AmateurRadio.com

The historical research I recently published in October issue of The Spectrum Monitor is now available on my companion website, foxmikehotel.com. It’s on the home page. TSM allows authors to hold secondary publication rights to articles so I can freely post the PDF now that the November issue is published. Have a look if you don’t subscribe to TSM.

The next episode of the ICQ Podcast, Number 363 that will drop on Sunday November 7th, will feature an audio version of these new research results. For those who’d rather listen than read, this might be a viable option.

One upshot of my research is this: if you begin with the ARRL-published and famous book, 200 Meters and Down by ARRL Secretary Sutton, you are going to be terribly mislead about how amateur radio got organized in the United States. The new website, worldradiohistory.com, amidst other sources such as online historical newspapers (e.g., https://www.newspapers.com), the Internet Archive, the Hathitrust archive, various university-based archives, and other sources, really opens up our ability to more fully understand the origins, emergence and organization of wireless telegraphy which begat amateur radio.

I’ve included a picture from Wikipedia of a person who made voluminous but unheralded contributions to the emergence of amateur radio. This included selling parts to the person who Elmered one of the founders of the ARRL into the hobby. (Did you know there were two co-founders?)

Do you recognize him from this picture?

If not, you’d find the TSM article and the ICQ Podcast feature in the next episode very informative. I’ve included another, one that looks a bit wacky from the day but if you’re familiar with 3D immersive technology, it was “seeing” far into the future of…today! (See the search results using the term, Oculus Quest, if you’re not familiar.)

During a somewhat boring world history class in college, I heard my professor say, “Yes, history is boring to many. Until it touches your life.” He had a point. I was living through some important history of America back in the late-sixties and early seventies. It led me into studying social movements and how they intersect the lives of not only the current participants but those who come afterwards, too.

I hope that the research I’ve done into the early part of the last century on this topic will touch your amateur radio life, so to speak. It has mine as I learned quite a bit from almost a year’s worth of reading and study. I’m delighted that we have an outlet like TSM whose Editor, Ken Reitz KS4ZR, is willing to publish pieces like this.

Frank Howell, K4FMH, is a regular contributor to AmateurRadio.com and writes from Mississippi, USA. Contact him at [email protected].

This imagery captured by NASA’s Solar Dynamics Observatory (SDO; link) covers a busy period of activity in October, during which we witnessed an X1.0-class X-ray flare.

From late afternoon October 25 through mid-morning October 26, an active region on the left limb of the Sun flickered with a series of small flares and petal-like eruptions of solar material.

Meanwhile, the Sun was sporting more active regions at its lower center, directly facing Earth. On October 28, the biggest of these released a significant flare, which peaked at 15:35, 28 Oct 2021 UTC.

This X1.0 X-ray flare that erupted from Active Region 12887 (we typically drop the left-most digit when referring to an active region, so this is AR2887) is the second X-class flare of Solar Cycle 25, as of the time this video goes live.

The first X-class flare occurred on 3 July 2021 and measured X1.59. It, too, caused an HF radio blackout. These blackouts will occur more often as the cycle activity increases, because the higher sunspot activity leads to many more flares, and thus cause the geomagnetic storms as the typical CME is erupted out into space, possibly colliding with Earth’s magnetosphere.

Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. When intense enough, they can disturb the atmosphere in the layer where GPS and communications signals travel. Some of these disturbances to communications are called radio blackouts. They cause the lower layers of the ionosphere to become more ionized, which results in the absorption of shortwave radio frequency signals.

This flare on October 28 was classified as X1.0 in intensity. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, and so on. Flares that are classified X10 or stronger are considered unusually intense.

This was the second X-class flare of Solar Cycle 25, which began in December 2019. A new solar cycle comes roughly every 11 years. Over the course of each cycle, the Sun transitions from relatively calm to active and stormy, and then quiet again; at its peak, known as solar maximum, the Sun’s magnetic poles flip.

Two other eruptions blew off the Sun from this active region: an eruption of solar material called a coronal mass ejection and an invisible swarm of solar energetic particles. These are high-energy charged particles accelerated by solar eruptions.

Credit: NASA/GSFC/SDO

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73 de NW7US dit dit

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Hello and welcome to the 438th episode of Linux in the Ham Shack. In this short-topics episode, the hosts discuss the educational possibilities of ham radio, the proliferation of 5G, Russia and Ukraine's radio war, tiny satellites, tiny utilities , multi-radio SDRs and much more. Thank you for listening and have a wonderful week.

73 de The LHS Crew

Russ Woodman, K5TUX, co-hosts the Linux in the Ham Shack podcast which is available for download in both MP3 and OGG audio format. Contact him at [email protected].

Lately, Joyce/K0JJW and I have been doing combined Summits On The Air (SOTA) and Parks On The Air (POTA) activations. Most of the SOTA summits we activate are inside parks as defined by POTA. Our primary focus is using VHF/UHF from SOTA summits with POTA is being a nice addition. Although the two programs have a lot of similarities, there are some significant differences that need to be understood.

SOTA / POTA Differences

Let’s compare the two programs to understand the differences, so you can have a successful activation with both. We will focus on differences when doing an activation so this is not an exhaustive list.

• Summits Vs Parks. Well, this is the fundamental difference. Summits tend to be small in area, defined by a specific lat/lon coordinate and the surrounding activation zone (AZ). The activation zone is roughly defined as the area surrounding the actual summit, staying within 25 vertical meters. Parks can be almost any size and may cover many square miles. Both SOTA and POTA maintain lists of official summits or parks, so it should be clear whether one of these is valid for an activation.
• Accessibility. While there are drive-up and easy walk-up summits, most SOTA summits require a hike. Many of them are physically challenging. Parks often have easier, park-like access. Or you can always do a 50-mile backpack trip for a POTA activation.
• Equipment restrictions. SOTA allows you to reach the activation zone in a vehicle but you must move away from the vehicle an unspecified distant and operate totally independent of the vehicle. On drive-up mountains, our practical application of this rule is to load up our normal SOTA gear into backpacks, hike away from the vehicle, and set up for the activation. SOTA requires the use of portable power sources but not fossil-fuel generators. This pretty much means battery power, perhaps augmented with solar panels. POTA does not have such restrictions, so if you meet the SOTA requirements you’ll be valid for both.
• Scoring. SOTA emphasizes the accumulation of activator and chaser points, while layering in other challenges such as Summit-to-Summit (S2S) scores. Each summit has a point value assigned to it, based on elevation. In POTA, all parks are created equal and the main focus tends to be on the number of activations and the number of parks hunted (chased).  POTA also has awards for the number QSOs. For example, the Kilo Award is achieved by making 1000 QSOs from a single park (usually over multiple activations). Both programs have quite a bit of variety and flexibility built into their awards and operating objectives, which is one of the reasons people enjoy the programs.
• Successful Activation. SOTA requires only one radio contact for a successful activation. But to receive point credit for the summit, which is what most people are after, you need to make at least 4 contacts. So most SOTA activators define success as getting at least four contacts. The 4 SOTA contacts must be with 4 different stations, with no credit for working the same station on multiple bands. In contrast, POTA requires 10 QSOs for a successful activation.  POTA does count QSOs with the same station on different bands. For example, an activator could obtain the required 10 POTA QSOs by working just two stations on 5 different bands.
• Same Location QSOs. A SOTA activator does not get credit for working another station on the same summit. That is, the other station must be outside of the summit activation zone to be counted. POTA allows an activator to work another activator in the same park for QSO credit. In fact, the activators can receive park-to-park credit for such a radio contact.

VHF SOTA and POTA

Racking up lots of contacts on VHF/UHF from a summit can be a challenge, dependent mostly on the range of your gear and the ham population in the area. Most of the time, we can get four contacts without too much trouble but at times even that can be a challenge. Getting ten contacts for POTA raises the bar higher.

