Creating Optics Groups from EPU AFIS data and more

So you recently used “Faster Acquisition” in EPU for your session, and you also want to try the newest features in RELION which allow you to correct for higher-order aberrations and anisotropic magnification. However, you quickly see this requires you to sort the data into “Optics Groups” before you begin processing. From the publication:

[…] in RELION-3.1. To facilitate this, we have introduced the concept of optics groups : partitions of the particle set that share the same optical properties, such as the voltage or pixel size (or the aberrations and the magnification matrix).

So the question becomes "How do I sort my AFIS data into Optics Groups?"

However if you want to know a bit more of how we got here you can keep reading.


Purpose

Traditionally SPA data is collected using the stage to move from hole to hole. This is because the alternative would be to use what is called beam-image shift, which for high-resolution TEM work was non-ideal.

The reason for why this is can be largely considered as two-fold:

  1. Off-axis use of the objective lens
  2. Coma and astigmatism due to beam-tilt

Off-axis collection

The ray diagram of a hole exposed using beam-image shift looks something like this:
lowdose

What you will notice is the beam does not go through the center of the objective lens, but “off-axis” to it. There is a common phrase that EM-lenses are equivalent to using the bottom of a Coca-Cola bottle for your microscope. This is not really the case anymore, but what is true is that EM-lenses are plagued by strong aberrations and we must take care to minimize these.

Spherical aberration (C_s) is a particularly strong defect in EM-lenses and it reduces the spatial coherence of our imaging system. We do all sorts of things to reduce the effects of Spherical aberration which range from the simple use of a small condenser aperture, to the exorbitantly expensive half-meter tall C_s-correctors installed on several Krioses around the world. Only the central tens of microns of an EM-lens is truly usable for focusing electrons, and the performance degrades extremely quickly as we move away from the optical axis of the objective lens, which is the most important and the strongest lens in the microscope.

From the ray diagram we see the displacement away from the optical axis entering the upper-objective. We can also see that the half-angle of collection exiting the lower-objective is much greater. This greatly decreases our resolution as showed in the figure below from source:

We see that the finite size of our source is governed by the cube of the angle, not good at all! In addition above we can see again how the effects of the spherical aberration increase as we move out from the lens center.

All of this together show why for so long we have always collected our micrographs “on-axis”, and limited exposures collected with beam-image shift to low-dose focusing and tracking images. Beam-image shift, unfortunately in my case, is often used in tomography data where we need to collect off-axis to align the offset between tilt-axis and the center of the detector.

Beam-tilt induced coma and astigmatism

The stronger error-inducing artifact of beam-image shift use is that it introduces both coma and astigmatism into our imaging system. While astigmatism is no longer the issue it had been previously, improvement in detectors increased the signal-to-noise ratio of diffractograms (2-D power spectra of micrographs that we use for CTF-fitting) allowing for more accurate measurements, Coma is a particularly nasty error and breaks a lot of the assumptions we use in our forward-model processing algorithms for refinement (before developments like RELION 3.1 that is :wink: .)

Coma, and its effects on phase-contrast data, is a rather complicated topic deserving of its own forum post. For now I will just put a link here to a very good review by Anchi Cheng and Bob Glaeser.

Now this coma as I mentioned is caused by beam-tilt, but in our beam-image shift ray diagram there is no tilt shown, both imaging beams pass through our sample as parallel beams. However this is an ideal case, and it requires that the deflection coils function perfectly and that the pivot points are well aligned. The pivot points ensure that beam-shift introduces minimal beam-tilt and vice versa. The image below helps put some visual context to pivot points:

shfttilt

Pivot points need to be well aligned, but that is our job! Adjusting the pivot points regularly decreases the stability of the microscope for the next user. DON’T TOUCH THEM!

We can see from above that if we change the height of the specimen (say away from the mechanical Eucentric height due to a bent grid) the pivot point is no longer perfect. If we change the strength of the objective lens (defocus) then the back-focal plane changes height (very slightly but it does change) and again the pivot point is no longer perfect. So we can only do our best to set the alignments at Eucentric focus and minimize the effects. Additionally, the deflector coils are not exact to begin with, nor are they situated perfectly orthogonal to each other which we need to handle the 2-D situation we are actually considering.

