Archive for the ‘crossband’ Category
Coast Guard Cutter Chelan: Biggest, Costliest Coast Guard Vessel of its Era
Take a step back in time to November 26, 1928, and take a look at what was then described as the biggest and costliest Coast Guard vessel of its era. The photograph shows the state of the art radio room aboard the U.S. Coast Guard Cutter Chelan. At the time this photo was taken, she was the newest cutter in the service, proudly anchored at the Navy Yard in Washington D.C.

Coast Guard Cutter Chelan
Constructed at a staggering cost of approximately $1,000,000 (1928 Dollars), the Chelan proved her incredible value right out of the gate. On her maiden trip, she picked up a desperate SOS signal and successfully towed a disabled schooner 1,500 miles to safety. This remarkable feat stood as a record tow for the service.
Chelan was laid down by Bethlehem Shipbuilding Corporation at Quincy, Massachusetts, on 14 November 1927 and launched on 19 May 1928. She was commissioned into U.S. Coast Guard service as USCGC Chelan on 5 November 1928.

Turbo-electric cutter, Lake-class (250-footers), built by Bethlehem Shipbuilding Corporation, Quincy, MA, at cost of $900,000 (hull & machinery), launched 19 May 1928, commissioned 5 September 1928, 2,075 tons displacement, 250ft long x 42ft beam x 12ft 11in draft, 17.5kts, armed with 1-5in/1-3in/2-6pdr (1929), 97 crew (1940).
The USCGC Chelan (WPG-45) was a 250-foot Lake-class cutter belonging to the United States Coast Guard, launched in 1928. Best known for its extensive operations in Alaska and a dramatic 1937 North Atlantic rescue, the ship was transferred to Great Britain during World War II.
Sitting at the operator station is Ensign Leslie B. Tollaksen. Tollaksen would go on to have a highly decorated military career, eventually serving as a Lieutenant Commander in World War II where he commanded a naval frigate, the USS Moberly, that helped sink a German submarine in the final days of the Atlantic naval war.
We see Tollacksen in the photo above as a fresh ensign aboard USCGC Chelan. From a genealogy page:
Tollaksen “attended the University of Washington for two years before going and graduating from the US Coast Guard Academy in New London, Connecticut. He graduated from The USCG Academy in the Class of 1927, a year early to man the ships chasing down rum runners.
As a young Lieutenant, he was assigned to the US Coast Guard HQ in Washington, DC. He helped establish “Radio Washington” the telegraph station on Telegraph Road in Washington, DC, and also served as Aid to the Secretary of the Treasury, Henry Morgenthau, Jr. (At that time, his sister worked in the typing pool for President Franklin D. Roosevelt’s White House).

Leslie Bliss Tollaksen (1903 – 1973), Also nown as,”Tolley”
Birthdate: April 13, 1903, Port Townsend, Jefferson County, Washington, United States. Death:1973 (69-70), Fort Lauderdale, Broward, Florida, United States
Leslie, about 1937 was the first US Coast Guard Officer selected for Post Graduate School at MIT.
Leslie, during WWII, and in command of the USS Moberly, sank the LAST German U-Boat U-853. U-8533 was a Type IXC/40 U-Boat, and lays on the bottom off Block Island…”
For history and technology buffs, the equipment in this radio room is absolutely fascinating. In 1928, maritime communication was undergoing a major technological revolution. Global maritime operations were beginning to phase out the older, notoriously noisy spark gap transmitters. Instead, the Chelan was outfitted with modern continuous wave vacuum tube technology. This room housed three powerful transmitters and three highly sensitive receiving sets.
If you look closely at the right side of the image, you can see the large glass vacuum tubes safely housed behind protective metal mesh doors. These power tubes allowed operators to transmit signals on specific, sharply tuned frequencies, reaching much further out to sea without causing interference for other ships. The tall black panels are also loaded with large rheostat dials for tuning, as well as precise ammeters and voltmeters to monitor the high voltages running through the system.
Meanwhile, Ensign Tollaksen has his hand positioned near a traditional straight telegraph key to send out Morse code. The receiver units he operated likely utilized regenerative or early superheterodyne circuits, giving operators the incredible sensitivity needed to hear faint SOS calls through heavy atmospheric static. It was exactly this kind of cutting edge machinery that allowed the crew to hear the distress call that led to their record breaking rescue!

