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VE1XOP

I’m Sean Bridge, a licensed Ham Radio Operator with a passion for digital operations. I enjoy exploring new technologies and sharing what I learn with others. Teaching and mentoring fellow operators is one of my favorite parts of the hobby. Email: qso@ve1xop.ca

Amateur Radio 12M Band Needs You

How to Check if 12m Is Open

When the 12-meter band does open, it can provide excellent DX — often with less QRM. But you have to catch it. Here’s how:

🛰️ 1. Use Real-Time Propagation Tools

🔭 2. Watch the Solar Numbers

12m comes alive during:

  • SFI (Solar Flux Index) above 120–130
  • Low K-index (0–3) for stable conditions
  • High sunspot activity (check spaceweatherlive.com)

📡 Tips to Activate Interest in 12m

 

1. Start Calling CQ

Even if you hear nothing — call anyway. 12m can pop open fast, and others will hear your CQ if the path is there.

2. Use FT8 or FT4

Digital modes work well even when SSB seems dead. Try calling on:

  • 24.915 MHz for FT8
  • 24.919 MHz for FT4

3. Join a 12m Group or Net

Some Facebook groups and forums focus on high bands. Examples:

  • “12 Meter Operators Group”
  • QRZ forums / Reddit’s r/amateurradio

4. Post Your Spot

  • Use DX clusters (e.g., dxwatch.com) to alert others that you’re calling CQ on 12m.
  • Helps generate interest and traffic.

5. Get Involved with SOTA / POTA (Optional)

  • If you’re an outdoor or portable operator, consider activating a Summits On The Air (SOTA) or Parks On The Air (POTA) site.
    • You can spot yourself on SOTAwatch or POTAWATCH to let others know you’re active on 12m.
    • Many POTA/SOTA ops focus on 12m when it’s open since it’s less crowded than 20m.

6. Get Noticed

  • If you’re stationary, use DX Cluster or RBN to spot your own CQ.
    • Post a message saying, “CQ 12m from [Your Location]”. This can alert others.

7. Have Patience

  • If you don’t hear much immediately, don’t worry. The band may open and close quickly, especially during sunspots or sporadic E openings.
  • Keep calling every 5–10 minutes, and you may catch a new opening.

8. Log Your Contacts

  • Once you make a QSO, be sure to log it! Using software like Log4OM, N1MM, or HamRadioDeluxe can make logging easy and automatic, especially for contests.

🏆 Bonus Tip: Boost Interest in 12m

  • Try a “CQ 12m” Challenge with your local club or on social media:
  • Post a challenge to call CQ on 12m for a day and report how many countries you’ve worked.
  • Share the challenge in local groups, forums, and DX clusters to encourage others to jump on.

📆 Quick Weekend Plan for 12m Activation

  • Saturday Morning: Check propagation conditions and get your antenna tuned.
  • Saturday Afternoon: Start with FT8 or SSB — call CQ, see if anyone’s listening.
  • Sunday: If 12m isn’t busy, try again — conditions may have changed!

With this plan, you’ll be ready to activate 12m even if it’s just for a short weekend experiment. The key is persistence and being ready when the band opens!

Need to Know items: (at least from what I know…)

Technical & Propagation Factors

  • Sporadic Propagation – 12m relies heavily on solar cycle peaks and sporadic E for reliable long-distance communication.
  • Narrow Bandwidth – Only 100 kHz wide, making it feel limited compared to broader bands.
  • Propagation Similar to 10m – Many ops default to 10m, which is adjacent and more active.
  • Poor Conditions During Solar Minimum – The band is nearly dead when solar activity is low.
  • Not Suitable for Nighttime Use – 12m closes down quickly after sunset.

Community & Culture

  • Lack of Activity – Few people calling means others don’t bother listening.
  • Chicken-and-Egg Problem – Nobody transmits because nobody is listening.
  • Limited Contest Use – Not many contests encourage or emphasize 12m operation.
  • Not Taught or Emphasized – Training materials and Elmers often focus on 20/40/80 meters instead.
  • Perception as a “Specialty” Band – Seen as something for advanced or niche operators.

