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