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.. _SPIDER-PIL:

SPIDER-PIL Spider 2D image
==========================

Extensions: None

*From the Pillow docs:*


PIL reads and writes SPIDER image files of 32-bit floating point data
("F;32F").

PIL also reads SPIDER stack files containing sequences of SPIDER images. The
:py:meth:`~file.seek` and :py:meth:`~file.tell` methods are supported, and
random access is allowed.

The :py:meth:`~PIL.Image.Image.write` method sets the following attributes:

**format**
    Set to ``SPIDER``

**istack**
    Set to 1 if the file is an image stack, else 0.

**nimages**
    Set to the number of images in the stack.

A convenience method, :py:meth:`~PIL.Image.Image.convert2byte`, is provided for
converting floating point data to byte data (mode ``L``)::

    im = Image.open('image001.spi').convert2byte()

Writing files in SPIDER format
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~

The extension of SPIDER files may be any 3 alphanumeric characters. Therefore
the output format must be specified explicitly::

    im.save('newimage.spi', format='SPIDER')

For more information about the SPIDER image processing package, see the
`SPIDER homepage`_ at `Wadsworth Center`_.

.. _SPIDER homepage: https://spider.wadsworth.org/spider_doc/spider/docs/spider.html
.. _Wadsworth Center: https://www.wadsworth.org/

Parameters for reading
----------------------

pilmode : str
    From the Pillow documentation:

    * 'L' (8-bit pixels, grayscale)
    * 'P' (8-bit pixels, mapped to any other mode using a color palette)
    * 'RGB' (3x8-bit pixels, true color)
    * 'RGBA' (4x8-bit pixels, true color with transparency mask)
    * 'CMYK' (4x8-bit pixels, color separation)
    * 'YCbCr' (3x8-bit pixels, color video format)
    * 'I' (32-bit signed integer pixels)
    * 'F' (32-bit floating point pixels)

    PIL also provides limited support for a few special modes, including
    'LA' ('L' with alpha), 'RGBX' (true color with padding) and 'RGBa'
    (true color with premultiplied alpha).

    When translating a color image to grayscale (mode 'L', 'I' or 'F'),
    the library uses the ITU-R 601-2 luma transform::

        L = R * 299/1000 + G * 587/1000 + B * 114/1000
as_gray : bool
    If True, the image is converted using mode 'F'. When `mode` is
    not None and `as_gray` is True, the image is first converted
    according to `mode`, and the result is then "flattened" using
    mode 'F'.

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