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  • Beaming internet from the middle of the woods, using an extra-large, pizza-sized satellite dish placed on top of your house, up to a satellite orbiting 550 kilometers outside

  • Earth's atmosphere, well, let's be honest, is technologically mind-blowing.

  • What's even crazier is that the Starlink satellites move incredibly fast, around 27,000 kilometers per hour, and data is being sent back and forth between them at hundreds of megabits per second, all while the dish and satellite are continuously angling or steering the beam of data pointed directly between them.

  • On top of that, the dish switches between different satellites every four or so minutes, because they move out of the dish's field of view rather quickly.

  • If you have no clue as to how this is possible, stick around, because we're going to dive into the multiple key technologies which enable satellite internet to magically work.

  • First, we'll explore inside the satellite dish and see how it generates a beam of data that is able to reach space.

  • Second, we'll see how this dish continuously steers the beam so that it points directly at a satellite moving across the sky.

  • And third, we'll dive into what exactly the dish and satellite are sending inside the beam that results in your ability to stream five HD movies or shows simultaneously.

  • This video is quite long as it's full of in-depth details.

  • We recommend watching it first at 1.25x speed and then a second time at 1.5x speed to understand it as a complete technology.

  • So stick around and let's jump right in.

  • First, let's start by clarifying the difference between a television satellite dish such as this one and the Starlink ground dish, which Elon Musk dubbed Dishy McFlatface, or Dishy for short.

  • TV dishes use a parabolic reflector to focus the electromagnetic waves which are the TV signals sent from broadcast satellites orbiting the Earth at an altitude of 35,000 km.

  • TV satellite dishes only receive TV signals from space.

  • They can't send data.

  • Dishy, however, both sends and receives internet data from a Starlink satellite orbiting 550 km away.

  • While the Starlink satellite is 60 times closer than TV satellites, it's still an incredible distance to wirelessly send a signal and thus the beams between Dishy and the Starlink satellite need to be focused into tight, powerful beams that are continuously angled or steered to point at one another.

  • Compare this to TV broadcast signals which come from a satellite the size of a van and whose signals propagate in a wide fan that covers land masses larger than North America.

  • Table-sized Starlink satellites, however, need to be in a low Earth orbit to provide for 20 millisecond latencies, which is critical for smoothly playing internet games or surfing the web, and as a result their coverage is much smaller.

  • Thus, 10,000 or more Starlink satellites, all orbiting at incredibly fast speeds in a low Earth orbit, are required to provide satellite internet to the entire Earth.

  • Let's now open up Dishy McFlatface.

  • At the back, we have a pair of motors and an ethernet cable that connects to the router.

  • Note that these motors don't continuously move Dishy to point directly at the Starlink satellite.

  • They're used only for initial setup to get the dish pointed in the proper general direction.

  • Opening up Dishy, we find an aluminum structural backplate and on the other side we find a massive printed circuit board or PCB.

  • One side has 640 small microchips and 20 larger microchips organized in a pattern with very intricate traces, fanning out from the larger to smaller microchips, along with additional chips including the main CPU and GPS module on the edge of the PCB.

  • On the other side are 1400-ish copper circles with a grid of squares between the circles.

  • On the next layer, there's a rubber honeycomb pattern with small, notched copper circles and behind that we find another honeycomb pattern and then the front side of Dishy.

  • So what are we looking at?

  • Well, in essence, we have 1,280 antennas arranged in a hexagonal honeycomb pattern with each stack of copper circles being a single antenna controlled by the microchips on the PCB.

  • This massive array works together in what's called a phased array in order to send and receive electromagnetic waves that are angled to and from a Starlink satellite orbiting 550 kilometers above.

  • Let's zoom in and see how a single antenna operates.

  • Here we have an aperture-coupled patch antenna composed of 6 layers, most of which are inside the PCB.

  • It looks very different from the antenna of an old-school radio and is honestly incredibly complicated, so let's simplify it.

  • We'll remove a few of the layers for now and step through the basic principles of how we generate an electromagnetic wave that propagates out from this antenna.