Equipment & Antennas

  • Antenna Size & Tuning Issues – Slightly harder to build efficient antennas than for 10m.
  • Some Rigs Don’t Cover 12m – Especially older or entry-level transceivers.
  • Multiband Antennas Skipping 12m – Many HF antennas prioritize more commonly used bands.
  • Poor SWR Performance – If antennas aren’t resonant on 12m, operators may avoid it.

Digital & Operating Modes

  • Less Digital Mode Activity – FT8, PSK31, etc., have more activity on other bands.
  • Not Supported by Some Automatic Band Plans – Especially with automated digital software.
  • Less SOTA / POTA Activity – Activators often skip 12m for more predictable results.

Human Behavior & Convenience

  • Operator Habit / Inertia – People stick to what they know: 20m for day, 40/80m for night.
  • Scanning Time & Patience – It’s easier to find QSOs on “busier” bands than to wait on 12m.
  • Lack of Awareness – Some hams just don’t know how good 12m can be when it’s open.

Final Thought:

12m is a fantastic band for those who want to explore something a bit different — less crowded, with the potential for exciting DX and quality contacts. Whether you’re using digital modes or SSB, the band offers a unique space for those willing to put in the time to listen for openings and call CQ when conditions are right. If you’re interested in exploring 12m, now might be the perfect time to give it a shot, especially if solar conditions are favorable. Even if you’re a casual operator, giving the band a try will likely be a rewarding experience!

73’s de VE1XOP

Comments or Feedback?

Please email: qso@ve1xop.ca or make a comment below this post.

 

Unlocking HF Potential with 12m and 10m in Amateur Radio

For many amateur radio enthusiasts, the lower HF bands (80m, 40m, 20m) represent the bread and butter of global communication. But venturing higher up the spectrum, into the realms of 12 meters (24 MHz) and 10 meters (28 MHz), offers unique propagation characteristics and exciting possibilities that deserve exploration. Often overlooked, these bands can provide exceptional DX opportunities, local and regional communication, and a playground for experimentation with various modes and techniques. This article delves into the benefits of operating on 12m and 10m, exploring their propagation nuances, suitable modes, and why every amateur radio operator should consider adding these frequencies to their operating repertoire.

Understanding the Allure: Why 12m and 10m?

While the lower bands offer reliable communication over longer distances, 12m and 10m present a dynamic and often unpredictable landscape. Their appeal stems from a combination of factors:

  • Sporadic-E (Es) Propagation: Arguably the most compelling reason to monitor 12m and 10m is the potential for Sporadic-E propagation. This phenomenon, primarily occurring during late spring and summer months, involves the formation of highly ionized patches in the E layer of the ionosphere. These patches act as “mirrors,” reflecting radio signals over distances ranging from a few hundred to thousands of kilometers. Es propagation allows for strong, short-skip contacts that can bypass typical F-layer propagation patterns. 10m is particularly renowned for Es, often opening up seemingly impossible paths.
  • F2-Layer Propagation: Under favorable solar conditions (high solar flux and sunspot numbers), the F2 layer of the ionosphere can support long-distance propagation on 12m and 10m. This allows for global communication with relatively low power. While not as consistently reliable as the lower bands, when F2 propagation is active, these bands can rival or even outperform 20m in terms of signal strength and skip distance.
  • Lower Noise Floor: Compared to the lower bands, 12m and 10m often experience a significantly lower noise floor. This is due to reduced atmospheric noise and man-made interference. A quieter band translates to better signal-to-noise ratio (SNR), making weaker signals more readable and improving overall communication quality.
  • Smaller Antennas: A significant advantage of operating on higher frequencies is the reduced antenna size required for optimal performance. A full-sized dipole on 80m can be hundreds of feet long, whereas a dipole for 10m is only around 16 feet. This makes 12m and 10m accessible to operators with limited space, such as apartment dwellers or those with strict homeowner association regulations.
  • Less Congestion: While activity on 12m and 10m can fluctuate, they generally experience less congestion than the more popular lower bands. This allows for easier access to the airwaves and reduces the likelihood of interference. It’s a great option when the lower bands are packed with signals.
  • Experimentation and Learning: 12m and 10m serve as excellent bands for experimentation with different antenna designs, propagation modes, and operating techniques. The unpredictable nature of these bands encourages innovation and provides valuable experience in troubleshooting and optimizing radio setups.

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The Fascinating Reach of Shortwave Radio

Catching Waves from Around the World

 

Introduction

Shortwave radios are a marvel of modern technology, providing listeners with access to a diverse range of content from all corners of the globe. Unlike their AM and FM counterparts, shortwave radios can receive transmissions from thousands of miles away, making it possible to tune into stations from different continents. In this article, we will explore the science behind shortwave radio technology and discover why we can hear radio stations from around the world on these versatile devices.

The Science Behind Shortwave Radios

Shortwave radio waves fall within the frequency range of 1.711 MHz to 30 MHz. These waves have the unique ability to travel long distances by bouncing off the Earth’s ionosphere, a layer of electrically charged particles in the upper atmosphere. The ionosphere reflects the radio waves back towards the Earth’s surface, allowing them to travel much farther than local AM or FM signals.

When a shortwave radio signal is transmitted, it first travels in a straight line from the antenna. As it encounters the ionosphere, the signal is refracted, or bent, into a curved path that follows the Earth’s curvature. This process enables the signal to bypass physical obstacles such as mountains, buildings, and other terrain features. The reflected signal can then be picked up by a shortwave radio receiver, even if the transmitting station is located on a different continent.

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Why Radio Teletype (RTTY) Still Matters

RTTY is Beyond the Bells and Whistles & Still Matters in the Digital Age

In a world dominated by lightning-fast fiber optics, ubiquitous Wi-Fi, and sophisticated digital modes like FT8 and JS8Call, why should anyone bother with Radio Teletype (RTTY)? It’s a fair question. RTTY, with its clattering sounds and seemingly archaic technology, might seem like a relic of the past, a dinosaur lumbering behind the sleek mammals of modern digital communication.

However, dismissing RTTY out of hand would be a mistake. Beneath its seemingly simple exterior lies a robust, reliable, and surprisingly versatile mode that continues to offer unique advantages in various scenarios. This isn’t about nostalgia; this is about appreciating a technology that has stood the test of time, and understanding why it remains a valuable tool in the toolbox of any serious radio communicator.

This article will delve into the compelling reasons why RTTY still deserves our attention, exploring its underlying principles, its unique benefits, and its surprising relevance in the 21st century.

Understanding the Basics: What is RTTY?

RTTY, short for Radio Teletype, is a method of transmitting text over radio waves using Frequency Shift Keying (FSK). In its simplest form, FSK involves transmitting two distinct audio tones, representing a “mark” (usually a higher frequency) and a “space” (a lower frequency). These tones correspond to the binary digits 1 and 0, which are then encoded into characters based on the Baudot code (also known as the Murray code).

Think of it like Morse code, but instead of varying the length of the tone, RTTY varies the frequency of the tone. A receiving station then demodulates these tones and uses a teleprinter or computer software to decode them back into readable text.

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The Dark Side of Ham Radio

The Dark Side of Ham Radio & Negative Comments and Social Media

The world of amateur radio, also known as ham radio, is a vibrant and diverse community of enthusiasts who share a passion for communication and technology. However, like any other community, ham radio operators are not immune to the negative effects of social media. In this article, we will explore the impact of negative comments and social media on the ham radio community.

The Ham Radio Community

The ham radio community is a global network of amateur radio operators who use various modes of communication, including Morse code, voice, and digital modes, to connect with each other. Ham radio operators come from diverse backgrounds and age groups, and they share a common interest in communication, technology, and community service.

Social Media and Ham Radio

Social media has become an integral part of the ham radio community, with many operators using platforms like Facebook, Twitter, and YouTube to connect with each other, share information, and showcase their activities. However, social media has also introduced a new set of challenges and negative effects that can impact the community.

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Dummy Load vs. Compromised Antenna with an Antenna Tuner

The Great Pretender: Dummy Load vs. Compromised Antenna with an Antenna Tuner

In the world of radio communication, antennas play a crucial role in transmitting and receiving signals. However, there are situations where an antenna may not be functioning correctly, or a dummy load is used to simulate an antenna load. In this article, we will delve into the differences between a dummy load and a compromised antenna, both used with an antenna tuner.

Understanding the Basics

Before we dive into the specifics, let’s cover some basic concepts:

– Dummy Load: A device designed to simulate an antenna load, absorbing RF energy without radiating a signal.
– Compromised Antenna: A faulty or inefficient antenna due to physical damage, incorrect installation, or environmental factors.
– Antenna Tuner: A device that matches the impedance of the transmitter to the antenna, optimizing power transfer and minimizing reflections.

Dummy Load with Antenna Tuner

When using a dummy load with an antenna tuner, the following scenarios unfold:

  • Impedance Matching: The antenna tuner attempts to match the impedance of the transmitter to the dummy load.
  • Low SWR: Since the dummy load is designed to absorb RF energy, the antenna tuner can typically achieve a low Standing Wave Ratio (SWR).
  • No Radiation: As the dummy load is not designed to transmit, no signal is radiated.
  • Transmitter Safety: The dummy load protects the transmitter from damage by absorbing RF energy.

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Antenna Types Explained

Let’s break down the differences between a long wire antenna, a dipole antenna, and an off-center fed (OCF) dipole antenna, focusing on their structures, operating principles, and typical applications.

1. Long Wire Antenna

  • Structure: A long wire antenna is essentially a single wire (or a wire with a specific length) that can be several wavelengths long. It can be oriented horizontally, vertically, or at an angle.
  • Length: Typically, a long wire antenna is at least half a wavelength long. The longer the wire, the better the efficiency in terms of radiating and receiving radio waves.
  • Operating Principle: It works by creating an electromagnetic field around the wire when current flows through it. The wire length and orientation affect its radiation pattern and impedance.
  • Radiation Pattern: The radiation pattern of a long wire antenna is generally broadside to the wire, with nulls (areas of minimal signal) off the ends.
  • Applications: Long wire antennas are often used in HF (high frequency) applications for receiving signals and can be effective for a variety of modes (CW, SSB, etc.).

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The History and Usage of ROS Amateur Radio Digital Mode

Amateur radio, often known as ham radio, has a rich history of innovation and adaptation. Among the various digital modes developed over the years, ROS (short for Robust Digital Radio) stands out for its resilience and effectiveness. Introduced in 2010 by Spanish amateur radio operator and software developer, José Alberto Nieto Ros, ROS was designed to offer reliable communication even under challenging conditions.

Historical Background

The inception of ROS came during a period when digital modes were rapidly gaining popularity among amateur radio operators. Modes like PSK31, RTTY, and JT65 had already established their niches, catering to different needs from low-power operations to weak-signal communications. ROS was introduced with a specific focus on robustness, making it particularly suitable for long-distance communications in adverse conditions.

José Alberto Nieto Ros, known by his callsign EA5HVK, developed ROS to leverage modern digital signal processing techniques. The mode was designed to work effectively with low signal-to-noise ratios, making it possible to communicate over great distances with minimal power. The introduction of ROS sparked considerable interest and debate within the amateur radio community, particularly regarding its legality under certain national regulations due to its wide bandwidth.

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Top Radio Pioneers

The pioneers of radio were instrumental in shaping the development of communication technology, transforming the way people share information and entertainment. Here are ten notable figures in radio history:

1. Guglielmo Marconi (1874–1937)

Known as the father of radio, Marconi was an Italian inventor who demonstrated the first successful long-distance wireless telegraphy system in 1895. He transmitted the first transatlantic radio signal in 1901, revolutionizing communication.

2. Nikola Tesla (1856–1943)

Although primarily known for his work with electricity, Tesla made key contributions to the development of radio. He conducted early experiments in wireless transmission and held patents that were later used in radio technology. Tesla often argued that his inventions predated Marconi’s.

3. Reginald Fessenden (1866–1932)

A Canadian inventor, Fessenden is credited with being the first to successfully transmit voice and music over the radio. His 1906 broadcast of Christmas music is often cited as the first instance of radio entertainment.

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