The ideas are straightforward; the problem is how these ideas are expressed through various programming APIs.
The cast of characters: space handedness, image coordinate systems
Discrete vs continuous spaces
Domain issues: MRC files
Consider an arbitrary 3D dataset. We rarely think of 3D data apart from some space and the most natural space is the cartesian space consisting of the dimensions x, y and z. This not only takes advantage of our considerable famiarity with the cartesian coordinate system but easily lends itself to both continous and discrete representations: the discrete case would simply involve define evenly spaced voxels between any two physical points.
We need to label the axes of this space. Unfortunately, we have two options: one having z axes jutting out perpendicular to the xy plane in one direction and the other having it jut out in the opposite direction. These two options provide the basis of handedness. Suppose we curl the finger of a hand so that the fingers began in the direction of increasing x then curled inwards towards the origin in the direction of decreasing y (a counterclockwise motion) if the thumb was pointing out of the xy plane (as would occur for the right hand) we call this axes orientation a right hand system. If we only swap the x and y axes then the opposite (a clockwise motion in the plane) with the z axis pointing outward (as would occur for the left hand) would constitute a left hand system.
Any space can only be one of the two: right or left hand.
So far we have taken care of the two most important attributes: orientation (right vs. left handed) and granularity (discrete vs. continuous).
Next, we turn the problem of addressing: how we refer to parts of the space. Again, the most natural way to do this is with the familiar notation of a triple of values. If the space is continuous, (x, y, z) will refer to the value at that point in the space. If the space is discretised then we use the indices (i, j, k). Related to the notion of addressing is the notion of the size of the space. Continous spaces have physical sizes so that the space would be described by a triple of lengths (Lx, Ly, Lz) while discrete spaces would have the number of discretisations in each dimension expressed using familiar triples: (Nx, Ny, Nz). Therefore, when addressing a continous space we would expect the value of x to be found along the length, while for a discrete space the index j would also have to be found along Ny.
Notice that the last sentence is quite vague ("found along"); this is because there is one more aspect of a space that we haven't covered yet: the location of the origin. Having the orientation, granularity and size are not sufficient to locate a space. We need to know where this space sits relative to the origin of the coordinate system.
Again, we have two perspectives to this: the physical origin specifies a linear transform that should be applied to the space to align its local origin to some global origin. If this is (0, 0, 0), then the local and global origins are coincident. If it is some value (Ox, Oy, Oz) then we would need to subtract the corresponding vector to every point in our space to align our space with the global origin.
Additionally, the discrete origin specifies which voxel (volume element) has the index (i=0, j=0, z=0).
For simplicity, most applications will treat both origins as (x=0, y=0, z=0) and (i=0, j=0, k=0) making subsequent operations easy.
With the fundamental properties of spaces out of the way it is now sensible to distinguish between the world and actors. The world is a space which is populated with various objects referred to as actors. Actors placed in the world are located relative to the world (or global) space i.e. coordinate system. Nevertheless, each actor has its own local coordinate system.
Alternatively, we can think of this as spaces interacting with each other.
https://www.mathworks.com/help/images/intro_r_1.png
scikit-image
https://scikit-image.org/docs/stable/user_guide/numpy_images.html
https://itk.org/ItkSoftwareGuide.pdf
mrcfile
https://www.ccpem.ac.uk/mrc_format/mrc2014.php
One of the main sources of confusion arises when images are treated as spaces. Conventionally, the directionality of an image is top-left to bottom-right in much the same way that text flows. This means that the first pixel corresponds to the first word and so on. When an image is treated as a space we have to coincide the image origin with the space origin and the latter wins. Effectively, the first voxel sits at the spatial origin. To add to the confusion, the lack of a handedness of the space means that 'reading direction' is ambiguous; it's bad enough in 2D but catastrophic in 3D. In 2D, we only have two axes so a simple transposition can resolve the issue. This is not the case in 3D as we have a total of six transpositions.
Scientific imaging is not about really about imaging but about spatial measurement. Therefore, every imaging event results in some measurement of some space. Often, this measurement is local so that the spatial origin has no reference to future imaging events. The exception is correlative experiments in which an implied origin is presented in the form of fiducials (chemical or physical) that facilitate registration across imaging events.
The other very confusing aspect of image representation is to say that a 2D RGB image is effectively a 5D image. While this is the case in practice, it is not the case in principal and in software design when taking into account domain matters principal is everything. A 2D RGB image is a vector space not a 5D space! By incorporating the channel information into the spatial information we lose the ability to work with the spatial information as is and likewise for the channel information. It is a poor abstraction.
Related to the above is treating time as an extra dimension. A 3D RGB animation is NOT a 7D image! Again, we lose representational faithful in order to exploit algorithmic convenience.
An image is a pictorial representation disregarding anything about the physical entity it represents. There is no notion of measurement in an image.
A visualisation is the process of converting some measurable entity into an image.
3D objects are characterised by some geometry which may be visualised. A visualisation library performs the task of transforming the geometries present into images for visualisation.
Whenever we assign a physical space to an image we have converted our image into a measurement. While it is the case that we can 'see' the space, its better to think of the pictorial representation as a visualisation of the mesurement given that the physical entity may not be amenable to direct visualisation. For example, cryo-image does not produce images but spatial measurements because they correspond to estimates of electron density in space. While we think of it as microscopy it is not: it is remote sensing since we remotely measure electronic effects produced by the interaction between the specimen and an electron beam or X-ray radiation.
numpy 3D arrays are left-hand oriented: (plane, row, column) means that the first index references the plane (depth); every plane is a 2D image of rows by columns, which is contrary to the image convention of (column, row).
The data stream representing the image information is encoded by an ordering. This ordering describes the directionality with which elements are arranged
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Lesson: It is important to bear in mind that numpy
is agnostic of domain of the application. You are completely at liberty to choose how your data is oriented in space (what the shape of the array means, how the array is oriented in space) as long as you are consistent. In this regard, the manner in which scipy
and scikit-image
have choosen to work with numpy
arrays as image representations is thus an innate design limitation. It seems to me painfully urgent that an intermediary library is needed that combines the needs of imaging workers from Pillow
, scipy
, scikit-image
and many others into one overarching imaging library which has a useful set of imaging domain representations that allows cross-pollination between all these libraries.