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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-03-04 21:21:30 -0500 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-03-04 21:21:30 -0500 |
commit | d54fe7c1f704a63824c5bfa0ece65245572e9b27 (patch) | |
tree | afc52015ffc2c74e0266653eecef1c8ef8ba5d91 /src/slalib/refz.f | |
download | calfuse-d54fe7c1f704a63824c5bfa0ece65245572e9b27.tar.gz |
Initial commit
Diffstat (limited to 'src/slalib/refz.f')
-rw-r--r-- | src/slalib/refz.f | 139 |
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diff --git a/src/slalib/refz.f b/src/slalib/refz.f new file mode 100644 index 0000000..d558c87 --- /dev/null +++ b/src/slalib/refz.f @@ -0,0 +1,139 @@ + SUBROUTINE sla_REFZ (ZU, REFA, REFB, ZR) +*+ +* - - - - - +* R E F Z +* - - - - - +* +* Adjust an unrefracted zenith distance to include the effect of +* atmospheric refraction, using the simple A tan Z + B tan**3 Z +* model (plus special handling for large ZDs). +* +* Given: +* ZU dp unrefracted zenith distance of the source (radian) +* REFA dp tan Z coefficient (radian) +* REFB dp tan**3 Z coefficient (radian) +* +* Returned: +* ZR dp refracted zenith distance (radian) +* +* Notes: +* +* 1 This routine applies the adjustment for refraction in the +* opposite sense to the usual one - it takes an unrefracted +* (in vacuo) position and produces an observed (refracted) +* position, whereas the A tan Z + B tan**3 Z model strictly +* applies to the case where an observed position is to have the +* refraction removed. The unrefracted to refracted case is +* harder, and requires an inverted form of the text-book +* refraction models; the formula used here is based on the +* Newton-Raphson method. For the utmost numerical consistency +* with the refracted to unrefracted model, two iterations are +* carried out, achieving agreement at the 1D-11 arcseconds level +* for a ZD of 80 degrees. The inherent accuracy of the model +* is, of course, far worse than this - see the documentation for +* sla_REFCO for more information. +* +* 2 At ZD 83 degrees, the rapidly-worsening A tan Z + B tan**3 Z +* model is abandoned and an empirical formula takes over. Over a +* wide range of observer heights and corresponding temperatures and +* pressures, the following levels of accuracy (arcsec) are +* typically achieved, relative to numerical integration through a +* model atmosphere: +* +* ZR error +* +* 80 0.4 +* 81 0.8 +* 82 1.5 +* 83 3.2 +* 84 4.9 +* 85 5.8 +* 86 6.1 +* 87 7.1 +* 88 10 +* 89 20 +* 90 40 +* 91 100 } relevant only to +* 92 200 } high-elevation sites +* +* The high-ZD model is scaled to match the normal model at the +* transition point; there is no glitch. +* +* 3 Beyond 93 deg zenith distance, the refraction is held at its +* 93 deg value. +* +* 4 See also the routine sla_REFV, which performs the adjustment in +* Cartesian Az/El coordinates, and with the emphasis on speed +* rather than numerical accuracy. +* +* P.T.Wallace Starlink 19 September 1995 +* +* Copyright (C) 1995 Rutherford Appleton Laboratory +*- + + IMPLICIT NONE + + DOUBLE PRECISION ZU,REFA,REFB,ZR + +* Radians to degrees + DOUBLE PRECISION R2D + PARAMETER (R2D=57.29577951308232D0) + +* Largest usable ZD (deg) + DOUBLE PRECISION D93 + PARAMETER (D93=93D0) + +* Coefficients for high ZD model (used beyond ZD 83 deg) + DOUBLE PRECISION C1,C2,C3,C4,C5 + PARAMETER (C1=+0.55445D0, + : C2=-0.01133D0, + : C3=+0.00202D0, + : C4=+0.28385D0, + : C5=+0.02390D0) + +* ZD at which one model hands over to the other (radians) + DOUBLE PRECISION Z83 + PARAMETER (Z83=83D0/R2D) + +* High-ZD-model prediction (deg) for that point + DOUBLE PRECISION REF83 + PARAMETER (REF83=(C1+C2*7D0+C3*49D0)/(1D0+C4*7D0+C5*49D0)) + + DOUBLE PRECISION ZU1,ZL,S,C,T,TSQ,TCU,REF,E,E2 + + + +* Perform calculations for ZU or 83 deg, whichever is smaller + ZU1 = MIN(ZU,Z83) + +* Functions of ZD + ZL = ZU1 + S = SIN(ZL) + C = COS(ZL) + T = S/C + TSQ = T*T + TCU = T*TSQ + +* Refracted ZD (mathematically to better than 1 mas at 70 deg) + ZL = ZL-(REFA*T+REFB*TCU)/(1D0+(REFA+3D0*REFB*TSQ)/(C*C)) + +* Further iteration + S = SIN(ZL) + C = COS(ZL) + T = S/C + TSQ = T*T + TCU = T*TSQ + REF = ZU1-ZL+ + : (ZL-ZU1+REFA*T+REFB*TCU)/(1D0+(REFA+3D0*REFB*TSQ)/(C*C)) + +* Special handling for large ZU + IF (ZU.GT.ZU1) THEN + E = 90D0-MIN(D93,ZU*R2D) + E2 = E*E + REF = (REF/REF83)*(C1+C2*E+C3*E2)/(1D0+C4*E+C5*E2) + END IF + +* Return refracted ZD + ZR = ZU-REF + + END |