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diff --git a/math/slalib/doc/dm2av.hlp b/math/slalib/doc/dm2av.hlp new file mode 100644 index 00000000..6448b842 --- /dev/null +++ b/math/slalib/doc/dm2av.hlp @@ -0,0 +1,38 @@ +.help dm2av Jun99 "Slalib Package" +.nf + + SUBROUTINE slDMAV (RMAT, AXVEC) + + - - - - - - + D M A V + - - - - - - + + From a rotation matrix, determine the corresponding axial vector. + (double precision) + + A rotation matrix describes a rotation about some arbitrary axis. + The axis is called the Euler axis, and the angle through which the + reference frame rotates is called the Euler angle. The axial + vector returned by this routine has the same direction as the + Euler axis, and its magnitude is the Euler angle in radians. (The + magnitude and direction can be separated by means of the routine + slDVN.) + + Given: + RMAT d(3,3) rotation matrix + + Returned: + AXVEC d(3) axial vector (radians) + + The reference frame rotates clockwise as seen looking along + the axial vector from the origin. + + If RMAT is null, so is the result. + + P.T.Wallace Starlink 24 December 1992 + + Copyright (C) 1995 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |