662 |
|
|
C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225 |
663 |
|
|
C |
664 |
|
|
C =============================================================== |
665 |
|
|
|
666 |
|
|
CHARACTER FSPEC*(*), FOUT*258 |
667 |
|
|
DIMENSION GH(*) |
668 |
|
|
C --------------------------------------------------------------- |
669 |
|
|
C Open coefficient file. Read past first header record. |
670 |
|
|
C Read degree and order of model and Earth's radius. |
671 |
|
|
C --------------------------------------------------------------- |
672 |
mocchiut |
1.1 |
WRITE(FOUT,667) FSPEC |
673 |
mocchiut |
1.3 |
c 667 FORMAT('/usr/local/etc/httpd/cgi-bin/natasha/IRI/',A12) |
674 |
|
|
667 FORMAT(A258) |
675 |
mocchiut |
1.7 |
c print *," gui" |
676 |
mocchiut |
1.1 |
OPEN (IU, FILE=FOUT, STATUS='OLD', IOSTAT=IER, ERR=999) |
677 |
mocchiut |
1.7 |
c print *," gua" |
678 |
mocchiut |
1.1 |
READ (IU, *, IOSTAT=IER, ERR=999) |
679 |
mocchiut |
1.7 |
c print *," gue" |
680 |
mocchiut |
1.1 |
READ (IU, *, IOSTAT=IER, ERR=999) NMAX, ERAD |
681 |
mocchiut |
1.7 |
c print *," guo" |
682 |
mocchiut |
1.1 |
C --------------------------------------------------------------- |
683 |
|
|
C Read the coefficient file, arranged as follows: |
684 |
|
|
C |
685 |
|
|
C N M G H |
686 |
|
|
C ---------------------- |
687 |
|
|
C / 1 0 GH(1) - |
688 |
|
|
C / 1 1 GH(2) GH(3) |
689 |
|
|
C / 2 0 GH(4) - |
690 |
|
|
C / 2 1 GH(5) GH(6) |
691 |
|
|
C NMAX*(NMAX+3)/2 / 2 2 GH(7) GH(8) |
692 |
|
|
C records \ 3 0 GH(9) - |
693 |
|
|
C \ . . . . |
694 |
|
|
C \ . . . . |
695 |
|
|
C NMAX*(NMAX+2) \ . . . . |
696 |
|
|
C elements in GH \ NMAX NMAX . . |
697 |
|
|
C |
698 |
|
|
C N and M are, respectively, the degree and order of the |
699 |
|
|
C coefficient. |
700 |
|
|
C --------------------------------------------------------------- |
701 |
|
|
|
702 |
|
|
I = 0 |
703 |
mocchiut |
1.3 |
DO 2211 NN = 1, NMAX |
704 |
|
|
DO 2233 MM = 0, NN |
705 |
mocchiut |
1.1 |
READ (IU, *, IOSTAT=IER, ERR=999) N, M, G, H |
706 |
|
|
IF (NN .NE. N .OR. MM .NE. M) THEN |
707 |
|
|
IER = -2 |
708 |
|
|
GOTO 999 |
709 |
|
|
ENDIF |
710 |
|
|
I = I + 1 |
711 |
|
|
GH(I) = G |
712 |
|
|
IF (M .NE. 0) THEN |
713 |
|
|
I = I + 1 |
714 |
|
|
GH(I) = H |
715 |
|
|
ENDIF |
716 |
|
|
2233 CONTINUE |
717 |
|
|
2211 CONTINUE |
718 |
mocchiut |
1.7 |
c print *," guj" |
719 |
mocchiut |
1.1 |
|
720 |
|
|
999 CLOSE (IU) |
721 |
mocchiut |
1.7 |
c print *," guw IER",IER |
722 |
mocchiut |
1.3 |
if ( IER .eq. -1 ) IER = 0 ! gfortran 4.1.2 bug workaround... hoping not to create problems with other versions |
723 |
mocchiut |
1.1 |
|
724 |
|
|
RETURN |
725 |
|
|
END |
726 |
|
|
C |
727 |
|
|
C |
728 |
|
|
SUBROUTINE INTERSHC (DATE, DTE1, NMAX1, GH1, DTE2, |
729 |
|
|
1 NMAX2, GH2, NMAX, GH) |
730 |
mocchiut |
1.9 |
|
731 |
mocchiut |
1.1 |
C =============================================================== |
732 |
|
|
C |
733 |
|
|
C Version 1.01 |
734 |
|
|
C |
735 |
|
|
C Interpolates linearly, in time, between two spherical |
736 |
|
|
C harmonic models. |
737 |
|
|
C |
738 |
|
|
C Input: |
739 |
|
|
C DATE - Date of resulting model (in decimal year) |
740 |
|
|
C DTE1 - Date of earlier model |
741 |
|
|
C NMAX1 - Maximum degree and order of earlier model |
