based on
DRAFT CBF DEFINITION
by
Andy Hammersley
European Synchrotron Radiation Facility, BP 200, Grenoble, 38043, CEDEX, France
hammersley@esrf.fr
This is a version of the CBF draft proposal, revised to include a coordinated pure ASCII ImgCIF definition, based on the Draft CBF Definition by Andy Hammersley, the work done at the Brookhaven imgCIF workshop, and the work on "CBFLIB: An ANSI-C API for Crystallographic Binary File" by Paul Ellis, ellis@SSRL.SLAC.STANFORD.EDU. For the binary CBF format, a "binary-string" approach, as proposed by Paul Ellis, is used, while for the ASCII imgCIF format, binary information is encoded using a variant on MIME (Multipurpose Internet Mail Extensions) format, which makes the CBF and ImgCIF formats very similar.
We have included an updated version of John Westbrook's DDL2-compliant CBF Extensions Dictionary, of Paul Ellis's CBFLIB manual, and examples of CBF/imgCIF files.
This is just a proposal. My apologies in advance, especially to Andy, John and especially to Paul for whatever I may have muddled here. Please be careful about basing any code on this until and unless there has been a general agreement.
Most of this document is adapted from Andy's, so we follow his convention by "...[separating] the definition from comments on discussion items by using round brackets to refer to notes kept separate from the main text e.g. (1) refers to point 1 in the notes section.". We have integrated all comments to date into this document without special annotation.
Note:
The initial aim is to support efficient storage of raw experimental data from area-detectors (images) with no loss of information compared to existing formats. The format should be both efficient in terms of writing and reading speeds, and in terms of stored file sizes, and should be simple enough to be easily coded, or ported to new computer systems.
Flexibility and extensibility are required, and later the storage of other forms of data may be added without affecting the present definitions.
The aims are achieved by a simple file format, consisting of lines of ASCII information defining information about the binary data as CIF tag-value pairs and tables, and either raw octets of binary data in delimited sections, or ASCII-based presentations of the same binary information in similarly delimited sections.
The present version of the format only tries to deal with simple Cartesian data. This is essentially the "raw" data from detectors that is typically stored in commercial formats or individual formats internal to particular institutes, but could be other forms of data. It is hoped that CBF can replace individual laboratory or institute formats for "home" built detector systems, be used as a inter-program data exchange format, and may be offered as an output choice by a number of commercial detector manufacturers specialising in X-ray and other detector systems.
This format does not imply any particular demands on processing software nor on the manner in which such software should work. Definitions of units, coordinate systems, etc. may quite different. The clear precise definitions within CIF, and hence CBF, help, when necessary, to convert from one system to another. Whilst no strict demands are made, it is clearly to be hoped that software will make as much use as is reasonable of information relevant to the processing which is stored within the file. It is expected that processing software will give clear and informative error messages when they encounter problems within CBF's or do not support necessary mechanisms for inputting a file.
imgCIF is also the name of the CIF dictionary which contains the terms specific to describing the binary data (the orginal, designed by John Westbrook, without the modifications in this proposal is avaliable from http://ndbserver.rutgers.edu/NDB/mmcif. Thus a CBF or ImgCIF files uses data names from the imgCIF dictionary and other CIF dictionaries.
The example is an image of 768 by 512 pixels stored as 16 bit unsigned integers, in little endian byte order. (This is the native byte ordering on a PC.) The pixel sizes are 100.5 by 99.5 microns. Comment lines starting with a hash sign (#) are used to explain the contents of the header. Only the ASCII part of the file is shown, but comments are used to describe the start of the binary section.
First the file is shown with the minimum of comments that a typical outputting program might add. Then it is repeated, but with "over- commenting" to explain the format.
