Home Manual Packages Global Index Keywords Quick Reference | # functions in drat.i - d
default_gate |
                 default_gate(times)

         initial value of drat_gate.  Refer to the source code
         to learn how to write your own gate function, making proper use
         of drat_start and drat_stop options in addition to the input times.

    interpreted function, defined at i0/drat.i   line 772
SEE ALSO: | gauss_gate, drat_gate
default_integrate |
                 atten_emit= default_integrate(f, mesh, time, irays, slimits)

         is the default drat_integrate routine.
         On entry, file F is positioned at TIME, from which MESH has already
         been read.  IRAYS and SLIMITS are the rays coordinates (in internal
         format) and integration limits.
         The result should be ngroup-by-2-by-raydims, where the second index
         is 1 for the attenuation factor, 2 for the self-emission (specific
         intensity due to emission along the ray).
       OPTIONS: drat_linear, drat_ocompute, drat_oadjust,
                drat_emult, drat_amult, drat_omult, drat_nomilne,
    	    drat_ekap, drat_akap, drat_glist

    interpreted function, defined at i0/drat.i   line 167
SEE ALSO: | streak
default_ocompute |
                 default_ocompute(f, time)

         initial value of drat_ocompute.  Extracts drat_akap and drat_ekap
         from file F, possibly using the subset drat_glist.  TIME is unused.

    interpreted function, defined at i0/drat.i   line 717
drat_akap |
     drat_akap

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_amult |
                 drat_amult, drat_emult, drat_omult

         are optional opacity multipliers used by the streak, snap, and
         streak_save functions.  The multipliers are applied to the
         opacity and source functions before the transport equation is
         integrated.  Setting them to [] is the same as setting them
         to 1.0.
         DRAT_EMULT     - multiply the emissivity by this factor,
                             without affecting the absorption
    	    opac   <- opac
    	    source <- source*DRAT_EMULT
         DRAT_AMULT   - multiply the absorption opacity by this
                             factor, without affecting the emissivity
    	    opac   <- opac*(DRAT_AMULT+1.e-20)
    	    source <- source/(DRAT_AMULT+1.e-20)
         DRAT_OMULT      - multiply BOTH the absorption opacity and the
                             emissivity by this factor
    	    opac   <- opac*DRAT_OMULT
    	    source <- source
         DRAT_IREG_ADJ   - list of region numbers to be zeroed.  This
                           has the same effect as a zero DRAT_OMULT in
    		       the corresponding zones, but is more efficient.
         Since opac and source are mesh-by-ngroup (where mesh is usually
         kmax-by-lmax), DRAT_EMULT, DRAT_AMULT, DRAT_OMULT can
         be scalars, mesh arrays, 1-by-1-by-ngroup arrays, or
         kmax-by-lmax-by-ngroup arrays.  If DRAT_GLIST is non-nil, ngroup
         should be numberof(DRAT_GLIST), not the total number of groups.

    keyword,  defined at i0/drat.i   line 484
SEE ALSO: | drat_glist, adjust_ireg
drat_backlight |
                 func drat_backlight(time) { extern gb, gav;  ... }
              or drat_backlight=
     	 or drat_backlight=

         supplies a backlighter for the snap function.
         Given ngroup-by-nrays transparency fraction transp and self-emission
         selfem (in specific intensity units), snap applies the backlighter
         using:
            result= backlighter*transp + selfem;
         where backlighter is drat_backlight(time), if drat_backlight is
         a function, or drat_backlight itself, if drat_backlight is an
         array.
         Note that the result (or value) of backlighter_func must be
         conformable with transp and selfem.  Most commonly, drat_backlight
         will be a vector of length ngroup -- a Planckian backlighter at
         temperature Tr would be
            drat_backlight= B_nu(gav, Tr);
         -- but that a scalar, 1-by-nrays, or ngroup-by-nrays are all
         possible.
         Note also that if drat_backlight is a function, the gb and gav
         arrays read from the history file are available as external
         variables.

    keyword,  defined at i0/drat.i   line 584
SEE ALSO: | snap, drat_channel, drat_gate, apply_funcs
drat_channel |
                 func drat_channel(time) { extern gb, gav;  ... }
              or drat_channel=
     	 or drat_channel=

