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functions in drat.i - d
default_gate
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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
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SEE ALSO:
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gauss_gate,
drat_gate
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default_integrate
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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
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SEE ALSO:
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streak
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default_ocompute
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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
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drat_amult
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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
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SEE ALSO:
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drat_glist,
adjust_ireg
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drat_backlight
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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
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SEE ALSO:
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snap,
drat_channel,
drat_gate,
apply_funcs
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drat_channel
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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
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SEE ALSO:
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drat_glist,
snap,
drat_backlight,
drat_gate,
apply_funcs
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drat_compress
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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
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drat_gate
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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
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SEE ALSO:
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snap,
drat_backlight,
drat_channel,
apply_funcs,
drat_start,
drat_stop,
gaussian_gate,
default_gate
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drat_glist
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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
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SEE ALSO:
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drat_channel
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drat_integrate
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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
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drat_linear
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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
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SEE ALSO:
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integ_linear,
integ_flat
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drat_ocompute
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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
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drat_quiet
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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
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drat_rt
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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
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SEE ALSO:
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streak,
snap,
streak_save,
drat_symmetry,
drat_linear
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drat_start
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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
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drat_static
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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
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SEE ALSO:
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streak_save
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drat_symmetry
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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
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