Here is how a file might appear if listed on a PC or on a Unix system using "more":
###CBF: VERSION 0.6 # Data block for image 1 data_image_1 _entry.id 'image_1' # Sample details _chemical.entry_id 'image_1' _chemical.name_common 'Protein X' # Experimental details _exptl_crystal.id 'CX-1A' _exptl_crystal.colour 'pale yellow' _diffrn.id DS1 _diffrn.crystal_id 'CX-1A' _diffrn_measurement.diffrn_id DS1 _diffrn_measurement.method Oscillation _diffrn_measurement.sample_detector_distance 0.15 _diffrn_radiation_wavelength.id L1 _diffrn_radiation_wavelength.wavelength 0.7653 _diffrn_radiation_wavelength.wt 1.0 _diffrn_radiation.diffrn_id DS1 _diffrn_radiation.wavelength_id L1 _diffrn_source.diffrn_id DS1 _diffrn_source.source synchrotron _diffrn_source.type 'ESRF BM-14' _diffrn_detector.diffrn_id DS1 _diffrn_detector.id ESRFCCD1 _diffrn_detector.detector CCD _diffrn_detector.type 'ESRF Be XRII/CCD' _diffrn_detector_element.id 1 _diffrn_detector_element.detector_id ESRFCCD1 _diffrn_frame_data.id F1 _diffrn_frame_data.detector_element_id 1 _diffrn_frame_data.array_id 'image_1' _diffrn_frame_data.binary_id 1 # Define image storage mechanism # loop_ _array_structure.id _array_structure.encoding_type _array_structure.compression_type _array_structure.byte_order image_1 "unsigned 16-bit integer" none little_endian loop_ _array_intensities.array_id _array_intensities.binary_id _array_intensities.linearity _array_intensities.undefined_value _array_intensities.overload_value image_1 1 linear 0 65535 # Define dimensionality and element rastering loop_ _array_structure_list.array_id _array_structure_list.index _array_structure_list.dimension _array_structure_list.precedence _array_structure_list.direction image_1 1 768 1 increasing image_1 2 512 2 decreasing loop_ _array_element_size.array_id _array_element_size.index _array_element_size.size image_1 1 100.5e-6 image_1 2 99.5e-6 loop_ _array_data.array_id _array_data.binary_id _array_data.data image_1 1 ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-Size: 374578 X-Binary-ID: 1 X-Binary-Element-Type: "unsigned 16-bit integer" Content-MD5: jGmkxiOetd9T/Np4NufAmA== START_OF_BIN *************'9*****`********* ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ;Here the file is shown again, but this time with many comment lines added to explain the format:
###CBF: VERSION 0.6 # This line starting with a "#" is a CIF and CBF comment line, # but the first line with the three "#"s is a CBF identifier. # (a "magic number") The text "###_CBF: VERSION" identifies # the file as a CBF and must be present as the very first line of # every CBF file. Following "VERSION" is the version number of # the file, which is the corresponding version of the CBF/imgCIF # extensions dictionary and supporting documentation. A version # 0.6 CIF should be readable by any program which fully supports # the version 1.0 CBF definitions. # Comment lines and white space (blanks and new lines) may appear # anywhere outside the binary sections. # In a CIF, the descriptive tags and values may be presented in # any convenient order, e.g. the data could come first, and the # parameters necessary to interpret the data could come later. # This order-independent convention holds for an imgCIF file, but # for a CBF, all the tags and values describing binary data (i.e. # all the tags other than those in the ARRAY_DATA category) should # be presented before the binary data, in the form of a header. # This does not mean that there cannot be more useful information # after the binary data. There could be another full header and # more blocks of binary data. All we are saying is that, in # the interest of efficiency in processing a CBF, the parameters # that relate to a particular block of binary data must appear # earlier in the CBF than the block itself. # The header begins with "data_", which is the CIF token to # identify a data block. Within a data block, any given tag may # be presented only once, either directly with an immediately # following value, or as one of the column headings for the rows # of a table. If you will need to resuse the same tag, you will # have to start a new data block. # Data block for image 1 data_image_1 # We've chosen to call this data block 'image_1', but this was an # arbitary choice. Within a data block a data item may only be used # once. _entry.id 'image_1' # Sample details _chemical.entry_id 'image_1' _chemical.name_common 'Protein X' # The apostrophes enclose the string which contains a space. # A double quote (") could have been used, just as well. # There is also a third way to quote string, with the string # "\n;", i.e. with a semicolon at the beginning of a line # which allows multi-lined strings to be presented. We'll # use that form of text quotation for the binary data. # Experimental details _exptl_crystal.id 'CX-1A' _exptl_crystal.colour 'pale yellow' _diffrn.id DS1 _diffrn.crystal_id 'CX-1A' _diffrn_measurement.diffrn_id DS1 _diffrn_measurement.method Oscillation _diffrn_measurement.sample_detector_distance 0.15 _diffrn_radiation_wavelength.id L1 _diffrn_radiation_wavelength.wavelength 0.7653 _diffrn_radiation_wavelength.wt 1.0 _diffrn_radiation.diffrn_id DS1 _diffrn_radiation.wavelength_id L1 _diffrn_source.diffrn_id DS1 _diffrn_source.source synchrotron _diffrn_source.type 'ESRF BM-14' _diffrn_detector.diffrn_id DS1 _diffrn_detector.id ESRFCCD1 _diffrn_detector.detector CCD _diffrn_detector.type 'ESRF Be XRII/CCD' _diffrn_detector_element.id 1 _diffrn_detector_element.detector_id ESRFCCD1 _diffrn_frame_data.id F1 _diffrn_frame_data.detector_element_id 1 _diffrn_frame_data.array_id 'image_1' _diffrn_frame_data.binary_id 1 # Many more data items can be defined, but the above gives the idea # of a useful minimum set (but not minimum in the sense of # compulsory, the above data items are optional in a CIF or CBF). # Define image storage mechanism # # Notice that we did not include a binary ID here. The idea of # the ARRAY_STRUCTURE category is to present parameters which # could be common to multiple blocks of binary data, which would # all have the same array ID, but would have distinct binary ID's loop_ _array_structure.id _array_structure.encoding_type _array_structure.compression_type _array_structure.byte_order image_1 "unsigned 16-bit integer" none little_endian # On the other hand, we do provide a binary ID for ARRAY_INTENSITIES, # since there might be different paremeters for each binary block. # We could have left it out here, since there is only one block and # the default binary ID happens to be 1 loop_ _array_intensities.array_id _array_intensities.binary_id _array_intensities.linearity _array_intensities.undefined_value _array_intensities.overload_value image_1 1 linear 0 65535 # Define dimensionality and element rastering # Here the size of the image and the ordering (rastering) of the data # elements is defined. The CIF "loop_" structure is used to # define different dimensions. (It can be used for defining multiple # images.) loop_ _array_structure_list.array_id _array_structure_list.index _array_structure_list.dimension _array_structure_list.precedence _array_structure_list.direction image_1 1 768 1 increasing image_1 2 512 2 decreasing loop_ _array_element_size.array_id _array_element_size.index _array_element_size.size image_1 1 100.5e-6 image_1 2 99.5e-6 # The "array_id" identifies data items belong to the same array. # Here we have chosen the name "image_1", but another name could # have been used, so long as it's used consistently. The "index" # component refers to the dimension being defined, and the # "dimension" component defines the number of elements in that # dimension. The "precedence" component defines which precedence # of rastering of the data. In this case the first dimension is the faster # changing dimension. The "direction" component tells us the # direction in which the data rasters within a dimension. Here the # data rasters faster from minimum elements towards the maximum # element ("increasing") in the first dimension, and more # slowly from the maximum element towards the minimum element in # the second dimension. (This is the default rastering order.) # The storage of the binary data is now fully defined. # Further data items could be defined, but we are ready to # present the data. That is done with the ARRAY_DATA category. # The start of this category marks the end of the header # (Well, almost the end, there is a bit more header information # below). loop_ _array_data.array_id _array_data.binary_id _array_data.data image_1 1 # The binary data itself will come just a little further down, # as the essential part of the value of _array_data.data, which # begins as semicolon-quoted text. The line immediately after # the line with the semicolon is a MIME boundary marker. As for # all MIME boundary markers, it begins with "--". The next # few lines are MIME headers, describing some useful information # we will need to process the binary section. MIME headers can # appear in different orders, and can be very confusing (look # at the raw contents of a email message with attachments), but # there is only a few headers which is have to be understood to # process a CBF: # # The "Content-Type" header may be any of discrete types # permitted in RFC 2045; "application/octet-stream" is # recommended. If an octet stream was compressed, the # compression should be specified by the parameter # 'conversions="x-CBF_PACKED"' or by specifying # one of the other compression types. # # The "Content-Transfer-Encoding" header should be 'BINARY' # for a CBF. We'll consider the other values used for imgCIF # below. # # The "X-Binary-Size" header specifies the size of the # binary data in octets. If compression was used, this size # is the size after compression, including any book-keeping # fields, but not the 8 bytes for the compression