We noted that most of the hams we work on 2m FM are also workable on 70 cm FM. So an easy thing to do is to ask 2m chasers (hunters) to switch over to 70 cm and work us there, doubling the number of POTA-valid QSOs. Interestingly, the SOTA QSO count recorded in the database includes these QSOs. (But you must have contacted at least four unique stations to get the summit points.)

Because Joyce and I usually activate together, we can also work each other for POTA credit. I have discovered that many POTA activator teams make it a standard practice to pull out a couple of handheld radios and work each other on 2m FM when they first set up. OK, maybe that’s not the most exciting QSO of the day, but it is allowed.  With a dual-band HT, you can make two QSOs this way. And it is a good idea to put out a call on 2m FM to work any locals that might be hunting parks. On a summit, these QSOs would not be valid for SOTA, unless one of the operators leaves the activation zone. Yes, we’ve done that, too, taking turns hiking down out of the AZ to make a quick contact.

Summary

This covers some of the things we’ve learned about doing combined SOTA and POTA activations. Again, this is with an emphasis on VHF/UHF operating. You should study the SOTA and POTA rules carefully because this article does not cover everything. However, some of the issues I’ve outlined here are not obvious from the SOTA and POTA rules, so I hope you find this article helpful.

73 Bob K0NR

The post Combined SOTA / POTA Activations appeared first on The KØNR Radio Site.

Bob Witte, KØNR, is a regular contributor to AmateurRadio.com and writes from Colorado, USA. Contact him at [email protected].

Ham College episode 82 is now available for download.

Extra Class Exam Questions – Part 20.
E5A Resonance and Q: characteristics of resonant circuits: series and parallel resonance, definitions and effects of Q, half-power bandwidth, phase relationships in reactive circuits.
1:05:41

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YouTube

George Thomas, W5JDX, is co-host of AmateurLogic.TV, an original amateur radio video program hosted by George Thomas (W5JDX), Tommy Martin (N5ZNO), Peter Berrett (VK3PB), and Emile Diodene (KE5QKR). Contact him at [email protected].

 

Yesterday I had a nice relaxing afternoon sitting at the 7610 checking out the bands. Solar conditions have been great the past while and that is a nice change to see.  I was able to work 7P8RU again, and I did see the DXpedition HD8R from Galápagos spotted on DX summit . I was not able to hear them on 20m and barely on 40m, but then I saw them spotted on 17m. I found 17m to be very quiet, and I definitely saw HD8R on the waterfall but no pile up was being shown.  I placed the Icom 7610 in Dual watch and split mode and found HD8R was working many stations, but most if not all I could not hear. The DX stations they were answering were mainly U.S. stations, so I realized the band was open in my direction.  As I listened and I emphasize "listening".  Now and then some U.S. stations were heard at my end working HD8R and this allowed me to get the team's strategy for working DX. 

I blindly threw my call-out a few times, and very soon after I heard VE9KE 599....I came back with VE9KK KK KK and low and behold the call was corrected, and I was in their log. Once again 100 watts and my Endfed antenna came through for me. 

This weekend is the CQWW SSB contest and for the SSB folks this is a big one. There is going to be lots of rare DX to be had for sure. For me I am a CW guy and not because I snub SSB but because in the past when operating SSB I have caused issues with neighbours. I am going to see if the rare CW stations have less of a pileup this weekend because of the SSB contest and many will be operating in that. 

Mike Weir, VE9KK, is a regular contributor to AmateurRadio.com and writes from New Brunswick, Canada. Contact him at [email protected].

It's time once again for The Weekender. This is our bi-weekly departure into the world of amateur radio contests, open source conventions, special events, listener challenges, hedonism and just plain fun. Thanks for listening and, if you happen to get a chance, feel free to call us or e-mail and send us some feedback. Tell us how we're doing. We'd love to hear from you.

73 de The LHS Crew

Russ Woodman, K5TUX, co-hosts the Linux in the Ham Shack podcast which is available for download in both MP3 and OGG audio format. Contact him at [email protected].