Home Manual Packages Global Index Keywords Quick Reference | # all functions - l
l_frame |
     l_frame

    struct l_frame {
      float x_min, x_max, y_min, y_max;
    }

    structure, defined at i/testb.i   line 884
lagrange |
     lagrange

    _frame

    interpreted function, defined at i/demo3.i   line 78
laguerre |
                 laguerre(a,x)

         Given the coefficients a(1:m+1) of the m'th degree
         complex polynomial Sum(a(i)*x^(i-1)) and a guess x, returns a root.
         See Numerical Recipes (Press, et. al., Cambridge Univ. Press 1988),
         section 9.5.

    interpreted function, defined at i/zroots.i   line 70
laplacian |
     laplacian

    interpreted function, defined at i/demo2.i   line 158
lcm |
                 lcm(a,b)

         returns the LCM (least common multiple) of A and B, which must
         be one of the integer data types.  A and B may be conformable
         arrays; the semantics of the lcm call are the same as any other
         binary operation.
         The absolute values of A and B are taken before the operation
         commences; if either A or B is 0, the return value will be 0.

    interpreted function, defined at i/gcd.i   line 47
SEE ALSO: | gcd, is_prime, factorize
legal |
                 legal

         Prints the legal details of Yorick's copyright, licensing,
         and lack of warranty.

    interpreted function, defined at i0/std.i   line 88
SEE ALSO: | copyright, warranty
legndr |
                 legndr(l,m, x)

         return the associated Legendre function Plm(x).  The X may
         be an array (-1<=x<=1), but L and M (0<=M<=L) must be scalar
         values.  For m=0, these are the Legendre polynomials Pl(x).
         Relation of Plm(x) to Pl(x):
           Plm(x) = (-1)^m (1-x^2)^(m/2) d^m/dx^m(Pl(x))
         Relation of Plm(x) to spherical harmonics Ylm:
           Ylm(theta,phi)= sqrt((2*l+1)(l-m)!/(4*pi*(l+m)!)) *
                               Plm(cos(theta)) * exp(1i*m*phi)

    interpreted function, defined at i/legndr.i   line 12
SEE ALSO: | ylm_coef
library |
                 library

         print the Y_SITE/i/README file at the terminal.

    interpreted function, defined at i0/std.i   line 1535
light3 |
                 light3, ambient=a_level,
                         diffuse=d_level,

    		    specular=s_level,
    		    spower=n,
    		    sdir=xyz
         Sets lighting properties for 3D shading effects.
         A surface will be shaded according to its to its orientation
         relative to the viewing direction.
         The ambient level A_LEVEL is a light level (arbitrary units)
         that is added to every surface independent of its orientation.
         The diffuse level D_LEVEL is a light level which is proportional
         to cos(theta), where theta is the angle between the surface
         normal and the viewing direction, so that surfaces directly
         facing the viewer are bright, while surfaces viewed edge on are
         unlit (and surfaces facing away, if drawn, are shaded as if they
         faced the viewer).
         The specular level S_LEVEL is a light level proportional to a high
         power spower=N of 1+cos(alpha), where alpha is the angle between
         the specular reflection angle and the viewing direction.  The light
         source for the calculation of alpha lies in the direction XYZ (a
         3 element vector) in the viewer's coordinate system at infinite
         distance.  You can have ns light sources by making S_LEVEL, N, and
         XYZ (or any combination) be vectors of length ns (3-by-ns in the
         case of XYZ).  (See source code for specular_hook function
         definition if powers of 1+cos(alpha) aren't good enough for you.)
         With no arguments, return to the default lighting.
       EXAMPLES:
         light3, diffuse=.1, specular=1., sdir=[0,0,-1]
           (dramatic "tail lighting" effect)
         light3, diffuse=.5, specular=1., sdir=[1,.5,1]
           (classic "over your right shoulder" lighting)
         light3, ambient=.1,diffuse=.1,specular=1.,
                 sdir=[[0,0,-1],[1,.5,1]],spower=[4,2]
           (two light sources combining previous effects)

    interpreted function, defined at i/pl3d.i   line 262
SEE ALSO: | rot3, save3, restore3
lightwf |
                 lightwf, cmax

         Sets the cmax= parameter interactively, assuming the current
         3D display list contains the result of a previous plwf call.
         This changes the color of the brightest surface in the picture.
         The darkest surface color can be controlled using the ambient=
         keyword to light3.

    interpreted function, defined at i/plwf.i   line 131
SEE ALSO: | plwf, light3
limit3 |
                 limit3, xmin,xmax, ymin,ymax
              or limit3, xmin,xmax, ymin,ymax, zmin,zmax

         Set the 3D axis limits for use with the cage.
         Use keyword aspect=[ax,ay,az] to set the aspect ratios of the
         cage to ax:ay:az -- that is, the ratios of the lengths of the
         cage axes will become ax:ay:az.

    interpreted function, defined at i/pl3d.i   line 181
SEE ALSO: | cage3, range3, plwf, plwf, orient3
limits |
                 limits
              or limits, xmin, xmax, ymin, ymax,

    	            square=0/1, nice=0/1, restrict=0/1
    	 or old_limits= limits()
    	 or limits, old_limits
         In the first form, restores all four plot limits to extreme values.
         In the second form, sets the plot limits in the current coordinate
         system to XMIN, XMAX, YMIN, YMAX, which may be nil or omitted to
         leave the corresponding limit unchanged, a number to fix the
         corresponding limit to a specified value, or the string "e" to
         make the corresponding limit take on the extreme value of the
         currently displayed data.
         If present, the square keyword determines whether limits marked
         as extreme values will be adjusted to force the x and y scales
         to be equal (square=1) or not (square=0, the default).
         If present, the nice keyword determines whether limits will be
         adjusted to nice values (nice=1) or not (nice=0, the default).
         There is a subtlety in the meaning of "extreme value" when one
         or both of the limits on the OPPOSITE axis have fixed values --
         does the "extreme value" of the data include points which
         will not be plotted because their other coordinate lies outside
         the fixed limit on the opposite axis (restrict=0, the default),
         or not (restrict=1)?
         If called as a function, limits returns an array of 5 doubles;
         OLD_LIMITS(1:4) are the current xmin, xmax, ymin, and ymax,
         and int(OLD_LIMITS(5)) is a set of flags indicating extreme
         values and the square, nice, restrict, and log flags.
         In the fourth form, OLD_LIMITS is as returned by a previous
         limits call, to restore the limits to a previous state.
         In an X window, the limits may also be adjusted interactively
         with the mouse.  Drag left to zoom in and pan (click left to zoom
         in on a point without moving it), drag middle to pan, and click
         (and drag) right to zoom out (and pan).  If you click just above
         or below the plot, these operations will be restricted to the
         x-axis; if you click just to the left or right, the operations
         are restricted to the y-axis.  A shift-left click, drag, and
         release will expand the box you dragged over to fill the plot
         (other popular software zooms with this paradigm).  If the
         rubber band box is not visible with shift-left zooming, try
         shift-middle or shift-right for alternate XOR masks.  Such
         mouse-set limits are equivalent to a limits command specifying
         all four limits EXCEPT that the unzoom command can revert to
         the limits before a series of mouse zooms and pans.
         The limits you set using the limits or range functions carry over
         to the next plot -- that is, an fma operation does NOT reset the
         limits to extreme values.

    builtin function, documented at i0/graph.i   line 658
SEE ALSO: | plsys, range, logxy, zoom_factor, unzoom, plg, viewport
lissajous |
                 lissajous

         runs the Yorick equivalent of an old graphics performance test
         used to compare PLAN, ALMA, and Basis with LTSS TMDS graphics.

    interpreted function, defined at i/testg.i   line 185
SEE ALSO: | testg, grtest
ln_gamma |
                 ln_gamma(z)

         returns natural log of the gamma function.
         Error is less than 2.e-10 for real part of z>=1.
         Use lngamma if you know that all z>=1, or if you don't care much about
         accuracy for z<1.

    interpreted function, defined at i/gamma.i   line 14
SEE ALSO: | lngamma, bico, beta
lngamma |
                 lngamma(x)

         returns natural log of the gamma function.
         Error is less than 2.e-10 for real part of x>=1.
         Use ln_gamma if some x<1.

    interpreted function, defined at i/gamma.i   line 35
SEE ALSO: | ln_gamma, bico, beta
log |
                 log(x)

         returns the natural logarithm of its argument (inverse of exp).

    builtin function, documented at i0/std.i   line 593
SEE ALSO: | log10, exp, asinh, acosh, atanh
log10 |
                 log10(x)

         returns the base 10 logarithm of its argument (inverse of 10^x).

    builtin function, documented at i0/std.i   line 599
SEE ALSO: | log, exp, asinh, acosh, atanh
logxy |
                 logxy, xflag, yflag

         sets the linear/log axis scaling flags for the current coordinate
         system.  XFLAG and YFLAG may be nil or omitted to leave the
         corresponding axis scaling unchanged, 0 to select linear scaling,
         or 1 to select log scaling.

    builtin function, documented at i0/graph.i   line 728
SEE ALSO: | plsys, limits, range, plg, gridxy
lon_lat |
     lon_lat

    interpreted function, defined at i/kepler.i   line 474
lon_subtract |
     lon_subtract

    interpreted function, defined at i/kepler.i   line 481
lookup_akap |
     lookup_akap

    interpreted function, defined at i/ylmdec.i   line 357
lsdir |
                 files = lsdir(directory_name)
              or files = lsdir(directory_name, subdirs)

         List DIRECTORY_NAME.  The return value FILES is an array of
         strings or nil; the order of the filenames is unspecified;
         it does not contain "." or ".."; it does not contain the
         names of subdirectories.  If SUBDIRS is given and is a simple
         variable name, it is set to a list of subdirecotry names (or
         nil if there are no subdirectories).
         If DIRECTORY_NAME does not exist, the return value is the
         integer 0 rather than nil.

    builtin function, documented at i0/std.i   line 1557
SEE ALSO: | cd, mkdir, rmdir, get_cwd, get_home