  • To start, at the bottom we have a microstrip transmission line feed coming from one of the small microchips.

  • This transmission line feed is just a copper PCB trace, or wire, that abruptly ends under the antenna stack.

  • We send a 12 gigahertz high-frequency voltage, or signal, to the feed wire, which is a voltage that goes up and down in a sinusoidal fashion, going from positive to negative and back to positive once every 83 picoseconds, 12 billion times a second, or 12 gigahertz.

  • Note that high-frequency electricity works differently from direct current or low-frequency 50 or 60 hertz household electricity.

  • For example, above the copper feed wire we have a copper circle with notches cut into it called an antenna patch.

  • With DC, or low-frequency alternating current, there wouldn't be much happening because the patch is isolated, but with a high-frequency signal, the power sent to the feed wire is coupled or sent to the patch.

  • How exactly does this happen?

  • Well, as mentioned earlier, a 12 gigahertz signal is applied to the copper feed wire.

  • When the voltage is at the bottom of its sinusoidal, or trough, we have a concentration of electrons pushed to the end of the feed wire, thus creating a zone of negative charge which corresponds to the maximum negative voltage.

  • This concentration of electrons on the tip of the wire repels all electrons away, including the electrons on the top of the patch, and as a result, these electrons are pushed to the other side of the circular patch.

  • Thus, one side of the patch becomes positively charged while the other becomes negatively charged, thereby creating electric fields between the patch and feed wire, like so.

  • However, when we reverse the voltage to the copper feed wire 42 picoseconds later, we have a concentration of positive charges, or a lack of electrons at the end of the wire, and thus the electrons in the patch flow to the other side.

  • The voltage in the patch is flipped, and the direction of the electric fields are also flipped.

  • Because the feed wire voltage oscillates back and forth 42 picoseconds between one peak and trough, the electric fields in the patch will also oscillate as the electrons, or current, flows back and forth.

  • If we pause the oscillation, we can see some of these electric field vectors, or arrows from the patch, are vertical, and because they're equal and opposite, they cancel out.

  • However, other electric fields are horizontal in the same plane of the patch, and are called fringing fields.

  • These fringing fields are in the same direction, and thus they add to each other, resulting in a combined electric field pointing in this direction.

  • At the same time, electrons flowing from one side of the disk to the other, which is an electric current, generate a magnetic field with a strength and direction, or vector, perpendicular to the fringing electric field vector.

  • As a result, we have an electric field pointing one way, and a magnetic field pointing perpendicular to that.

  • Let's move forward in time to where the voltage on the feed line becomes positive, and now we're at the peak of the sinusoid, 42 picoseconds later.

  • The charge concentrations, or voltage, as well as the current, is all flipped, and thus the electric and magnetic fields point in the opposite directions.

  • Electric and magnetic fields propagate in all directions, and by creating these oscillating fringing fields, we've generated an electromagnetic wave, which travels in the direction perpendicular to both the electric and magnetic field vectors.

  • Because the two sets of field vectors are not all in the same plane, but rather are curved, the propagating electromagnetic wave travels outwards in an expanding shell or balloon-like fashion, kind of like a light bulb on the ceiling.

  • Let's simplify the visual, so we can see the peak and trough, or top and bottom, of each wave, and note that the trough is just a vector pointed in the opposite direction.

  • Additionally, the strengths of these field vectors directly relate back to the voltage and signal that we originally sent to the copper microstrip feed wire at the bottom of the stack.

  • Which means, if we want to make these electric and magnetic fields stronger, we just have to increase the voltage sent to the feed line.

  • Just like a dimmer on a light switch, more power equals a brighter light.

  • Thus far, we've been talking about this aperture-coupled patch antenna as transmitting, however it can also be used for receiving a signal.

  • In this microchip, called a front-end module, we switch the antenna from transmit to receive and turn off the 12 GHz signal.