type. # # The "X-Binary-Element-Type" header specifies the # type of binary data in the octets, using the same # descriptive phrases as in _array_structure.encoding_type. # The default value is "unsigned 32-bit integer". # # The MIME header items are followed by an empty line and then by # a special sequence marked here as 'START_OF_BIN', consisting of # Control-L, Control-Z, Control-D to stop printing on most systems, # and then a single binary flag character of hexadecimal value D5 # (213 decimal). The binary data follows immediately after this # flag character. # ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-Size: 374578 X-Binary-ID: 1 X-Binary-Element-Type: "unsigned 16-bit integer" Content-MD5: jGmkxkrpnizOetd9T/Np4NufAmA== START_OF_BIN *************'9*****`********* ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; # After the last octet (i.e. byte) of the binary data, there is a # special trailer "\n--CIF-BINARY-FORMAT-SECTION----\n;" # which repeats the initial bounday marker with an extra "--" # at the end (a MIME convention for the last boundary marker), and # then the closing semicolon quote for a text section. This # is essential in an imgCIF, and we include it in a CBF for # consistency.
###CBF: VERSIONwhich must always be present so that a program can easily identify whether or not a file is a CBF, by simply inputting the first 15 characters. (The space is a blank (ASCII 32) and not a tab. All identifier characters are uppercase only.)
The first hash means that this line within a CIF would be a comment line, but the three hashes mean that this is a line describing the binary file layout for CBF. (All CBF internal identifiers start with the three hashes, and all other must immediately follow a "line separator".) No whitespace may precede the first hash sign.
Following the file identifier is the version number of the file. e.g. the full line might appear as:
###CBF: VERSION 0.6The version number must be separated from the file identifier characters by whitespace e.g. a blank (ASCII 32).
The version number is defined as a major version number and minor version number separated by the decimal point. A change in the major version may well mean that a program for the previous version cannot input the new version as some major change has occurred to CBF (3). A change in the minor version may also mean incompatibility, if the CBF has been written using some new feature. e.g. a new form of linearity scaling may be specified and this would be considered a minor version change. A file containing the new feature would not be readable by a program supporting only an older version of the format.
Note: Until we reach major version 1 (the first official release), the rules are a little more relaxed. While there will be some effort at upwards compatability, in order to ensure a reasonable agreed specification without too many strange artifacts, changes between minor versions may, unfortunately, introduce incompatabilities which require program changes to still read CBFs compliant with an earlier draft, e.g. the change in the "magic number" and from binary sections to binary strings in going to version 0.3, and a removal of the redundant parts of the binary header in going to version 0.6. Naturally, such changes should be sufficiently well documented to allow for conversions.>>>
###_START_OF_HEADERmay be used before the "data_" taken, followed by the carriage return, line-feed pair, as an aid in debugging, but it is no longer required. (Naturally, another carriage return, line-feed pair should immediately precedes this and all other CBF identifiers, with the exception of the CBF file identifier which is at the very start of the file.)
e.g.
Any CIF data name may occur within the header section.
###_END_OF_HEADERfollowed by carriage return, line-feed, may be used as well as an aid to debugging, but it is not required.
Note: Under CBFlib "binary sections" have been replaced by "binary strings" values within a data name/value pair. The structure of the proposed "binary string" is similar to the former binary sections, but there are significant differences.
--CIF-BINARY-FORMAT-SECTION--
at the beginning of a line. The initial "--" says that
this is a MIME boundary. We cannot put "###" in front
of it and conform to MIME conventions. Immediately after the boundary
marker are MIME headers, describing some useful information
we will need to process the binary section. MIME headers can
appear in different orders, and can be very confusing (look
at the raw contents of a email message with attachments), but there
is only a few headers with a narrow range of values which is have
to be understood to process a CBF (as opposed of an imgCIF, for which the
headers can be more varied):
In general, if the value given for "Content-Transfer-Encoding" is one of the
real encodings: "BASE64", "QUOTED-PRINTABLE", "X-BASE8",
"X-BASE10" or "X-BASE16", this file is an imgCIF.
