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: http://www.eso.org/~chummel/oyster/manual/node185.html
Дата изменения: Tue Apr 28 19:12:50 2015 Дата индексирования: Sun Apr 10 20:39:11 2016 Кодировка: Поисковые слова: moon |
All arguments for these procedures and functions can be arrays. All require
existence of GeoParms variable. A default can be created by using
get_geoparms
utc2ut1(utc_real)
Function. Returns UT1 in seconds, with UTC input in seconds.ut12gst(utc_real[,ut1_real])
Function. Returns GST in hours, inputs are in seconds.hourangle(gst_real,ra_real)
Function. Return hourangle in hours, with inputs also in hours.zenithangle(ha_real,dec_real)
Function. Return zenithangle in degrees with inputs ha in hours and dec in degrees.mirrorangle(ha_real,dec_real)
Function. Return mirrorangle in degrees with inputs ha in hours and dec in degrees.horizon2equatorial(coord_real)
Function. Return equatorial coordinates for input horizontal coordinates X=east, Y=north, and Z=up.equatorial2horizon(coord_real)
Function. Return horizon coordinates for input equatorial coordinates X=projection of local meridian on equator, Y=east, and Z=north.angle2horizon(coord_real)
Function. Return horizon coordinates for input azimuth and elevation angle in degrees. No GeoParms required.equatorial2angle(coord_real)
Function. Return hour angle in hours and declination in degrees for input equatorial coordinates. No GeoParms required.topostar,times_real,stars_char,startable,ra,dec
Compute apparent declinations and right ascensions for a list of times (in seconds UTC) and corresponding stars. (The arrays time and stars have to have the same number of elements therefore.) The startable is a standard STARBASE startable. The geoparms structure has to be loaded.calcastrom
Procedure. Compute astrometric variables in scans structure.calcvis
Procedure. Compute estimated visibilities, i.e. normalized visibilities.referencestation,station_char[,class_char]
Change reference station for data of specified class (default all classes) to station.precess,theta,jy,ra,dec,direction
Precess J2000 position angles (theta) to current Julian Year epoch (jy) for direction=1, from current to J2000 for direction=-1. (see: Heintz, "Double stars", p. 33). Input theta is in radians, dec in degrees, ra in hours; output is in radians.