That's awesome. Great animation. Not surprisingly, although the wave is somewhat intensified, it is quite nonuniform and does not come into a sharp focus at the antipode, thanks to the effects of Earth's oblateness and probably reflections as well.
True that.
There's now a beautiful visualization about this, made by Angel Amores:
https://youtu.be/oXa-QsSYpfg
[Source:
https://twitter.com/an_amores/status/1484516695087759363]
You can see a simulated atmospheric pressure wave traveling across the globe from Tonga.
A few things to comment here:
1) The antipodal focusing is not perfectly symmetric and thus the model might have some interesting level of detail. I'm guessing that he has considered the departure from the ideal perfect sphericity of Earth (as
Watsisname has commented), the damping and deceleration of the wave when crossing important topographic features (the Himalayas perhaps?) and possibly the Coriolis effect due to the differential motion of the atmosphere at different latitudes due to Earth's rotation (but my guess is that this might be extremely weak since other random winds might have a larger effect on the wave).
2) Another consideration here is the fact that the pressure wave gets a 90º phase shift when reflected against itself in the antipodes, as
midtskogen noted with his weather station when he recorded the antipodal rebound as a decrease in pressure followed by an increase (instead of the increase followed by a decrease as in the first wave transit). This can be clearly seen in the simulation as the incoming wave has a blue-yellow color palette that gets inverted in order after the rebound.
3) One awesome thing of this video is that you can see the expected data retrieved from the theoretical simulation overlayed on top of the actual data registered by a few barometers around the world. You can see there that the timing of the wave and its rebounds is precisely predicted as well as the general intensity of each signal. This in my opinion shows how well we actually know the shape of the Earth, the wave propagation properties of our atmosphere and the energy involved in the eruption. I hope that almost all the fluctuations seen in the data come from local pressure variations unrelated to the Tonga event. But in any case we will see more detailed models in the next months.
This is also an awesome visualization of the barometric data gathered in Switzerland:

[Source:
https://twitter.com/myweather_ch/status/1484150854236135428]
The S1 mark shows the first wave passing over Switzerland, followed some hours later by the rebound (N1). Then the wave rebounded once again at Tonga and came back (S2) and rebound at the antipodes for a second time (N2). You can clearly see the barometric signal of even the fourth rebound after 5 days of traveling across the globe several times.
Another thing I liked about this data is the way it is visualized. The actual barometric signal is the bottom graph. You can see the wave decaying as expected after each passage. You can see that the peaks in pressure are noticeable but if we wish to make them stand more strongly above the noise (other pressure fluctuations registered that have nothing to do with the shock wave from Tonga), then we must increase the contrast between low values and large values. We could mathematically do that by multiplying the signal by some number (for example by ten), which would enlarge the differences between peaks and valleys in the signal. But this is problematic because the peaks in the noise will also be enlarged and we will end up noticing more noise than before. A nice technique is to perform the first derivative of the signal below. This is a neat trick. By doing that mathematically you are looking for changes in pressure and not the pressure itself. You can perform a second derivative over the signal to get knowledge about the curvature of the signal as we approach a drastic peak. That's exactly what they do in the first and second graph. You can clearly see the peaks as prominent lines on those graphs.
I'm using this data as an excuse to show the technique, which I think is quite neat, and because now we can understand how satellite data can be processed to show the wave traveling around the world quite clearly.
By performing a first derivative with respect to time on the IR images (apparently infrared shows changes in pressure more clearly than optical images) taken GOES-West Satellite (which is geostationary) we can clearly see the wave as if the atmosphere was a giant pond:
https://i.imgur.com/lvxhFUX.mp4
[Source:
https://twitter.com/MathewABarlow/status/1484907406182301697]
The same thing can be done with IR images from EUMETSAT (another geostationary satellite) to reveal the wave as it converges in the antipodes as clearly as possible:
https://i.imgur.com/e7bJhud.mp4
[Source:
https://github.com/mathewbarlow/animations]