742 |
|
|
C GH1 - Schmidt quasi-normal internal spherical |
743 |
|
|
C harmonic coefficients of earlier model |
744 |
|
|
C DTE2 - Date of later model |
745 |
|
|
C NMAX2 - Maximum degree and order of later model |
746 |
|
|
C GH2 - Schmidt quasi-normal internal spherical |
747 |
|
|
C harmonic coefficients of later model |
748 |
|
|
C |
749 |
|
|
C Output: |
750 |
|
|
C GH - Coefficients of resulting model |
751 |
|
|
C NMAX - Maximum degree and order of resulting model |
752 |
|
|
C |
753 |
|
|
C A. Zunde |
754 |
|
|
C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225 |
755 |
|
|
C |
756 |
|
|
C =============================================================== |
757 |
|
|
|
758 |
|
|
DIMENSION GH1(*), GH2(*), GH(*) |
759 |
|
|
|
760 |
|
|
C --------------------------------------------------------------- |
761 |
|
|
C The coefficients (GH) of the resulting model, at date |
762 |
|
|
C DATE, are computed by linearly interpolating between the |
763 |
|
|
C coefficients of the earlier model (GH1), at date DTE1, |
764 |
|
|
C and those of the later model (GH2), at date DTE2. If one |
765 |
|
|
C model is smaller than the other, the interpolation is |
766 |
|
|
C performed with the missing coefficients assumed to be 0. |
767 |
|
|
C --------------------------------------------------------------- |
768 |
|
|
|
769 |
|
|
FACTOR = (DATE - DTE1) / (DTE2 - DTE1) |
770 |
|
|
|
771 |
|
|
IF (NMAX1 .EQ. NMAX2) THEN |
772 |
|
|
K = NMAX1 * (NMAX1 + 2) |
773 |
|
|
NMAX = NMAX1 |
774 |
|
|
ELSE IF (NMAX1 .GT. NMAX2) THEN |
775 |
|
|
K = NMAX2 * (NMAX2 + 2) |
776 |
|
|
L = NMAX1 * (NMAX1 + 2) |
777 |
mocchiut |
1.3 |
DO 1122 I = K + 1, L |
778 |
mocchiut |
1.1 |
1122 GH(I) = GH1(I) + FACTOR * (-GH1(I)) |
779 |
|
|
NMAX = NMAX1 |
780 |
|
|
ELSE |
781 |
|
|
K = NMAX1 * (NMAX1 + 2) |
782 |
|
|
L = NMAX2 * (NMAX2 + 2) |
783 |
mocchiut |
1.3 |
DO 1133 I = K + 1, L |
784 |
mocchiut |
1.1 |
1133 GH(I) = FACTOR * GH2(I) |
785 |
|
|
NMAX = NMAX2 |
786 |
|
|
ENDIF |
787 |
|
|
|
788 |
mocchiut |
1.3 |
DO 1144 I = 1, K |
789 |
mocchiut |
1.1 |
1144 GH(I) = GH1(I) + FACTOR * (GH2(I) - GH1(I)) |
790 |
|
|
|
791 |
|
|
RETURN |
792 |
|
|
END |
793 |
|
|
C |
794 |
|
|
C |
795 |
|
|
SUBROUTINE EXTRASHC (DATE, DTE1, NMAX1, GH1, NMAX2, |
796 |
|
|
1 GH2, NMAX, GH) |
797 |
|
|
|
798 |
|
|
C =============================================================== |
799 |
|
|
C |
800 |
|
|
C Version 1.01 |
801 |
|
|
C |
802 |
|
|
C Extrapolates linearly a spherical harmonic model with a |
803 |
|
|
C rate-of-change model. |
804 |
|
|
C |
805 |
|
|
C Input: |
806 |
|
|
C DATE - Date of resulting model (in decimal year) |
807 |
|
|
C DTE1 - Date of base model |
808 |
|
|
C NMAX1 - Maximum degree and order of base model |
809 |
|
|
C GH1 - Schmidt quasi-normal internal spherical |
810 |
|
|
C harmonic coefficients of base model |
811 |
|
|
C NMAX2 - Maximum degree and order of rate-of-change |
812 |
|
|
C model |
813 |
|
|
C GH2 - Schmidt quasi-normal internal spherical |
814 |
|
|
C harmonic coefficients of rate-of-change model |
815 |
|
|
C |
816 |
|
|
C Output: |
817 |
|
|
C GH - Coefficients of resulting model |
818 |
|
|
C NMAX - Maximum degree and order of resulting model |
819 |
|
|
C |
820 |
|
|
C A. Zunde |
821 |
