Awesome
AVSfldIO
https://github.com/JuliaIO/AVSfldIO.jl.git
File IO for AVS format "field" data files
with extension .fld
for the
Julia language,
in conjunction with the
FileIO package.
This data format supports N-dimensional arrays of real numbers.
Methods
Following the FileIO API, this package provides (but does not export) methods
AVSfldIO.load(filename)
AVSfldIO.save(filename, data)
It does export the following methods:
header, is_external_file, fid = fld_open(file ; dir="", chat=false)
header = fld_header(file::String ; dir="", chat=false)
data = fld_read(file::String ; dir="", chat=false)
fld_write(file, data ; kwargs...)
Use chat=true
for verbose debugging output.
Use dir=somepath
to prepend a path to file
.
See docstrings for more details.
Usage
Most users will simply use the FileIO
load
and save
methods
as follows.
using FileIO # need version ≥ 1.9
data1 = rand(6,7,8) # random 3D data
file = "test.fld"
save(file, data1) # will throw error if the file exists already
data2 = load(file)
@assert data1 == data2
File format overview
The AVS .fld
data format
comes in two flavors.
In the AVS "internal" format:
- an ASCII header is at the top of the file,
- the header is followed by two "form-feed" (
^L
) characters, - which are then followed by the data in binary format.
In the AVS "external" format, the header and the data are in separate files, and the ASCII header file includes the name of the data file. The data file can contain either ASCII or binary data.
AVS internal format
For a 128 × 64
array
(first dimension varies fastest)
consisting of short integers
(Int16
in Julia),
the format of the AVS internal header would be:
# AVS field file
ndim=2
dim1=128
dim2=64
nspace=2
veclen=1
data=short
field=uniform
followed by the two form feeds,
and then the 128 × 64
short integers
in binary format.
For a 3D array of size 128 × 64 × 20
of 32-bit floating point numbers
with the host CPU endianness,
the header is
# AVS field file
ndim=3
dim1=128
dim2=64
dim3=20
nspace=3
veclen=1
data=float
field=uniform
The save
method in this library
writes to the AVS internal format by default,
and the filename must end with the extension .fld
.
AVS external format
Now suppose you have stored the above array data
in a binary file named, say, sino.dat
with some home-brew header in it that consists
of, say, 1999 bytes.
And suppose you do not want to convert from home-brew format
to AVS internal format.
Then you can use the AVS external format
by creating an ASCII file named, say,
sino.fld
containing:
# AVS field file
ndim=2
dim1=128
dim2=64
nspace=2
veclen=1
data=short
field=uniform
variable 1 file=sino.dat filetype=binary skip=1999
You can add additional comments
to these headers
using lines that begin with #
.
The skip=1999
option
indicates that there is a 1999
byte header to be skipped
before reading the binary data.
This format does not allow for additional headers buried within the data.
If there is no binary header,
then you can omit the skip=0
line altogether.
If your data is in ASCII format (hopefully not),
then replace
filetype=binary
with
filetype=ascii
.
However,
for ASCII data,
the skip=
option
refers to ASCII entries, not bytes.
See table below
for supported types in the
data=...
line.
The complete AVS .fld
format
includes other features
that almost certainly are not supported
by this IO library.
This library supports some extensions that are not standard AVS but are very handy, like a single 3D header file that points to multiple 2D files that get treated as a single entity. More documentation coming on request.
Magic bytes
It is convention that an AVS .fld
file begins with
# AVS
in the first line,
as illustrated in the examples above,
so the interface to this library
in
FileIO.jl
uses that 5-byte string
as the
"magic bytes"
or
"magic number"
for this file type.
If you have a file that does not have that string as the start of its header,
then simply add it with an editor
(including a newline at the end).
Data types
The following table shows the supported options
for the data=
field in the header.
The options that end in _le
or _be
or _sun
are "extensions"
designed for portability, because options like int
are not portable between hosts with different
endianness.
format | Julia type | endian | bytes |
---|---|---|---|
byte | UInt8 | n/a | 1 |
short_be | UInt16 | be | 2 |
short_sun | UInt16 | be | 2 |
xdr_short | UInt16 | be | 2 |
short_le | UInt16 | le | 2 |
int | Int32 | ? | 4 |
int_le | Int32 | le | 4 |
int_be | Int32 | be | 4 |
xdr_int | Int32 | be | 4 |
float | Float32 | ? | 4 |
float_le | Float32 | le | 4 |
float_be | Float32 | be | 4 |
xdr_float | Float32 | be | 4 |
double | Float64 | ? | 8 |
double_le | Float64 | le | 8 |
double_be | Float64 | be | 8 |
xdr_double | Float64 | be | 8 |
Entries with ?
are native to the host CPU and thus not portable.
The byte
format is unsigned 8 bits.
The following table shows the saved output data=
field
for various input Julia data fields,
assuming little endian (:le
) default
to AVSfldIO.fld_write
.
Julia type | data | note |
---|---|---|
Bool | byte | |
UInt8 | byte | |
Int16 | short_le | |
Int32 | int_le | |
Int64 | int_le | (downgraded) |
Float16 | float_le | (upgraded) |
Float32 | float_le | |
Float64 | double_le | |
BigFloat | double_le | (downgraded) |
History
The "application visualization system" (AVS) https://www.avs.com was an interactive graphics and computation framework developed in the early 1990s and used widely in the medical imaging community. See the article at https://doi.org/10.1109/38.31462 for an overview.
AVS data files have the extension .fld
and many software frameworks provide file IO support
for this format.
- https://doi.org/10.1109/38.31462
- https://www.ks.uiuc.edu/Research/vmd/plugins/molfile/avsplugin.html
- https://dav.lbl.gov/archive/NERSC/Software/express/help6.1/help/reference/dvmac/Field_Fi.htm
- http://paulbourke.net/dataformats/field/
- http://surferhelp.goldensoftware.com/subsys/subsys_avs_field_file_desc.htm
- https://lanl.github.io/LaGriT/pages/docs/read_avs.html
Tested with latest Julia 1.x
Authors
Jeff Fessler and his group at the University of Michigan, and contributors
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