         supplies a channel response for the snap function.
         Use the drat_glist option to select a subset of the groups;
         drat_channel can be used in addition to drat_glist.
         Given ngroup-by-nrays specific intensity, snap applies the
         channel response using:
            result= drat_channel(..,+)*specific_intensity(+,..);
         if drat_channel is an array, or
            result= drat_channel(specific_intensity, time);
         if drat_channel is a function.
         Note that if drat_channel is an array, its final dimension must
         be of length ngroup.  A multidimensional drat_channel represents
         more than one channel response function.  Most drat_channel
         arrays will be proportional to the bin widths gb(dif).  The
         correct way to interpolate a filter function transmission
         fraction known at photon enrgies efa is:
            drat_channel= integ(ffa, efa, f.gb)(dif)
         If you have more than one channel, the first dimension of
         drat_channel should be the channel number.
         The best way to generate a filter response function is to
         use Yorick's cold opacity library.  To do this:
            #include "coldopac/xray.i"
         This will define the functions cold_opacity and cold_reflect,
         which you can use to build up channel response functions from
         filter materials and thicknesses and mirror compositions.
         Note also that if drat_channel is a function, the gb and gav
         arrays read from the history file are available as external
         variables.

    keyword,  defined at i0/drat.i   line 612
SEE ALSO: | drat_glist, snap, drat_backlight, drat_gate, apply_funcs
drat_compress |
                 func drat_compress(transp, selfem, time)
              or drat_compress=

         supplies a compression algorithm to the streak function.
         The drat_compress can return anything, as long as it returns the
         same shape array (or nil) at each time.  The snap_worker and
         streak_saver routines are examples of compression algorithms.

    keyword,  defined at i0/drat.i   line 575
drat_ekap |
     drat_ekap

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_emult |
     drat_emult

    keyword,  defined at i0/drat.i   line 484
SEE | drat_amult
drat_gate |
                 func drat_gate(times) { extern gb, gav;  ... }
              or drat_gate=

         supplies a gate (to make gated images) for the snap function.
         For a simple gate, the drat_start and drat_stop options will
         be more efficient than drat_gate.
         The input to drat_gate is the list of dump times; the output
         should be the "effective dt" for each of these dumps.  This is
         the product of the actual time interval and the gate transparency;
         the sum of the return vector is the gate time.  See the default_gate
         and gaussian_gate functions for examples.
         Note that the gb and gav arrays read from the history file are
         available as external variables, in case the gate transparency is
         frequency dependent.

    keyword,  defined at i0/drat.i   line 652
SEE ALSO: | snap, drat_backlight, drat_channel, apply_funcs, drat_start, drat_stop, gaussian_gate, default_gate
drat_gav |
     drat_gav

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_gb |
     drat_gb

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_glist |
                 drat_glist

         if non-nil, an index list into the final dimension of akap and ekap.
         Only these groups will be read from disk and used in the transport
         calculation.  All other options which depend on "ngroup" or "gav"
         should use numberof(DRAT_GLIST) or gav(DRAT_GLIST) instead.  The
         "gb" group boundary array is not well-defined in this case, since
         the group boundaries need not be contiguous.  The best strategy is
         to save drat_glist and the original gb array.
         DRAT_GLIST must be a 1-D, 1-origin index list.  (1-origin even if
         gav and gb are not 1-origin, since use_origins(0) will be in effect
         when DRAT_GLIST is used.)  The streak function will be most efficient
         if DRAT_GLIST is strictly increasing.

    keyword,  defined at i0/drat.i   line 531
SEE ALSO: | drat_channel
drat_integrate |
                 func drat_integrate(file, mesh, time, irays, slimits) { ... }
              or drat_integrate=

         integrate the transport equation.  FILE is positioned to TIME, and
         MESH has already been read.  IRAYS are the rays in internal format
         and SLIMITS is the integration limits.  The return value should be
         ngroup-by-2-by-raydims (where irays is 6-by-raydims).  The default
         integrator is default_integrate, which handles the drat_ocompute,
         drat_oadjust, drat_amult, drat_emult, drat_omult, drat_akap,
         drat_ekap, drat_glist, drat_linear, and drat_nomilne options.
         Reasons to replace the default routine include: (1) Some or all of
         the opacities come from a source other than the FILE, e.g.- a second
         post processing file.  (2) The total number of zones times number of
         groups is debilitatingly large, even though the number of rays times
         the number of groups is not.

    keyword,  defined at i0/drat.i   line 693
drat_ireg |
     drat_ireg

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_ireg_adj |
     drat_ireg_adj

    keyword,  defined at i0/drat.i   line 484
SEE | drat_amult
drat_isymz |
     drat_isymz

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_khold |
     drat_khold

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_lhold |
     drat_lhold

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt
drat_linear |
                 drat_linear, drat_nomilne

         Set DRAT_LINEAR to 1 in order to use integ_linear to perform the
         transport integration instead of the default integ_flat.
         The DRAT_NOMILNE option, if non-nil, is a list of "norad"
         edges in the (rt,zt) mesh (other than the khold and lhold lines),
         which is required for the source function point centering operation.
         DRAT_NOMILNE is a 2 or 3-D array with the format:
            [[k1,l1], [k2,l2]]
         or an array of elements of that form, where either k1==k2 or
         l1==l2.  (Where k is the first index of rt or zt and l is the second.)
         DRAT_NOMILNE must always be a 1-origin index list into the (rt,zt)
         mesh, independent of the index origins of rt and/or zt.