For either a CBF or an imgCIF the optional "Content-MD5" header provides a much more sophisticated check on the integrity of the binary data.
In a CBF, the raw binary data begins after an empty line terminating
the MIME headers and after the START_OF_BIN identifier.
"START_OF_BIN" contains bytes to separate the "ASCII" lines
from the binary data, bytes to try to stop the listing of the header,
bytes which define the binary identifier which should match the
"binary_id" defined in the header, and bytes which define the
length of the binary section.
Octet | Hex | Decimal | Purpose |
---|---|---|---|
1 | 0C | 12 | (ctrl-L) End the current page |
2 | 1A | 26 | (ctrl-Z) Stop listings in MS-DOS |
3 | 04 | 04 | (Ctrl-D) Stop listings in UNIX |
4 | D5 | 213 | Binary section begins |
5..5+n-1 | Binary data (n octets) |
Only bytes 5..5+n-1 are encoded for an imgCIF file
using the indicated Content-Transfer-Encoding.
Note: Earlier versions of the specification included three 8-byte words of information in binary which replicated information now available in the MIME header:
5..12 | Binary Section Identifier (See _array_data.binary_id) 64-bit, little endian | ||||||||||
13..20 | the size (n) of the binary section in octets (i.e. the offset from octet 29 to the first byte following the data) | ||||||||||
21..28 | Compression type:
|
The binary characters serve specific purposes:
--CIF-BINARY-FORMAT-SECTION--
;
with each of these lines followed by the carriage return / line feed pair.
This brings us back into a normal CIF environment
The first "line separator" separates the binary data from the
pseudo-ASCII line.
This identifier is in a sense redundant since the binary data
length value tells the a program how many bytes to jump over to
the end of the binary data. However, this redundancy has been
deliberately added for error checking, and for possible file
recovery in the case of a corrupted file.
This identifier must be present at the end of every block of
binary data.
However, in general no guarantee is made of block nor word alignment
in a CBF of unknown origin.
###_END_OF_CBF
(including the carriage return, line-feed pair) can help in debugging.
The binary identifier values used within a given data block section, and
hence the binary data must be unique for any
given array_id, and, it would be best to make them truly unique.
A different data block may reuse binary identifier values.
(This allows concatenation of files without re-numbering the
binary identifiers, and provides a certain level of localization
of data within the file, to avoid programs having to search
potentially huge files for missing binary sections.)
Here only the ASCII part of the file structuring identifiers is shown. The CIF data items are not shown, apart from the "data_" identifier which indicates the beginning of a data block.
This shows the structuring of a simple example e.g. one header section followed by one binary section. Such as could be used to store a single image.
###CBF: VERSION 0.3 data_ ### ... various CIF tags and values here loop_ array_data.id array_data.binary_id array_data.data image_1 1 ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-ID: 1 Content-MD5: jGmkxiOetd9T/Np4NufAmA== START_OF_BIN *************'9*****`********* ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; ###_END_OF_CBF
Here only the ASCII part of the file structuring identifiers is shown. The CIF data items are not shown, apart from the "data_" identifier which indicates the beginning of a data block.
This shows the a possible structuring of a more complicated example. Two header sections, the first contains two data blocks and defines three binary sections. CIF comment lines, starting with a hash (#) are used to example the structure.
