EME - It's Not Rocket Science, But it's Close!

EME - It's Not Rocket Science, But it's Close!
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EME - It's Not Rocket Science, But it's Close!

Ever gazed up at the Moon and wondered if you could bounce a signal off it? Well, you can! It's called Earth-Moon-Earth communication, or EME for short, and it's one of the most exciting and challenging aspects of ham radio. If you're new to the concept, let me take you on a quick tour of what EME is all about, and how even modest stations can get in on the action.

What is EME, Anyway?

EME is like a celestial game of billiards, but instead of balls, we're bouncing radio waves. We send a signal up to the Moon, it reflects back down to Earth, and voila - a QSO that spans hundreds of thousands of miles! Sounds simple, but the reality is, it's a bit more involved. You see, the Moon isn't exactly a mirror-smooth reflector. It's more like a giant, rocky golf ball, scattering those radio waves in all directions and even absorbing a portion of the signal. In fact, only about 7% of the signal that hits the lunar surface actually bounces back towards Earth. This makes EME even more challenging, as the returning signal is incredibly weak, battling both the vast distance and the Moon's less-than-perfect reflectivity.

And speaking of distance, that's the other major hurdle in EME. Your signal has to travel to the Moon and back, which is roughly half a million miles round trip! Imagine shouting to someone standing across a vast canyon – your voice would become faint and distorted by the time it reached them. It's the same with radio waves travelling to the Moon and back. They spread out and weaken, becoming a mere whisper by the time they return to Earth. That's why we need some serious firepower to get those signals through: high-power transmitters, large antennas with lots of gain to focus the signal, and incredibly sensitive receivers to pick up those faint whispers from the Moon.

QSOs on the Moon: Q Codes and Modes

Let’s talk ham lingo. An EME conversation is an EME QSO, and the folks you're chatting with are your EME QSO partners.

Now, you might be wondering what kind of signals we actually use for EME. Well, CW (Morse code) has been the traditional choice due to its efficiency in weak signal conditions. It's like whispering really clearly and precisely so your message can be heard across that vast canyon. But in recent years, digital modes have become increasingly popular for EME, especially JT65. This mode was a real game-changer, allowing for successful QSOs with even lower power levels. And these days, the newer Q65 mode is gaining ground. It's incredibly sensitive and can decode signals even when they're barely above the noise floor, like picking out a single voice in a crowded room. It's quite remarkable!

X Marks the Spot: X-pol Antennas and Circular Polarisation

So, why do we often use crossed Yagi antennas (X-pol) for EME instead of regular single-plane ones? Well, it's like having two ears instead of one – you're more likely to hear what's being said, no matter where the sound is coming from. X-pol antennas are similar. They have two sets of elements, one horizontal and one vertical, allowing them to receive signals from both directions.

But here's where it gets even cooler. These X-pol Yagis can actually create something called "circular polarization." Imagine a radio wave spiralling through space like a corkscrew – that's circular polarization! It happens when the horizontal and vertical signals are slightly out of sync, like two dancers performing a perfectly choreographed routine.

Now, there are two types of circular polarization: "Right Hand Circular" (RHCP) and "Left Hand Circular" (LHCP), depending on which way the signal is spiralling. Think of it like turning a screw clockwise or anticlockwise.

Why is this important? Well, as the signal travels through the Earth's atmosphere, it can get twisted and turned like a rollercoaster. Circular polarization helps to reduce the impact of this twisting, ensuring a stronger signal at the receiving end.


Fig.3 - An impressive 144MHz X-pol EME array at OH2BC.

However, circular polarization has its quirks. If you're trying to "work" (that's ham-speak for "communicate with") a station that's only using horizontal or vertical polarization, you might encounter some difficulties. It's like trying to fit a square peg in a round hole – it just doesn't quite match up.

But fear not! Digimode pioneer and Nobel laureate Joe Taylor, K1JT, a professor from Princeton University, developed some really cool modes like MAP65, Q65, and JT65 that can solve this problem. These programs allow you to connect two receivers, one to the horizontal part of your X-pol antenna and one to the vertical part. This clever software then adjusts the timing of the signals to perfectly match the incoming wave, no matter how it's been twisted. It's like having a universal adapter for your radio, ensuring you can connect with anyone, regardless of their polarization.


Fig.1 - The view from a part of the EME/Radio astronomy 432MHz X-pol array at W2PU – Princeton University in New Jersey .

And it's not just clever software that can lend a helping hand with EME. Mother Nature can play a part too! Atmospheric refraction, the bending of radio waves in the atmosphere, can sometimes allow you to work EME QSOs even when the Moon is below the horizon, especially at moonrise and moonset. It's like getting a little boost from the atmosphere, extending the reach of your signal. So, even if the Moon hasn't quite peeked over the horizon or has just dipped below, you might still be able to snag an EME QSO!


Fig.2 - A huge 50MHz X-pol EME array installed at HB9Q.

Small Stations, Big Dreams

You might be thinking, "EME sounds awesome, but I don't have a massive antenna farm!" Fear not, my friend. Thanks to advancements in technology and the generosity of the ham community, even modest stations can experience the thrill of EME.

In fact, with as little as 100 watts and a single 3-element Yagi, you can potentially complete EME QSOs. Of course, you'll be relying on the station at the other end to have a more powerful setup (what we sometimes call a "super-station" with 4 or more Yagis), but the possibility is there.

I remember one of my first EME experiences. I was using two 9-element LFA Yagis, each 4.5 meters long, mounted on a 6-foot pole stuck through the centre of a garden table! It wasn't fancy, but it worked. I managed to work many stations via EME, including some other 2-antenna stations in the USA. So don't let a lack of a "super-station" discourage you from giving it a try.

Ready to Reach for the Moon?

EME is a journey, not a destination. It’s about pushing boundaries, experimenting, and connecting with fellow hams across the globe in a way that few other modes can offer. If you're ready to take on the challenge, do some research, join an EME group, and start planning your first lunar QSO.

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