Comments (4)
The management of the different signals is taken care by the workflow: the python script or the notebook.
In the case of the navigator, it would be worth considering improving support signal navigator if this is thought in a generic fashion and in a way that it doesn't too much burden to other functions. Maybe it is worth continuing this part of the discussion at hyperspy/hyperspy#2639?
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So you mean I should stick to keeping track of the changes in the navigation axis of the cl
signal and manually applying the same changes to the s
SE image file?
That's what I am doing, but I still think there must be a better way...
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@jordiferrero - I understand your point. In principle it applies also for EELS and EDX data and might be of more general interest. Though in many cases the spectral maps will have a lower resolution than proper HAADF or SE images of the same region, and a direct linking of this data is of limited value.
For example, our CL system does not record the SE signal in parallel. I usually have a corresponding SE image taken beforehand and the spectral image corresponds to only a ROI on that image. That SE image usually has a better resolution than the spectral image as I hardly ever use step sizes below 20 nm.
The main issue I see with your approach is that quite a number of functions would need to be adapted directly in hyperspy (e.g. crop
, inav
, rebin
). What you want to do is basically stacking of signals. But I am not sure if stacking two signals with the same navigation dimensions, but different signal dimensions (e.g. 1024 and 1) is possible @ericpre, I do not have enough experience with that function. It might be worth thinking along the lines of adding such a functionality instead of adding an additional signal to the metadata.
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Indeed, there is room for improvement for the navigator and it would good to discuss how to improve it with others who are interested in this and this is why I put the link to the other issue!
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Related Issues (20)
- Docstring formatting in RTD HOT 11
- Transient signal classes HOT 3
- LumiSpy v0.2 HOT 2
- Create a `remove_background_signal` function HOT 1
- Extend functionality of crop_edges HOT 3
- Implementation of Spectroscopy File Readers HOT 18
- Increase coverage HOT 2
- Webhook failing HOT 3
- Adding an interactive way to slice HS over a wavelength range, and view the result spatially! HOT 12
- Consolidate axis conversion codes
- Failure with numpy 1.24.dev
- Slicing of energy/wavenumber signal with isig fails
- Failure with numpy dev HOT 1
- Documentation is broken HOT 3
- Azure tests failing HOT 2
- Find maximum and width of a peak HOT 1
- Reminder: Change doc-links to sphinx
- Fix test for `remove_spikes` HOT 4
- Slicing TransientSpec HOT 22
- `to_eV()` function and non-uniform axis HOT 1
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