###CBF: VERSION 0.6 # CBF file written by cbflib v0.6 # A comment cannot appear before the file identifier, but can appear # anywhere else, except within the binary sections. # Here the first data block starts data_ ### ... various CIF tags and values here ### but none that define array data items # The "data_" identifier finishes the first data block and starts the # second data_ ### ... various CIF tags and values here ### including ones that define array data items loop_ array_data.array_id array_data.binary_id array_data.data image_1 1 ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-Size: 3745758 X-Binary-ID: 1 X-Binary-Element-Type: "signed 32-bit integer" Content-MD5: 1zsJjWPfol2GYl2V+QSXrw== START_OF_BIN <D5>^P<B8>P^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@ ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; # Following the "end of binary" identifier the file is pseudo-ASCII # again, so comments are valid up to the next "start of binary" # identifier. Note that we have bumped the binary ID. image_1 2 ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-Size: 3745758 X-Binary-ID: 2 X-Binary-Element-Type: "signed 32-bit integer" Content-MD5: xR5kxiOetd9T/Nr5vMfAmA== START_OF_BIN <D5>^P<B8>P^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@^@ ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; # Third binary section, note that we have a new array id. image_2 3 ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-ID: 3 Content-MD5: yS5kxiOetd9T/NrqTLfAmA== START_OF_BIN *************'9*****`********* ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; # Second Header section data_ ### ... various CIF tags and values here ### including ones that define array data items # Since we only have one block left, we won't use a loop array_data.id image array_data.binary_id 1 array_data.data # Note that I can put a comment here ; --CIF-BINARY-FORMAT-SECTION-- Content-Type: application/octet-stream; conversions="x-CBF_PACKED" Content-Transfer-Encoding: BINARY X-Binary-ID: 1 Content-MD5: fooxiOetd9T/serNufAmA== START_OF_BIN *************'9*****`********* ... [This is where the raw binary data would be -- we can't print it here] --CIF-BINARY-FORMAT-SECTION---- ; ###_END_OF_CBF
The _array_* categories cover all data names concerned with the storage of images or regular array data.
Data names from any of the existing categories may be relevant as auxiliary information in the header section, but data names from the _diffrn_ category, are likely to be the most relevant, and a number of new data names in this category are necessary.
The "array" class is defined by data names from the ARRAY_STRUCTURE and ARRAY_STRUCTURE_LIST categories.
Here is a short summary of the data names and their purposes.
e.g. "unsigned_16_bit_integer" is used if the stored image was 16 bit unsigned integer values, regardless of any compression scheme used.
Fundamental to treating a long line of data values as a 2-D image or an N-dimensional volume or hyper-volume is the knowledge of the manner in which the values need to be wrapped. For the raster orientation to be meaningful we define the sense of the view:
For a detector image the sense of the view is defined as that looking from the crystal towards the detector.
(For the present we consider only an equatorial plane geometry, with 2-theta = 0; the detector as being vertically mounted.)
The rastering is defined by the three data names _array_structure_list.index, _array_structure_list.precedence, and _array_structure_list.direction data names.
index refers to the dimension index i.e. In an image 1 refers to the X-direction (horizontal), 2 refers to the Y-direction (vertical).
precedence refers to the order in which the data in wrapped.
direction refers the direction of the rastering for that index.
We define a preferred rastering orientation, which is the default if the keyword is not defined. This is with the start in the upper-left-hand corner and the fastest changing direction for the rastering horizontally, and the slower change from top to bottom.
(Note: With off-line scanners the rastering type depending on which way round the imaging plate or film is entered into the scanner. Care may need to be taken to make this consistent.)
# Define image size and rastering loop_ _array_structure_list.array_id _array_structure_list.index _array_structure_list.dimension _array_structure_list.precedence _array_structure_list.direction image_1 1 1300 1 increasing image_1 2 1200 2 decreasingTo define two arrays, the first a volume of 100 times 100 times 50 elements, fastest changing in the first dimension, from left to right, changing from bottom to top in the second dimension, and slowest changing in the third dimension from front to back; the second an image of 1024 times 1280 pixels, with the second dimension changing fastest from top to bottom, and the first dimension changing slower from left to right; the following header section might be used:
# Define array sizes and rasterings loop_ _array_structure_list.array_id _array_structure_list.index _array_structure_list.dimension _array_structure.precedence _array_structure.direction volume_a 1 100 1 increasing volume_a 2 100 2 increasing volume_a 3 50 3 increasing slice_1 1 1024 2 increasing slice_1 2 1280 1 decreasing
Existing data storage formats use a wide variety of methods for storing physical intensities as element values. The simplest is a linear relationship, but square root and logarithm scaling methods have attractions and are used. Additionally some formats use a lower dynamic range to store the vast majority of element values, and use some other mechanism to store the elements which over-flow this limited dynamic range. The problem of limited dynamic range storage is solved by the data compression methods byte_offsets and predictor_huffman (see next Section), but the possibility of defining non-linear scaling must also be provided.
The _array_intensities.linearity data item specifies how the intensity scaling is defined. Apart from linear scaling, which is specified by the value linear, two other methods are available to specify the scaling.