  • When an electromagnetic wave from the satellite is directed towards DISHI, the electric fields from this incoming signal will influence the electrons in the copper patch, thus generating an oscillating flow of electrons.

  • This received high-frequency signal is then coupled to the feed line where it's sent to the front-end module chip which amplifies the signal.

  • Thus, these antennas can be used to both transmit and receive electromagnetic waves, but not at the same time.

  • Two quick things to note.

  • First, as seen earlier, this antenna has many more layers, and is more complicated than we've discussed.

  • For example, here are two circular patches.

  • The bottom is used to transmit at 13 GHz, while the top to receive at 11.7 GHz.

  • Additionally, there are two H-slots and two feed wires to support circular polarization, a reflective plane in the back, and also there are multiple features for isolating the operation of one antenna from the adjacent antennas.

  • We've included these and many more details in the creator's comments, which you can find in the English-Canadian subtitles.

  • The second note is that there are electromagnetic waves of all different frequencies from thousands of different sources, passing through every point on Earth.

  • Whether it be visible light from the sun, radio waves from radio or cell towers, or

  • TV signals from satellites or towers.

  • Therefore, in order to block out all other frequencies of electromagnetic waves, these antenna patches are designed with very exact dimensions, so that they receive and transmit only a very narrow range of frequencies, and all the other frequencies outside this range are essentially ignored by the antenna.

  • Let's move on and see how a single antenna can be combined with others in order to amplify the beam to reach outer space.

  • This single antenna is only a centimeter or so in diameter, and using only it would be like turning on and off one light bulb and trying to see it from the International Space

  • Station.

  • What we need is a way to make the light a few thousand times brighter, and then focus all the electromagnetic waves into a single, powerful beam.

  • Consider the massive Mr. McFlatface PCB, 55 centimeters wide, with a total of 1,280 identical antennas in a hexagonal array.

  • The technique of combining all the antennas' power together is called beamforming.

  • So how does it work?

  • Well, let's first see what happens when we have two simplified antennas spaced a short distance away.

  • As mentioned before, one antenna generates an electromagnetic wave that propagates outwards in a balloon shape.

  • At every single point in space, there's only one electric field vector with a strength and direction, and thus, the two antennas' oscillating electric field vectors combine together at all points in space.

  • In some areas, the electric fields from the antennas are pointing in the same direction with overlapping peaks, and thus, add together via constructive interference.

  • And in other locations, they're opposite with one peak on one trough, and thus, they cancel each other via destructive interference.

  • We can now see that the zone where they add together constructively is far tighter, or more focused, than a single antenna alone.

  • When we add even more antennas, the zone of constructive interference becomes even more focused in what is called a beam front.

  • Thus, by adding 1280 antennas together, we can form a beam with so much intensity and directionality that it can reach outer space.

  • Now you might be thinking that the strength of one antenna duplicated 1280 times over would result in a combined power of, well, 1280 times a single antenna.

  • But you'd be mistaken.

  • The effective power and range of the main beam from all these antennas combined is actually closer to 3500 times that of a single antenna.

  • The quick explanation is that by having these patterns of constructive and destructive interference, it's as if we took a single antenna, multiplied it by 1280, and then placed a whole bunch of mirrors around it, and left only a single hole for the main beam to exit through.

  • The long explanation requires a ton of math and physics, so let's move on.

  • Dishy McFlatface and the Starlink satellites undoubtedly have some rather complicated science and engineering inside.

  • And to fully comprehend it all, you have to be a multidisciplinary student.

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  • Brilliant is nothing like a boring textbook, but rather all the courses use interactive modules to make the lessons entertaining and to help the concepts stick in your head.

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  • Now let's continue exploring how a powerful beam can be continuously swept across the sky and then how we fill it with hundreds of megabits of data every second.

  • As a quick refresher from before, here's an array of 1280 antennas and we fed them all with the same 12 GHz signal in order to create a laser-like beam propagating perpendicular to Dishi.

  • However, as mentioned earlier, we need to be able to angle this beam so that it points directly at the Starlink satellite zooming across the sky at 27,000 km per hour.

  • Using the motors isn't feasible because they would break within a month and aren't accurate enough.

  • So the solution is to use what's called phased array beam steering.

  • Let's go back to our two antenna example.

  • Before, we were feeding the same signal to the two antennas and thus the antennas were in phase with one another.

  • Changing phase is critical.

  • So quickly, changing the height or amplitude of the signal is done by changing the power sent to the antenna, thus making the signal stronger or weaker.

  • The frequency is how many peaks and troughs or wavelengths there are in one second and changing the phase is shifting the signal left or right.

  • Phase shifting is measured in degrees between 0 and 359 because if we shift the signal 360 degrees, or one full wavelength, then we're back at the beginning, exactly as if we were to loop around a circle.

  • For example, here's a signal with a 45 degree phase shift, here's another with a 180 degree shift, and then another with a 315 degree shift.

  • Your eyes can't see differences in phase shifted visible light.

  • However, high-tech circuitry such as what's inside Dishi is really good at detecting and working with phase shifts.

  • So then, how do we use phase shifting to angle the beam and have it point directly at the satellite?

  • The solution is to phase shift the signal sent to one antenna with respect to the other antenna and, as a result, the timing of the peaks and troughs emitted from one antenna is different from the other.

  • These peaks and troughs propagate outwards and the location of the constructive interference is now angled to the left with destructive interference everywhere else.

  • If we change the phase of the antennas again, the zone of constructive interference is angled to the right.

  • Therefore, by continuously changing the phase of the signal sent to the antennas, we can create a sweeping zone of constructive interference.

  • Let's bring in six more antennas and simplify the visual so that we only see a section of the peaks from each wave.

  • Far away from the antennas, the waves join to form a wavefront that is a planar wave, kind of like ocean waves crashing on a shoreline.

  • Just as before, by continuously changing the timing of when each wave peak is emitted by each antenna, we can change the angle at which the wavefront is formed, essentially steering the beam in one direction or another.

  • And if we bring in more antennas in a two-dimensional array, we can now steer the beam in any direction within a 100-degree field of view.

  • Let's move back to view all 1280 antennas in DISHI.

  • In order to know the exact angle the beam needs to be pointed or steered, we use the

  • GPS coordinates of DISHI from this chip over here, along with the orbital position of the

  • Starlink satellite which is known in DISHI software.

  • The software computes the exact set of 3D angles and the required phase shift for each of the antennas.

  • These phase shift results are then sent to the 20 larger chips called beamformers and each beamformer coordinates between 32 smaller chips called front-end modules, each of which controls two antennas.

  • Every few microseconds, these computations are recalculated and disseminated to all the microchips in order to perfectly aim the beam at the satellite.

  • As a result, the beam can be steered anywhere in a 100-degree field of view.

  • Here are a few quick notes.

  • First, the main beam, also called the main lobe, looks like this.

  • However, constructive and destructive interference isn't perfect and, as a result, there are additional side lobes of lesser power.

  • Third, Mr. McFlatface holds a single phased array.

  • However, on the Starlink satellite, there are, in fact, four phased array antennas.

  • Two are used to communicate with multiple DISHIs and two are used to communicate with the ground stations to relay the internet traffic.

  • And fourth, phased arrays are used in many applications and, interestingly, they're used on commercial airlines to allow for mid-flight internet.

  • So this video also tangentially explains how mid-flight internet works.

  • Before we explore how actual data is sent, we want to mention that this video took a month to research, two dozen script revisions, and two months to model and animate.

  • If your mind is blown by the complexity of this technology and the depth of this video, click the subscribe button, like this video, write a comment below, and we'll be sure to create more videos like this one.

  • The third topic we're going to dive into is how information gets sent between DISHI and the Starlink satellite.

  • For example, we've talked about high-frequency sinusoid-shaped electromagnetic waves, but that doesn't look anything like binary, and even less like your favorite TV show.

  • So what's happening?

  • Well, DISHI and the satellite indeed send a signal that looks like this.

  • However, they vary the amplitude and the phase of the transmitted signal and then assign or encode 6-bit binary values to each different combination or permutation of amplitude and phase.

  • With 6 bits, there are 64 different values, and thus we need 64 different permutations of amplitude and phase.

  • However, instead of listing all the permutations, it's more easily visualized by arranging the 64 different values in a graph, called a constellation diagram, as shown.

  • Let's look at the point 011101 and draw a line from the origin to this point.

  • The distance from the origin is the amplitude of the signal, and the angle from the positive x-axis is the phase.

  • It's a bit like using polar coordinates.

  • Thus for DISHI to send these 6 bits, it transmits a signal with an amplitude of 59% and a phase shift of 121 degrees.

  • Then, if the next value being sent is 101000, the signal switches to an 87% amplitude or brightness and a 305 degree phase shift.

  • After that, it sends the next value with a different amplitude and phase shift.

  • Each of these 6-bit groupings are called symbols, and they last for only 10 or so nanoseconds before the next symbol is sent.

  • Lots of times you see the signal scrunched up like this, however, because the frequency of the signal is just once every 83 picoseconds, or 12 gigahertz.

  • And since a symbol lasts 10 nanoseconds, it's more accurate to have around 120 wavelengths per symbol before the next symbol is sent.

  • Because we're dealing on the order of pico and nanoseconds, that means that we can fit 90 million 6-bit groups or symbols, resulting in 540 million bits per second.

  • However, note that this data transfer is shared between download and upload.

  • Since this particular antenna can't transmit and receive data at the same time, about 74 milliseconds of every second is used to send data from DISHI to the Starlink satellite, and 926 milliseconds is used to send data from the satellite down to DISHI.

  • And for the sake of reducing latency, these time slots get distributed throughout a single second instead of grouping them all together.

  • This technique of sending 6-bit values using different variations of amplitude and phase is called 64-QAM, or Quadrature Amplitude Modulation, and is more complicated than we've discussed.

  • But let's not get sidetracked.

  • Now that we have a stream of millions of 6-bit symbols yielding hundreds of megabits of data per second, in order to turn it into your favorite TV show, we use the Advanced Video

  • Codec, or H.264 format.

  • You can learn more about that in our video that explores image compression, shown here.

  • I'm sure you have many questions, and by all means put them in the comments below.

  • But before we finish, let's clarify two things.

  • First, the scale of practically everything in this video is off.

  • Here's the correct scale of DISHI and the Starlink satellite.

  • However, DISHI is 550 kilometers away, which we can't correctly show.

  • In stark contrast, the emitted electromagnetic waves are only around 2.5 centimeters apart, and thus, between DISHI and the satellite, there are around 22 million wavelengths, which is many more than the few waves that you see here.

  • Additionally, in this animation, we're showing the wavelengths slowly making their way up and down, when actually it only takes around 2 milliseconds for an electromagnetic wave emitted from DISHI or the Starlink satellite to reach the other.

  • The second clarification is that we disproportionately show DISHI emitting electromagnetic waves and sending them to the satellite.

  • In reality, the satellite dishes more frequently in receive mode, and the steps and physics of receiving an electromagnetic wave are similar to emitting one, just in reverse.

  • That's pretty much it for how Starlink and DISHI send data to each other.

  • The original script for this video was over 45 minutes long, so all the details that were cut got their own in the creator's comments, found in the English Canada subtitles.

  • Thank you to all of our Patreon and YouTube membership sponsors for helping to make this video.

  • Also, thank you to Colin O'Flynn at NewAeTechnology for lending us a Starlink DISHI PCB for imaging and research.

  • This is Branch Education, and we create 3D animations that dive deep into the technology that drives our modern world.

  • Watch another Branch video by clicking one of these cards, or click here to subscribe.

  • Thanks for watching to the end.

Beaming internet from the middle of the woods, using an extra-large, pizza-sized satellite dish placed on top of your house, up to a satellite orbiting 550 kilometers outside

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