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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/slalib.men | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
Diffstat (limited to 'math/slalib/doc/slalib.men')
-rw-r--r-- | math/slalib/doc/slalib.men | 179 |
1 files changed, 179 insertions, 0 deletions
diff --git a/math/slalib/doc/slalib.men b/math/slalib/doc/slalib.men new file mode 100644 index 00000000..2288c0aa --- /dev/null +++ b/math/slalib/doc/slalib.men @@ -0,0 +1,179 @@ + addet - add the E-terms to a pre IAU 1976 mean place + afin - convert a sexagesimal character string to radians (s.p.) + airmas - compute the airmass at a given zenith distance + altaz - compute altazimuth positions, velocities, accelerations + amp - convert a geocentric apparent to post IAU 1976 mean place + ampqk - convert a geocentric apparent to post IAU 1976 mean place + aop - convert an apparent to observed place + aoppa - pre-compute the set of apparent to observed place parameters + aoppat - recompute the apparent to observed place sidereal time parameter + aopqk - convert an apparent to observed place + atmdsp - apply atmospheric dispersion terms to refraction coefficients + av2m - compute a rotation matrix from an axial vector (s.p.) + bear - compute the bearing of a point on a sphere w.r.t. another + caf2r - convert degrees, arcminutes, and arcseconds to radians + caldj - convert a Gregorian calendar date to a modified Julian date + calyd - convert a Gregorian calendar date to a Julian calendar year, day + cc2s - convert Cartesian to spherical coordinates (s.p.) + cc62s - convert a 6-vector from Cartesian to spherical coordinates + cd2tf - convert an interval in days to hours, minutes, and seconds + cldj - convert a Gregorian calendar date to a modified Julian date + clyd - convert a Gregorian calendar date a Julian calendar year, day + cr2af - convert radians to degrees, arcminutes, and arcseconds + cr2tf - convert radians to hours, minutes, and seconds + cs2c - convert spherical to Cartesian coordinates (s.p.) + cs2c6 - convert spherical position/velocity to Cartesian coordinates + ctf2d - convert hours, minutes, and seconds to days + ctf2r - convert hours, minutes, and seconds to radians + daf2r - convert degrees, arcminutes, and arcseconds to radians (d.p) + dafin - convert a sexagesimal character string to radians (d.p.) + dat - compute difference between TAI and UTC in seconds + dav2m - compute a rotation matrix from an axial vector (d.p) + dbear - compute the bearing of a point on a sphere w.r.t. another (d.p.) + dbjin - convert a character string to a Besselian/Julian epoch + dc62s - convert Cartesian position/velocity to spherical coordinates (d.p.) + dcc2s - convert Cartesian to spherical coordinates (d.p) + dcmpf - convert linear fit coefficients to geometric parameters + dcs2c - convert spherical to Cartesian coordinates (d.p) + dd2tf - convert interval in days to hours, minutes, and seconds (d.p.) + de2h - convert hour angle and declination to azimuth and elevation (d.p.) + deuler - convert Euler angles to a rotation matrix (d.p.) + dfltin - convert a character string to a floating point number (d.p.) + dh2e - convert azimuth and elevation to hour angle and declination (d.p.) + dimxv - apply a 3D reverse rotation to a 3-vector (d.p.) + djcal - convert an MJD to a Gregorian calendar date + djcl - convert an MJD to a Gregorian year, month, and day + dm2av - convert a rotation matrix to an axial vector (d.p) + dmat - solve a set of simultaneous equations (d.p.) + dmoon - compute approximate geocentric position/velocity of moon (d.p.) + dmxm - compute the product of two 3X3 matrices (d.p.) + dmxv - multiple a 3-vector by a rotation matrix (d.p.) + dpav - compute the bearing of a point on a sphere w.r.t. another (d.p.) + dr2af - convert radians to degrees, arcminutes, and arcseconds (d.p) + dr2tf - convert radians to hours, minutes, and seconds (d.p.) + drange - normalize an angle to the range -pi <= angle <= pi (d.p.) + dranrm - normalize an angle to the range 0 <= angle <= 2pi (d.p.) + ds2c6 - convert spherical position/velocity to Cartesian coordinates (d.p.) + ds2tp - project spherical coordinates onto the tangent plane (d.p) + dsep - compute the angle between two points on a sphere (d.p.) + dt - estimate the approximate difference between ET and UT in seconds + dtf2d - convert hours, minutes, and seconds to days (d.p) + dtf2r - convert hours, minutes, and seconds to radians (d.p.) + dtp2s - convert tangent plane to spherical coordinates (d.p.) + dtp2v - convert tangent plane coordinates to direction cosines (d.p.) + dtps2c - compute the spherical coordinates of the tangent point (d.p.) + dtpv2c - compute the direction cosines of the tangent point (d.p.) + dtt - compute the difference between TT and UTC in seconds + dv2tp - convert direction cosines to tangent plane coordinates (d.p) + dvdv - compute the scalar product of 2 3-vectors (d.p.) + dvn - normalize a 3-vector and compute the modulus (d.p.) + dvxv - compute the vector product of 2 3-vectors (d.p.) + e2h - convert hour angle and declination to azimuth and elevation (d.p.) + earth - compute approximate heliocentric position/velocity of earth + ecleq - convert from ecliptic to equatorial FK5 coordinates + ecmat - compute the equatorial FK5 to ecliptic coordinates rotation matrix + ecor - compute rv of earth and time correction to sun in given direction + eg50 - convert equatorial FK4 to IAU 1958 galactic coordinates + el2ue - convert osculating orbital elements into universal form + epb - convert an MJD to a Besselian epoch + epb2d - convert a Besselian epoch to an MJD + epco - convert a Besselian/Julian epoch to match a given epoch + epj - convert an MJD to a Julian epoch + epj2d - convert a Julian epoch to an MJD + eqecl - convert equatorial FK5 to ecliptic coordinates + eqeqx - compute the equation of the equinoxes + eqgal - convert equatorial FK5 to IAU 1958 galactic coordinates + etrms - compute the E-terms vector + euler - convert Euler angles to a rotation matrix (s.p.) + evp - compute the barycentric/heliocentric velocity/position of earth + fitxy - fit a linear model to 2 sets of [x,y] coordinates + fk425 - convert equatorial FK4 to FK5 coordinates + fk45z - convert equatorial FK4 to FK5 coordinates excluding proper motion + fk524 - convert equatorial FK5 to FK4 coordinates + fk54z - convert equatorial FK5 to FK4 coordinates excluding proper motion + fk52h - convert equatorial FK5 to ICRS coordinates + fk5hz - Convert equatorial FK5 to ICRS coordinates (0 ICRS proper motions) + flotin - convert a character string to a floating point number + galeq - convert IAU 1958 galactic to equatorial FK5 coordinates + galsup - convert IAU 1958 galactic to deVaucouleurs supergalactic coordinates + ge50 - convert IAU 1958 galactic to equatorial FK4 coordinates + geoc - convert geodetic to geocentric position + gmst - convert from UT1 to GMST + gmsta - convert from UT1 to GMST while minimizing rounding errors + h2e - convert azimuth and elevation to hour angle and declination (s.p.) + h2fk5 - Convert equatorial ICRS to FK5 coordinates + hfk5z - Convert equatorial ICRS to FK5 coordinates (0 ICRS proper motions) + imxv - apply a 3D reverse rotation to a 3-vector (s.p.) + intin - convert a character string into an integer + invf - invert the linear model computed from 2 sets of [x,y] coordinates + kbj - select the epoch prefix B or J + m2av - convert a rotation matrix to an axial vector (s.p.) + map - convert a post IAU 1976 mean to geocentric apparent place + mappa - precompute the set of mean to geocentric apparent place parameters + mapqk - convert a post IAU 1976 mean to geocentric apparent place + mapqkz - convert a post IAU 1976 mean to geocentric apparent place + moon - compute approximate geocentric position/velocity of moon + mxm - compute the product of two 3X3 matrices (s.p.) + mxv - multiply a 3-vector by a rotation matrix (s.p.) + nut - compute the nutation matrix for a given date + nutc - compute the nutation components for a given date + oap - convert from observed to apparent place + oapqk - convert from observed to apparent place + obs - look up an entry in a list of groundbased observing stations + pa - compute the parallactic angle from the hour angle and declination + pav - compute the bearing of a point on a sphere w.r.t. another + pcd - apply pincushion/barrel distortion to tangent plane coordinates + pda2h - compute the hour angle corresponding to a given azimuth + pdq2h - compute the hour angle corresponding to a given parallactic angle + pertel - update osculating orbital elements by applying perturbations + pertue - update universal elements by applying perturbations + planel - compute the approximate heliocentric position/velocity of a planet + planet - compute the approximate heliocentric position/velocity of a planet + plante - compute approximate topocentric apparent position of a planet + pm - apply the correction for proper motion to a star + polmo - correct site longitude and latitude for polar motion + prebn - compute the FK4 matrix of precession between two epochs + prec - compute the FK5 matrix of precession between two epochs + preces - precess coordinates in either the FK4 or FK5 systems + precl - compute the longterm matrix of precession between two epochs + precss - precess coordinates in either the FK4 or FK5 systems + prenut - compute the FK5 matrix of precession and nutation + pv2el - convert J2000 position and velocity to osculating elements + pv2ue - convert instantaneous position and velocity to universal element set + pvobs - compute the geocentric position / velocity of an observing station + pxy - apply a linear model to a set of expected and measured [x,y] + range - normalize an angle to the range -pi <= angle <= pi (s.p.) + ranorm - normalize an angle to the range 0 <= angle <= 2pi (s.p.) + rcc - compute the difference between TDB and TT in seconds + rdplan - compute approximate topocentric apparent position of a planet + refco - compute the refraction coefficients + refcoq - compute the refraction coefficients (fast version) + refro - compute the atmospheric refraction for optical and radio wavelengths + refv - apply the refraction correction to a Cartesian 3-vector + refz - apply the refraction correction to a zenith distance + rverot - compute the earth rotation velocity component in a given direction + rvgalc - compute the dynamical LSR velocity component in a given direction + rvlg - compute the solar velocity component in a given direction + rvlsrd - compute the peculiar solar velocity component in a given direction + rvlsrk - compute the standard solar velocity component in a given direction + s2tp - project spherical coordinates onto the tangent plane (s.p.) + sep - compute the angle between two points on a sphere (s.p.) + smat - solve a set of simultaneous equations (s.p.) + subet - remove the E-terms from a pre IAU 1976 catalog position + supgal - convert deVaucouleurs supergalactic to IAU 1958 galactic coordinates + svd - compute the SVD factorization of a matrix + svdcov - compute the covariance matrix from the SVD factorization + svdsol - solve a set of simultaneous equations using SVD factorization + tp2s - convert tangent plane to spherical coordinates (s.p.) + tp2v - convert tangent plane coordinates to direction cosines (s.p.) + tps2c - compute the spherical coordinates of the tangent point (s.p.) + tpv2c - compute the direction cosines of the tangent point (s.p.) + ue2el - convert universal elements into heliocentric osculating elements + ue2pv - compute heliocentric position and velocity from universal form + unpcd - remove pincushion/barrel distortion from distorted coordinates + v2tp - convert direction cosines to tangent plane coordinates (s.p.) + vdv - convert the scale production of two 3-vectors (s.p.) + vn - normalize a 3-vector and compute the modulus (s.p.) + vxv - compute the vector product of two 3-vectors (s.p.) + xy2xy - apply a computed linear model to a set of [x,y] + zd - convert hour angle and declination to zenith distance |