|
|
C USGS, MS 964, Box 25046 Federal Center, Denver, CO 80225 |
822 |
|
|
C |
823 |
|
|
C =============================================================== |
824 |
|
|
|
825 |
|
|
DIMENSION GH1(*), GH2(*), GH(*) |
826 |
|
|
|
827 |
|
|
C --------------------------------------------------------------- |
828 |
|
|
C The coefficients (GH) of the resulting model, at date |
829 |
|
|
C DATE, are computed by linearly extrapolating the coef- |
830 |
|
|
C ficients of the base model (GH1), at date DTE1, using |
831 |
|
|
C those of the rate-of-change model (GH2), at date DTE2. If |
832 |
|
|
C one model is smaller than the other, the extrapolation is |
833 |
|
|
C performed with the missing coefficients assumed to be 0. |
834 |
|
|
C --------------------------------------------------------------- |
835 |
|
|
|
836 |
|
|
FACTOR = (DATE - DTE1) |
837 |
|
|
|
838 |
|
|
IF (NMAX1 .EQ. NMAX2) THEN |
839 |
|
|
K = NMAX1 * (NMAX1 + 2) |
840 |
|
|
NMAX = NMAX1 |
841 |
|
|
ELSE IF (NMAX1 .GT. NMAX2) THEN |
842 |
|
|
K = NMAX2 * (NMAX2 + 2) |
843 |
|
|
L = NMAX1 * (NMAX1 + 2) |
844 |
mocchiut |
1.3 |
DO 1155 I = K + 1, L |
845 |
mocchiut |
1.1 |
1155 GH(I) = GH1(I) |
846 |
|
|
NMAX = NMAX1 |
847 |
|
|
ELSE |
848 |
|
|
K = NMAX1 * (NMAX1 + 2) |
849 |
|
|
L = NMAX2 * (NMAX2 + 2) |
850 |
mocchiut |
1.3 |
DO 1166 I = K + 1, L |
851 |
mocchiut |
1.1 |
1166 GH(I) = FACTOR * GH2(I) |
852 |
|
|
NMAX = NMAX2 |
853 |
|
|
ENDIF |
854 |
|
|
|
855 |
mocchiut |
1.3 |
DO 1177 I = 1, K |
856 |
mocchiut |
1.1 |
1177 GH(I) = GH1(I) + FACTOR * GH2(I) |
857 |
|
|
|
858 |
|
|
RETURN |
859 |
|
|
END |
860 |
|
|
C |
861 |
|
|
C |
862 |
mocchiut |
1.12 |
SUBROUTINE INITIZE(ISSEC,TP1,TL1,TP2,TL2) |
863 |
mocchiut |
1.1 |
C---------------------------------------------------------------- |
864 |
|
|
C Initializes the parameters in COMMON/GENER/ |
865 |
|
|
C |
866 |
|
|
C UMR = ATAN(1.0)*4./180. <DEGREE>*UMR=<RADIANT> |
867 |
|
|
C ERA EARTH RADIUS FOR NORMALIZATION OF CARTESIAN |
868 |
|
|
C COORDINATES (6371.2 KM) |
869 |
|
|
C EREQU MAJOR HALF AXIS FOR EARTH ELLIPSOID (6378.160 KM) |
870 |
|
|
C ERPOL MINOR HALF AXIS FOR EARTH ELLIPSOID (6356.775 KM) |
871 |
|
|
C AQUAD SQUARE OF MAJOR HALF AXIS FOR EARTH ELLIPSOID |
872 |
|
|
C BQUAD SQUARE OF MINOR HALF AXIS FOR EARTH ELLIPSOID |
873 |
|
|
C |
874 |
|
|
C ERA, EREQU and ERPOL as recommended by the INTERNATIONAL |
875 |
|
|
C ASTRONOMICAL UNION . |
876 |
|
|
C----------------------------------------------------------------- |
877 |
mocchiut |
1.12 |
INTEGER TL1,TL2,ISSEC |
878 |
|
|
CHARACTER (len=*) :: TP1,TP2 |
879 |
|
|
INTEGER L1,L2 |
880 |
|
|
CHARACTER *258 P1,P2 |
881 |
|
|
COMMON/PPATH/ I1,L1,L2,P1,P2 |
882 |
mocchiut |
1.1 |
SAVE/PPATH/ |
883 |
|
|
|
884 |
mocchiut |
1.9 |
COMMON/GENER/UMR,ERA,AQUAD,BQUAD |
885 |
mocchiut |
1.1 |
SAVE/GENER/ |
886 |
|
|
|
887 |
mocchiut |
1.12 |
I1 = ISSEC |
888 |
mocchiut |
1.1 |
L1 = TL1 |
889 |
|
|
L2 = TL2 |
890 |
mocchiut |
1.12 |
|
891 |
mocchiut |
1.2 |
P1 = TP1(1:L1) |
892 |
|
|
P2 = TP2(1:L2) |
893 |
mocchiut |
1.1 |
|
894 |
|
|
ERA=6371.2 |
895 |
|
|
EREQU=6378.16 |
896 |
|
|
ERPOL=6356.775 |
897 |
|
|
AQUAD=EREQU*EREQU |
898 |
|
|
BQUAD=ERPOL*ERPOL |
899 |
|
|
UMR=ATAN(1.0)*4./180. |
900 |
|
|
RETURN |
901 |
|
|
END |