One is to refer to the detector system, and then knowledge of the manufacturers method will either be known or not by a program. This has the advantage that any system can be easily accommodated, but requires external knowledge of the scaling system.
The recommended alternative is to define a number of standard intensity linearity scaling methods, with additional data items when needed. A number of standard methods are defined by _array_intensities.linearity values: offset, scaling_offset, sqrt_scaled, and logarithmic_scaled. The "offset" methods require the data item _array_intensities.offset to be defined, and the "scaling" methods require the data item _array_intensities.scaling to be defined. The above scaling methods allow the element values to be converted to a linear scale, but do not necessarily relate the linear intensities to physical units. When appropriate the data item _array_intensities.gain can be defined. Dividing the linearized intensities by the value of _array_intensities.gain should produce counts. Two special optional data flag values may be defined which both refer to the values of the "raw" stored intensities in the file (after decompression if necessary), and not to the linearized scaled values. _array_intensities.undefined_value specifies a value which indicates that the element value is not known. This may be due to data missing e.g. a circular image stored in a square array, or where the data values are flagged as missing e.g. behind a beam-stop. _array_intensities.overload_value indicates the intensity value at which and above, values are considered unreliable. This is usually due to saturation.
# Define image intensity scaling loop_ _array_intensities.array_id _array_intensities.binary_id _array_intensities.linearity _array_intensities.gain _array_intensities.undefined_value _array_intensities.overload_value image_1 1 linear 1.2 0 65535
In CBFlib version 0.1, Paul Ellis has coded two lossless compression algorithms: canonical and packed.
The canonical-code compression scheme encodes errors in two ways: directly or indirectly. Errors are coded directly using a symbol corresponding to the error value. Errors are coded indirectly using a symbol for the number of bits in the (signed) error, followed by the error iteslf.
At the start of the compression, CBFLIB constructs a table containing a set of symbols, one for each of the 2^n direct codes from -(2^(n-1)) .. 2^(n-1) -1, one for a stop code, and one for each of the maxbits -n indirect codes, where n is chosen at compress time and maxbits is the maximum number of bits in an error. CBFLIB then assigns to each symbol a bit-code, using a shorter bit code for the more common symbols and a longer bit code for the less common symbols. The bit-code lengths are calculated using a Huffman-type algorithm, and the actual bit-codes are constructed using the canonical-code algorithm described by Moffat, et al. (International Journal of High Speed Electronics and Systems, Vol 8, No 1 (1997) 179-231).
The structure of the compressed data is:
Byte | Value |
---|---|
1 .. 8 | Number of elements (64-bit little-endian number) |
9 .. 16 | Minimum element |
17 .. 24 | Maximum element |
25 .. 32 | Repeat length (currently unused) |
33 | Number of bits directly coded, n |
34 | Maximum number of bits encoded, maxbits |
35 .. 35+2^n-1 | Number of bits in each direct code |
35+2^n | Number of bits in the stop code |
35+2^n+1 .. 35+2^n+maxbits-n | Number of bits in each indirect code |
35+2^n+maxbits-n+1 .. | Coded data |
The CCP4-style compression writes the errors in blocks . Each block begins with a
6-bit code. The number of errors in the block is 2^n,
where n
is the value in bits 0 .. 2.
Bits 3 .. 5 encode the number of bits in each error:
Value in bits 3 .. 5 |
Number of bits in each error |
---|---|
0 | 0 |
1 | 4 |
2 | 5 |
3 | 6 |
4 | 7 |
5 | 8 |
6 | 16 |
7 | 65 |
Byte | Value |
---|---|
1 .. 8 | Number of elements (64-bit little-endian number) |
9 .. 16 | Minumum element (currently unused) |
17 .. 24 | Maximum element (currently unused) |
25 .. 32 | Repeat length (used, starting with version 0.2) |
33 .. | Coded data |
In addition, Andy Hammersley has proposed two types of lossless data compression algorithms for CBF version 1.0. In later versions other types including lossy algorithms may be added.
The first algorithm is referred to as byte_offsets and has been chosen for the following characteristics: it is very simple, may be easily implemented, and can easily lead to faster reading and writing to hard disk as the arithmetic complication is very small. This algorithm can never achieve better than a factor of two compression relative to 16-bit raw data, but for most diffraction data the compression will indeed be very close to a factor 2.
The second algorithm is referred to as predictor_huffman and has been chosen as it can achieve close to optimum compression on typical diffraction patterns, with a relatively fast algorithm, whilst avoiding patent problems and licensing fees. This will typically provide a compression ratio between 2.5 and 3 on well exposed diffraction images, and will achieve greater ratios on more weakly exposed data e.g. 4 - 5 on "thin phi-slicing" images. Normally, this would be a two pass algorithm; 1st pass to define symbol probabilities; second pass to entropy encode the data symbols. However, the Huffman algorithm makes it possible to use a fixed table of symbol codes, so faster single pass compression may be implemented with a small loss in compression ratio. With very fast cpus this approach may provide faster hard disk reading and writing than the "byte_offsets" algorithm owing to the smaller amounts of data to be stored.
There are practical disadvantages to data compression: the value of a particular element cannot be obtained without calculating the values of all previous elements, and there is no simple relationship between element position and stored bytes. If generally the whole array is required this disadvantage does not apply. These disadvantages can be reduced by compressing separately different regions of the arrays, which is an approach available in TIFF, but this adds to the complexity reading and writing images.
For simple predictor algorithms such as the byte_offsets algorithm a simple alternative is an optional data item, which defines a look-up table of element addresses, values, and byte positions within the compressed data, and it is suggested that this approach is followed.
The algorithm works because of the following property of almost all diffraction data and much other image data: The value of one element tends to be close to the value of the adjacent elements, and the vast majority of the differences use little of the full dynamic range. However, noise in experimental data means that run-length encoding is not useful (unless the image is separated into different bit-planes). If a variable length code is used to store the differences, with the number of bits used being inversely proportional to the probability of occurrence, then compression ratios of 2.5 to 3.0 may be achieved. However, the optimum encoding becomes dependent of the exact properties of the image, and in particular on the noise. Here a lower compression ratio is achieved, but the resulting algorithm is much simpler and more robust.
The byte_offsets algorithm is the following:
It may be noted that one element value may require up to 7 bytes for storage, however for almost all 16-bit experimental data the vast majority of element values will be within +-127 units of the previous element and so only require 1 byte for storage and a compression factor of close to 2 is achieved.
9.0 REFERENCES
1. S R Hall, F H Allen, and I D Brown, "The Crystallographic Information
File (CIF): a New Standard Archive File for Crystallography",
Acta Cryst., A47, 655-685 (1991)
(1) A pure ASCII CIF based format has been considered inappropriate given the
enormous size of many raw experimental data-sets and the desire for
efficient storage, and reading and writing.
However, an ASCII format is helpful for debugging software and
in understanding what has been written in a CBF when problems
arise, and there are other CIF application for which a convenience
binary format should be useful (e.g. illustrations in
a manuscript).
(2) Some simple method of checking whether the file is a CBF or not is
needed. Ideally this would be right at the start of the file. Thus, a
program only needs to read in n bytes and should then know immediately
if the file is of the right type or not. Andy though this identifier should
be some straightforward and clear ASCII string.
With the use of binary strings and MIME conventions identification of
a CBF versus a CIF is less critical than it was before, but the distinct
header as a simple ASCII string is still a good idea for the sake of the most efficient processing
of large files.
The underscore character has been used to avoid any ambiguity in the
spaces.
(Such an identifier should be long enough that it is highly unlikely to
occur randomly, and if it is ASCII text, should be very slightly
obscure, again to reduce the chances that it is found accidently. Hence
I added the three hashes, but some other form may be equally valid.)
(3) The format should maintain backward compatibility e.g. a version 1.0
file can be read in by a version 1.1, 3.0, etc. program, but to allow
future extensions the reverse cannot be guaranteed to be true.
However, prior to actual adoption of version 1.0, we are not
yet trying to ensure full upwards compatibility, just that the effort to
convert won't be unreasonable.
Examples of CBF and imgCIF Files
by Herbert J. Bernstein (email:
yaya@bernstein-plus-sons.com),
based on the 14 November 1998 and 8 July 1998 versions and the
page produced by Andy Hammersley (E-mail: hammersley@esrf.fr).