    keyword,  defined at i0/drat.i   line 549
SEE ALSO: | integ_linear, integ_flat
drat_nomilne |
     drat_nomilne

    keyword,  defined at i0/drat.i   line 549
SEE | drat_linear
drat_oadjust |
     drat_oadjust

    keyword,  defined at i0/drat.i   line 673
SEE | drat_ocompute
drat_ocompute |
                 func drat_ocompute(file, time) { extern opac, source; ...}
              or drat_ocompute=

    	and func drat_oadjust(file, time) { extern opac, source; ...}
             or drat_oadjust=
         supply opacities from a source other than the file.drat_akap and
         file.drat_ekap, or adjust these values.  You need to be cognizant of
         the drat_glist option (see get_kaps source code).
         DRAT_OCOMPUTE must set opac and source entirely on its own;
         DRAT_OADJUST will be called afterwards.
         The default DRAT_OCOMPUTE (default_ocompute) reads drat_akap and
         drat_ekap from FILE, optionally extracting drat_glist, and places
         them in opac and source.
         DRAT_OADJUST is free to modify opac and source them at will; the
         default DRAT_OADJUST is nil, which means no adjustment.
         Any opacity or emissivity multipliers will be applied after
         DRAT_OADJUST, as will the point centering operation if necessary
         (DRAT_OADJUST should return zone centered opacities).

    keyword,  defined at i0/drat.i   line 673
drat_omult |
     drat_omult

    keyword,  defined at i0/drat.i   line 484
SEE | drat_amult
drat_quiet |
                 drat_quiet

         By default, Drat prints the total number of records it will process,
         and the number of the record it is currently processing.  If drat_quiet
         is non-nil and non-zero, the printout is supressed.

    keyword,  defined at i0/drat.i   line 710
drat_rt |
                 drat_rt, drat_zt, drat_ireg,
                 drat_akap, drat_ekap,

    	    drat_isymz,
    	    drat_khold, drat_lhold,
    	    drat_gb, drat_gav
         can be set to strings other than "rt", "zt", etc. (their default
         values) to force the streak, snap, and streak_save routines to use
         alternative names to look up these quantites in the history file.
         The following 4 variables are NOT optional:
         (rt, zt) must be a 2-D mesh in cylindrical coordinates
         akap is a mesh-by-ngroup array of absorption opacities, in units
              of reciprocal length (1/rt or 1/zt)
         ekap is a mesh-by-ngroup array of source functions, in (arbitrary)
              specific intensity units
         The akap and ekap arrays must be zone centered; the first row and
         column of akap and ekap will be ignored.
         The remaining variables are all optional -- set the drat_.. variable
         to [] to ignore them completely.  Otherwise, they will be ignored if
         they are not present in the history file, and used as follows
         otherwise:
         ireg is a mesh-size region number array (zone centered as akap and
              ekap).  Zones where ireg==0 do not exist.
         isymz is non-zero if the problem has reflection symmetry about z=0,
              zero otherwise.  The drat_symmetry option overrides this value.
         khold and lhold are mesh indices specifying "hold lines" --
              khold is an index into the first dimension of (rt,zt), and
              lhold is an index into the second dimension of (rt,zt).
    	  These are used only if the drat_linear option is specified.
         gb and gav are, respectively, the group boundary energies and group
              center energies.  These are used by the snap and streak_save
    	  functions.

    keyword,  defined at i0/drat.i   line 445
SEE ALSO: | streak, snap, streak_save, drat_symmetry, drat_linear
drat_start |
                 drat_start, drat_stop

         if non-nil, specify the minimum and maximum dump times which will
         be considered by the streak, snap, or streak_save functions.

    keyword,  defined at i0/drat.i   line 518
drat_static |
                 drat_static

         if non-nil, a list of strings representing variable names in the
         input file which the streak_save function should copy to the
         output file.

    keyword,  defined at i0/drat.i   line 567
SEE ALSO: | streak_save
drat_stop |
     drat_stop

    keyword,  defined at i0/drat.i   line 518
SEE | drat_start
drat_symmetry |
                 drat_symmetry

         set to 2 to force spherical symmetry, 1 to force reflection symmetry
         about the z=0 plane, 0 to force no symmetry, [] (the default) to
         use the guess_symmetry function to compute problem symmetry.

    keyword,  defined at i0/drat.i   line 524
drat_zt |
     drat_zt

    keyword,  defined at i0/drat.i   line 445
SEE | drat_rt