Again with all of this considered it is no surprise that we have always avoided beam-image shift exposures for high-resolution data collection. But a number of things have changed recently that have led to beam-image shift collection to become more attractive:

  • Refinement algorithms have improved to become more sophisticated
    • This is also largely tied to the detector advancements which are essential to increase the SNR needed for these software devolpments
  • We are tackling more heterogeneous samples which demand huge number of particles foremost
  • Microscope access is limited and so high-throughput is essential

This has led of course for Thermo-Fisher to develop

Aberration Free Image Shift


source

AFIS attempts to further minimize the effects of coma and astigmatism induced by beam-image shift. The idea is fairly simple and is setup (AFIS alignment (service)) starting from a well-aligned microscope with coma and astigmatism already corrected for the on-axis condition:

  1. Use beam-image shift using the X-axis deflector coils a decent amount (4um)
  2. Calculate a Zemlin tableau to measure and correct the induced coma (as is done in Sherpa or EPU Coma-free autofunction)
  3. Calculate the diffractogram to measure and correct the induced astigmatism.
  4. Note the adjustments to the objective stigmator and beam deflection coils
  5. Repeat 1 - 4 in 4um steps up to 20um and then in -4um steps to -20um
  6. Repeat 1 - 5 but now using the Y-axis deflector coils
  7. Finally a combination of X and Y deflector coils is used to account for perpendicular correction

With this data the system can now compensate the coma and astigmatism implied by the imperfect beam-image shift system. The correction is not perfect though and so you will find that even though calibration is done out to 20um, EPU restricts beam-image shift to 6um. data collected with AFIS has been shown to substantially reduce the amount of accumulated beam-tilt (in the published case found to be 0.19 mrad/um shift) and improve the final achieved resolution (source.)

However it is important to note AFIS does not reduce the aberration caused by:

  • Beam-tilt induced by changes in sample height / defocus
  • Any beam-tilt existing in the on-axis condition
  • Spherical aberration
  • Off-axial imaging

Furthermore since we can estimate aberrations due to beam-tilt and beyond in software post-collection we should continue to do so. This requires the data to be grouped into sets of similar aberration conditions, which requires dividing the AFIS data based on the amount of beam-image shift applied.

Unfortunately with the development of EPU and RELION being anything but synced, this division is not particularly straightforward. However I hope the code and Python notebook linked to at the start of the post will prove to be useful in getting the data split appropriately. I truly hate writing Python, but I hope it makes the process a little more transparent compared to early iterations written in BASH.

Please let me know as always if you have any comments, suggestions or questions about this topic. I am always happy to talk further. I would like to hope that our community will more actively engage in discussion when we have time to read and digest the topics, and when there is maybe not the same stage-fright as speaking up in the bi-weekly meeting :sweat_smile:

Super nice Dustin, thanks!
I am a bit confused about what would exactly happened in the presence of a Cs corrector. There will be still a problem induced by beam tilt I guess. Is this correct?
xxx

Yes! C_s\text{-corrected} microscopes have to use the corrector to manage all of the other aberrations, which with no remaining C_s, increase in their impact on imaging (There’s these slides from EMBO 2015 which is useful). This means that AFIS, as far as I am aware of is not really usable in these scopes. In the TFS poster I think that’s shown with Note 2

Coma correction via beam tilt is not applied in Cs image-corrected systems

I even think that the corrected microscopes cannot use hardly any beam-image shift because of off-axial aberrations the system is not suited for, but this could be changing in the future with developments which account for off-axial effects: https://patents.google.com/patent/WO2019133433A1

So it was brought to my attention from the cryoSPARC documentation that template positions are indicated in the filenames of EPU movies. However, upon further inspection EPU is not creating different tags for different holes (hopefully this is something they will be adding soon):

Here’s the link to the cryoSPARC information in case you don’t have the patience to read through the issue :wink:

But regardless, this was news to me and so I wanted to share the information to you all as well in case you find it useful.

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