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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /math/slalib/doc/refro.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
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diff --git a/math/slalib/doc/refro.hlp b/math/slalib/doc/refro.hlp new file mode 100644 index 00000000..8b66c95d --- /dev/null +++ b/math/slalib/doc/refro.hlp @@ -0,0 +1,123 @@ +.help refro Jun99 "Slalib Package" +.nf + + SUBROUTINE slRFRO (ZOBS, HM, TDK, PMB, RH, WL, PHI, TLR, + : EPS, REF) + + - - - - - - + R F R O + - - - - - - + + Atmospheric refraction for radio and optical/IR wavelengths. + + Given: + ZOBS d observed zenith distance of the source (radian) + HM d height of the observer above sea level (metre) + TDK d ambient temperature at the observer (deg K) + PMB d pressure at the observer (millibar) + RH d relative humidity at the observer (range 0-1) + WL d effective wavelength of the source (micrometre) + PHI d latitude of the observer (radian, astronomical) + TLR d temperature lapse rate in the troposphere (degK/metre) + EPS d precision required to terminate iteration (radian) + + Returned: + REF d refraction: in vacuo ZD minus observed ZD (radian) + + Notes: + + 1 A suggested value for the TLR argument is 0.0065D0. The + refraction is significantly affected by TLR, and if studies + of the local atmosphere have been carried out a better TLR + value may be available. + + 2 A suggested value for the EPS argument is 1D-8. The result is + usually at least two orders of magnitude more computationally + precise than the supplied EPS value. + + 3 The routine computes the refraction for zenith distances up + to and a little beyond 90 deg using the method of Hohenkerk + and Sinclair (NAO Technical Notes 59 and 63, subsequently adopted + in the Explanatory Supplement, 1992 edition - see section 3.281). + + 4 The code is a development of the optical/IR refraction subroutine + AREF of C.Hohenkerk (HMNAO, September 1984), with extensions to + support the radio case. Apart from merely cosmetic changes, the + following modifications to the original HMNAO optical/IR refraction + code have been made: + + . The angle arguments have been changed to radians. + + . Any value of ZOBS is allowed (see note 6, below). + + . Other argument values have been limited to safe values. + + . Murray's values for the gas constants have been used + (Vectorial Astrometry, Adam Hilger, 1983). + + . The numerical integration phase has been rearranged for + extra clarity. + + . A better model for Ps(T) has been adopted (taken from + Gill, Atmosphere-Ocean Dynamics, Academic Press, 1982). + + . More accurate expressions for Pwo have been adopted + (again from Gill 1982). + + . Provision for radio wavelengths has been added using + expressions devised by A.T.Sinclair, RGO (private + communication 1989), based on the Essen & Froome + refractivity formula adopted in Resolution 1 of the + 13th International Geodesy Association General Assembly + (Bulletin Geodesique 70 p390, 1963). + + . Various small changes have been made to gain speed. + + None of the changes significantly affects the optical/IR results + with respect to the algorithm given in the 1992 Explanatory + Supplement. For example, at 70 deg zenith distance the present + routine agrees with the ES algorithm to better than 0.05 arcsec + for any reasonable combination of parameters. However, the + improved water-vapour expressions do make a significant difference + in the radio band, at 70 deg zenith distance reaching almost + 4 arcsec for a hot, humid, low-altitude site during a period of + low pressure. + + 5 The radio refraction is chosen by specifying WL > 100 micrometres. + Because the algorithm takes no account of the ionosphere, the + accuracy deteriorates at low frequencies, below about 30 MHz. + + 6 Before use, the value of ZOBS is expressed in the range +/- pi. + If this ranged ZOBS is -ve, the result REF is computed from its + absolute value before being made -ve to match. In addition, if + it has an absolute value greater than 93 deg, a fixed REF value + equal to the result for ZOBS = 93 deg is returned, appropriately + signed. + + 7 As in the original Hohenkerk and Sinclair algorithm, fixed values + of the water vapour polytrope exponent, the height of the + tropopause, and the height at which refraction is negligible are + used. + + 8 The radio refraction has been tested against work done by + Iain Coulson, JACH, (private communication 1995) for the + James Clerk Maxwell Telescope, Mauna Kea. For typical conditions, + agreement at the 0.1 arcsec level is achieved for moderate ZD, + worsening to perhaps 0.5-1.0 arcsec at ZD 80 deg. At hot and + humid sea-level sites the accuracy will not be as good. + + 9 It should be noted that the relative humidity RH is formally + defined in terms of "mixing ratio" rather than pressures or + densities as is often stated. It is the mass of water per unit + mass of dry air divided by that for saturated air at the same + temperature and pressure (see Gill 1982). + + Called: slDA1P, slATMT, slATMS + + P.T.Wallace Starlink 3 June 1997 + + Copyright (C) 1997 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |