Battalion Tactical Groups

As Russia redeploys its forces in and around Ukraine, you can expect to hear more about how they are attempting to reconstitute their battalion tactical groups. But what exactly is a battalion tactical group?

Recently in Russia, the army has been reorganised increasingly away from regiments and divisions and towards smaller, more integrated units that theoretically can operate more independently: battalion tactical groups. They typically comprise less than a thousand soldiers, about 200 of which are infantry. But they also include a number of tanks, infantry fighting vehicles (IFVs), armoured personnel carriers (APCs), artillery, and other support units.

In an article from two weeks ago, the Washington Post explained why the Russian army had stalled out in Ukraine. And as part of that, they explained what a battalion tactical group is with a nice illustration.

Just some of the vehicles in a BTG

Russia’s problem is that in the first month of the war, Ukrainian anti-armour weapons like US-made Javelins and UK-made NLAWs have ripped apart Russian tanks, IFVs, and APCs. Atop that, Ukrainian drones and artillery took out more armour. The units that Russia withdrew from Ukraine now have to be rebuilt and resupplied. Once fresh, Russia can deploy these into the Donbas and southern Ukraine.

This graphic isn’t terribly complicated, but the nice illustrations go a long way to showing what comprises a battalion tactical group. And when you see photos of five or six tanks destroyed along the side of a Ukrainian road, you now understand that constitutes half of a typical unit’s available armour. In other words, a big deal.

I expect to hear more out of Russia and Ukraine in coming days about how Russia is providing new vehicles and fresh soldiers to resupply exhausted units.

Credit for the piece goes to Bonnie Berkowitz and Artur Galocha.

Let There Be Light

In several decades…

Just a quick little piece today, a neat illustration from the BBC that shows how the process of nuclear fusion works. The graphic supports an article detailing a significant breakthrough in the development of nuclear fusion. Long story short, a smaller sort-of prototype successfully proved the design underpinning a much larger fusion reactor currently under construction in France. We are potentially on our way to proving the viability of nuclear fusion as an energy source.

Why is that important? Well, first of all, no carbon emissions. Nuclear fusion powers the Sun, where hydrogen is fused with hydrogen to produce helium and in the process release an enormous amount of energy. Mankind wants to take that energy and use it to heat water to generate steam to spin turbines to create electricity.

And we use a lot of electricity.

So how does fusion work?

The BBC graphic shows how. This is a bit simplified, even for my tastes, but it’s generally pretty good. For example, I probably would have labelled protons and neutrons earlier (to the left) of the graphic. And my big question mark is about the widths of the arrows, because if the width of the arrows relates to the scale of the energy, as that is the crux of the matter. (See what I did there?)

Basically when we want to generate energy we want to add as little as possible to start a reaction to net as much output as possible. A little bit of energy is used to split a uranium isotope and that generates a tremendous amount of energy. Thus far with nuclear fusion, however, we use a lot of energy to fuse hydrogen into helium and get little back as output. In other words, a net loss.

The graphic omits how this reactor in the UK works, by using a doughnut-shaped vessel to contain the hydrogen reaction. To do this they use superconducting magnets to generate powerful electromagnetic fields. This contains the hydrogen that turns into a superheated plasma. After all, it’s not like there are any materials known to man that can safely contain the temperatures of the Sun. But we have evidence that as the amount of plasma scale up, the closer we get to breaking even. And that’s the goal for the French reactor.

The other big question in the room is how this helps us with climate change, because as I stated up top, no carbon emissions. Unfortunately, not much. The French reactor is still several years away from being complete. And if that works as expected, commercial-scale reactors powering electricity generation stations are many more years away. Fusion will help power us into the 22nd century. And so we will still need nuclear fission and renewables to get us through the 21st.

Credit for the piece goes to the BBC graphics department.

Tea. Earl Grey. Hot.

Any science fiction fan—and likely many who are not—can identify the character who utters those words in that order: Jean-Luc Picard, Star Trek’s captain of the USS Enterprise, NCC-1701-D. Ask your Amazon Alexa for it. Or your Google Home.

Thanks to the work of xkcd, we now know that Jean-Luc—may I call him Jean-Luc?—had a number of other options in the replicator from which to choose before he settled on “hot”.

Although Garak would still like to meet that Earl Grey and tell him a thing or two about tea leaves.

Credit for the piece goes to Randall Munroe.

Even Older Family Trees

Yesterday we looked at a graphic about an old family tree, revealed by ancient DNA. But at the end of the day it is a family tree of descent for a human male. But mankind itself fits within a kind of family tree, the circle family tree of life.

The tree of life continues to evolve as we discover new species and then reconfigure what we have to fit what we now know. When I was a wee lad in school, we learned about the three kingdoms of life: plants, animals, and fungi. Bacteria were a separate branch.

A few weeks ago, however, I was reading an article about how a recent DNA analysis identified a new “supergroup” within our larger group of complex cellular life, eukaryotes (plants, animal, and fungi fall within this). Luckily for our purposes the article contains a small graphic at which we can take a look.

Humans are way, way, way down on the tree.

The diagram uses a fairly simple design. Two panels split the largest groupings into its branches whilst the second panel breaks up eukaryotes. Colour links the eukaryotes together and shows how they fit into the broader tree to the left, which uses dark grey and light blue for bacteria and archaea, respectively.

A nice additional touch was the designer’s decision to include a small icon that represents the name of the supergroups within eukaryotes. Because, as the text points out, we don’t have commonly known names for these supergroups. Did I know that we belong to the opisthokonts? Absolutely not. Although dog people may be upset that the cat got the call to represent animals.

Regardless of the design, you can still see in the second panel how people are more closely related to amoeba than we are plants. But this new supergroup, hemimastigotes, branches off from the rest of us eukaryotes at a very early point. And the DNA proves it.

Overall this was a really nice graphic to see in a fascinating article. Science is cool.

Credit for the piece goes to Lucy Reading-Ikkanda.

Sunshield

Happy Friday, everyone.

At the beginning of the week, we looked at the launch and deployment of the new James Webb telescope. If you recall, one of the key elements of the satellite’s design is its sunshield. As the name says, it shields the satellite from the sun, thus keeping the equipment super cold, which is necessary to operate in the range of infrared.

But, as xkcd points out, that’s not actually the real reason for the sunshield.

Credit for the piece goes to Randall Munroe.

Fire in Fairmount

Philadelphia made the national and international news last week, although for once not because we’re all being shot to death. This time because a fire in a rowhome killed 12 people, including nine children. The Philadelphia Inquirer quickly posted a short article explaining what occurred that morning. But the early indication, based upon the confession of a five-year old, is that a child playing with a light set a live Christmas tree on fire.

Ironically, the city prohibits live trees in high rises, apartment buildings, and multi-family dwellings. The rule is in place because live trees are a very real fire hazard. Just a few weeks earlier, a man and two of his sons were killed in a suburb north of Philadelphia (his wife and a third son survived). They died in a fire that began with lights on a live tree. But here in the city, the code states that multi-family dwellings begin at three households. This rowhome had been converted into two separate units, so a live tree was legal. But they would have been better without.

The Inquirer article features a scrolling illustration depicting what we presently know about the fire: how and where it started, why it may have spread, and ultimately who died.

Live trees smell great, but they’re a very real fire risk.

Credit for the piece goes to Sam Morris.

Space: The Final Frontier

We’re back after a nice holiday break. And one of the most fascinating things to happen was the successful—and seemingly easy, more on that in a bit—launch of the James Webb space telescope. The James Webb was developed by NASA with contributions from both the European Space Agency (ESA) and the Canadian Space Agency (CSA). Whilst it did launch behind schedule and at a price tag of $10 billion, the James Webb is the most sophisticated and complex space telescope mankind has yet launched into space. It will look backwards into time to some of the earliest stars and galaxies in the universe. It will also look at the thousands of exoplanets we have discovered in the last three decades. The instruments aboard James Webb will be able to help us identify if any of these planets have water and other ingredients necessary for life as we know it. This could be one of the most monumental space missions yet.

But James Webb’s launch was far from guaranteed. As this great article from the BBC explains, the construction, assembly, launch, and deployment were all incredibly complicated. James Webb is expected to operate for ten years before its fuel, needed to keep the telescope cold, runs out. However, the seemingly easy launch and deployment means that it used less fuel than expected. Some early reports suggest that the telescope may have some additional time left in it now before the fuel runs dry.

I encourage you to read the article, because it explains the advantages of the telescope, how it works, and its deployment with several illustrations. There are five in particular, though I’ll share only two screenshots.

The most important is this, the key distinction between Hubble and James Webb. It shows how the two space telescopes will be operating in different parts of the electromagnetic spectrum.

All the light…

The graphic fakes the colours, because by definition we can only see the visible portions of the spectrum. Wavelengths get either too short or too long on either side of the visible spectrum—which differs for different species. I would actually really enjoy seeing how these two spectra stack up against other space observatories like Chandra (x-ray) and Spitzer (infrared).

Next we have the deployment, which finished just last week. The graphic summarises how complicated this process was—and how fraught with risk. But in the end it went off without any major hitch.

Make sure to read the instructions before deployment…

This uses a nice series of small multiples of illustrations. These simplified drawings show how the tightly packed telescope unfolds and then begins deploying its vital heat shield then its mirror.

The last thing to check out in the article is a slider showing the “before” and “after”. You have seen them before for things like flood or hurricane damages. Here, however, you can compare a photo in Hubble’s visible light to an existing infrared version of the same photo.

Of course, just because the telescope finished deploying its mirror last week doesn’t mean we get photos this week. The Baltimore-based team running the observatory will spend the next few months tuning everything up. But the goal is hopefully to have the first images from James Webb sometime in June.

And then we have the next ten years to hopefully start collecting data.

Credit for the piece goes to the BBC graphics team.

Toronto Keeps It Cool

Last month the Washington Post published a nice article that detailed the deep water cooling system that the city of Toronto, Canada uses to keep itself cool. For the unfamiliar, deep water cooling at its simplest means sucking up very cold water from the bottom of a lake or ocean or wherever you can get very cold water, and then pumping that inland to absorb heat before cycling it back.

Of course, for the longer explanation—and what makes Toronto’s system different—you should read the article. And for our purposes it includes some nice illustrations that diagram just how that system works. The screenshot below captures the basic process I just described, but there are additional illustrations that do a great job showing just how the system works.

Just look at those gloriously cool temperatures…

What I particularly enjoy about this style is how the illustrations of the building and similar are minimal and restrained. This allows the diagrammatic elements to come to the forefront, which is important to make the system understood.

Credit for the piece goes to Daisy Chung.

Greater Delaware

We are at that point in the year where I begin to use up my holiday time for work. I just returned from two weeks away, but I am out again tomorrow, so no post. Ergo, this Thursday is my Friday. And so I’ll leave you with a post from xkcd that talks vexillology, or the study of flags.

Beware Greater Delaware.

Credit for the piece goes to Randall Munroe.