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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/altaz.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
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diff --git a/math/slalib/doc/altaz.hlp b/math/slalib/doc/altaz.hlp new file mode 100644 index 00000000..0f701093 --- /dev/null +++ b/math/slalib/doc/altaz.hlp @@ -0,0 +1,79 @@ +.help altaz Jun99 "Slalib Package" +.nf + + SUBROUTINE slALAZ (HA, DEC, PHI, + : AZ, AZD, AZDD, EL, ELD, ELDD, PA, PAD, PADD) + + - - - - - - + A L A Z + - - - - - - + + Positions, velocities and accelerations for an altazimuth + telescope mount. + + (double precision) + + Given: + HA d hour angle + DEC d declination + PHI d observatory latitude + + Returned: + AZ d azimuth + AZD d " velocity + AZDD d " acceleration + EL d elevation + ELD d " velocity + ELDD d " acceleration + PA d parallactic angle + PAD d " " velocity + PADD d " " acceleration + + Notes: + + 1) Natural units are used throughout. HA, DEC, PHI, AZ, EL + and ZD are in radians. The velocities and accelerations + assume constant declination and constant rate of change of + hour angle (as for tracking a star); the units of AZD, ELD + and PAD are radians per radian of HA, while the units of AZDD, + ELDD and PADD are radians per radian of HA squared. To + convert into practical degree- and second-based units: + + angles * 360/2pi -> degrees + velocities * (2pi/86400)*(360/2pi) -> degree/sec + accelerations * ((2pi/86400)**2)*(360/2pi) -> degree/sec/sec + + Note that the seconds here are sidereal rather than SI. One + sidereal second is about 0.99727 SI seconds. + + The velocity and acceleration factors assume the sidereal + tracking case. Their respective numerical values are (exactly) + 1/240 and (approximately) 1/3300236.9. + + 2) Azimuth is returned in the range 0-2pi; north is zero, + and east is +pi/2. Elevation and parallactic angle are + returned in the range +/-pi/2. Position angle is +ve + for a star west of the meridian and is the angle NP-star-zenith. + + 3) The latitude is geodetic as opposed to geocentric. The + hour angle and declination are topocentric. Refraction and + deficiencies in the telescope mounting are ignored. The + purpose of the routine is to give the general form of the + quantities. The details of a real telescope could profoundly + change the results, especially close to the zenith. + + 4) No range checking of arguments is carried out. + + 5) In applications which involve many such calculations, rather + than calling the present routine it will be more efficient to + use inline code, having previously computed fixed terms such + as sine and cosine of latitude, and (for tracking a star) + sine and cosine of declination. + + P.T.Wallace Starlink 14 March 1997 + + Copyright (C) 1997 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |