• Standalone scripts
• CodeV macros
• Zemax macros
• Converters

• cam.py - focusing cam generator

  Creates cam functions (tabulated and approximated) for floating elements based on zoom data in a CodeV .seq file. Distance to object (S0 thickness) is converted to diopters and treated as a free variable that other zoomed thicknesses depend on.

  Unlike CodeV built-in CAM option, uses Akima splines for interpolation and offers power series approximation. Plots airspace thickness and approximation error graphs.

• af3c.py - first order layout of a 3-group Galilean telescope

  Generates 3 Zemax files for each of the 'scope's thin lenses. Those can be transformed into thick groups using Russinov's methodology, pre-optimized independently for minimum tolerance sensitivity with a curved field, and eventually assembled into a flat-field system.

1. Copy into a dir that's traversed by CodeV, e.g. c:\cvuser\macros\.
2. Load libraries on startup. Your defaults.seq will contain something like this:

   pth seq pre c:\cvuser\macros\
   ddm m
   in libmath
   in libtxt
   in libgeom
   in libmfg
   in globals
   

3. Macros with req'd arguments provide 'Usage: ...' notes when invoked w/o args.

These macros, as dowloaded from GitHub, are in UTF8. But since they only use ISO 8859-1 characters, they should be byte-to-byte identical to ASCII and thus palatable to CodeV.

• res.seq - resolution figures & transverse aberration plots
• petz.seq - element power distribution and Petzval sums
• amag.seq - afocal magnification
• mtf.seq - resolution figures for any 2 modulation values (default is 0.2 and 0.3)

• lay.seq - view lens at one (e.g. in lay 2) or every (just in lay w/o args) zoom position with auto scaling and color coded surface types
• xz.seq - same as lay.seq, but XZ section is shown instead of YZ
• xy.seq - 3D plot of a lens
• prescr2tex.seq - generates a LaTeX table with current lens' prescription

• galilean.seq - insert a 2-group afocal Galilean subsystem

• af3c.seq - layout and insert a 3-group Galilean

  Plots P2 and P3 (2nd and 3rd lens' power) vs P1, finds optimal P1 values for minimum RMS power and minimum Petzval.

• reverse.seq - flip lens & auto-convert fields and pupils

• ins_lens.seq - fully interactive insertion of a subsystem from a lens file

  Unlike CodeV built-in COPY command, this macro

  1. takes care of zoom data (variable airspaces and conjugates);
  2. recognizes a relay/converter inserted right before the image and brings along its image-space conjugates;
  3. doesn't require a long string of parameters: lens file and surface indices are specified interactively.

  Because of (3), both main and aux lenses have to be in the same directory.

• ins_elt.seq - insert a spherical element of given power & bending

• ins_xcyl.seq, ins_ycyl.seq - insert a cylindrical element

• ins_plate.seq - insert a (bent) plane parallel plate

• bend.seq - bend a singlet (spherical or cylindrical) to a specified Coddington shape factor

• bendflip.seq - flip a singlet w/o changing its power

• cement.seq - convert a singlet into a cemented doublet

• move_srf.seq

• relay.seq - create a new lens relaying the current lens' image

  Image becomes object, EXP becomes ENP. Fields, wavelengths and image curvature are taken care of.

• sph2xcyl.seq, sph2ycyl.seq - convert surfaces M..N into X or Y cylinders

• apertures.seq - auto set hard apertures (rectangular if element is not rotationally symmetric).

• wtz.seq - matrix of optimization weigths for each field at every zoom position

  All field weights for a given zoom position can be scaled at once with in wtz [z] [multiplier] - wtz.seq acts like a 'missing' WTZ command would've acted.

• fields_diag.seq - N equal-area field rings
• fields_skew.seq - rectangular angular field with diagonal points
• fields_diag2xy.seq - convert a diagonal field spec to a rectangular with a given aspect ration
• fields_xy2diag.seq - convert a rectagular field spec into a diagonal one

• store.seq - save and refresh derivatives

  Saves both a binary LEN and a text SEQ file. Deals with a decades-old problem of Code V randomly corrupting the derivative increment vector in LEN files - this is what has been causing all those 'Singular variable' and 'Unstable condition' errors since CV9 or probably even CV8.

• get.seq - search for lenses in directory and load by ordinal

  This is too much to type:

  > lib
  > dir *.len
  > can
  > res reverse_telephoto_1f8_v1o2achr1
  > vie; go
  

  This is much better:

  > in get 'rev'
  > 12
  > y
  

  Here, all lenses with 'rev' in the name are listed, and you select the №12. If no search string is specified, all LEN files in the directory are displayed.

• gsview.seq - view Nth best GS solution

  Requires worksheet recording to be on (buf y) during optimization and a gallery.seq run immediately after.

  Example:

  buf y
  auto
      gs y
      tim 10
      err cdv
  go
  buf n
  in gallery 
  
  > in gsview 3 ! load & view third-best lens
  > in gsview   ! view next (4th) lens
  

• libgeom.seq - geometric optics
• lib_ys.seq - Yuan-Seidel anamorphic lens aberrations
• libmfg.seq - manufacturability
• libmath.seq - non-optics specific math
• libtxt.seq - string processing
• globals.seq - env var declarations

• autocentering.zpl - fill in wedge tolerances for elements that can self-center in a grinder's chuck

• cvmacro/zmx_plate_import.seq - convert Zemax .tpd test plate file into a .seq file that can be used by Code V's TES option