USCGC Chelan was a Lake-class cutter belonging to the United States Coast Guard launched on 19 May 1928 and commissioned on 5 September 1928. After 13 years of service to the Coast Guard, she was transferred to the Royal Navy as part of the Lend-Lease Act, and named HMS Lulworth (Y60). During the war Lulworth served in a convoy Escort Group for Western Approaches Command. She returned to the U.S. Coast Guard after World War II.
USCGC Chelan was a Lake-class cutter belonging to the United States Coast Guard launched on 19 May 1928 and commissioned on 5 September 1928. After 13 years of service to the Coast Guard, she was transferred to the Royal Navy as part of the Lend-Lease Act, and named HMS Lulworth (Y60). During the war Lulworth served in a convoy Escort Group for Western Approaches Command. She returned to the U.S. Coast Guard after World War II.
Read more about this vessel: https://en.wikipedia.org/wiki/USCGC_Chelan.
GERMANY: USAGM Shortwave Operations Return to Lampertheim

Following the recent suspension of Voice of America (VOA) shortwave and medium-wave (AM) transmitters, the U.S. Agency for Global Media (USAGM) is orchestrating a gradual return to the airwaves.
Starting next week, USAGM will begin testing shortwave transmissions from the historic Lampertheim site in Hesse, Germany, which formerly served as a primary broadcasting node for Radio Free Europe and Radio Liberty (RFE/RL). This reactivation indicates that USAGM is working to restore its global broadcast capacity after surviving a period of severe operational cuts and the near-abandonment of its legacy transmission centers.

Lampertheim joins a growing list of international USAGM transmitting stations seeing renewed activity, including sites in Marathon (Florida), Greenville (North Carolina), Kuwait, the Philippines, Botswana, and Thailand. The permanent commissioning of these shortwave sites will depend heavily on the results of ongoing signal testing. The Lampertheim reactivation may ultimately serve as a temporary measure while USAGM awaits the completion of a major transmitter installation and upgrade project currently underway at the Kuwait Transmitting Station.

Built in the early 1950s during the height of the Cold War, the Lampertheim site was an RF (radio frequency) powerhouse, ruling the airwaves with eight massive 100 kW shortwave transmitters designed to pierce the Iron Curtain. Following the corporate merger of RFE and RL in 1976, the station broadcasted both services simultaneously. In 1995, under the newly formed Broadcasting Board of Governors (BBG–the predecessor to USAGM–the station became a consolidated hub for American international broadcasting.

The fall of the Soviet Union and the subsequent independence of Eastern European satellite states drastically altered the station’s mission. The target areas for Lampertheim’s massive curtain antennas were no longer geopolitical priorities, and direct shortwave programming was shrunk to almost nothing.

Instead, Lampertheim’s primary mission shifted toward technical, administrative, and logistical support. It became a vital satellite uplink and distribution gateway, beaming TV and radio programming to relay stations across Europe, Asia, and the Middle East. It also functioned as the remote-control nerve center for USAGM’s global network of transmitters, which included the medium-wave transmitter in Cape Greco, Cyprus (installed at the former RMC Middle East Transmitter Center), the strategic relay station in Djibouti, the massive 1,000 kW medium-wave transmitter in Orzu, Tajikistan, and, Technical oversight for nearly a hundred USAGM-affiliated FM transmitters globally.

During the wars in Afghanistan and Iraq, Lampertheim saw a brief resurgence in direct broadcasting as antennas were reconfigured to target the Persian Gulf and Southwest Asia, filling coverage gaps left by the Kuwait transmitters.

Today, radio enthusiasts and DXers can track the ongoing progress of USAGM’s shortwave broadcasts by consulting the HFCC A26 (Summer 2026) seasonal schedules here: HFCC A26 Schedule: https://new.hfcc.org/data/schedbybrc.php?seas=A26&broadc=AGM

A Pileup? What It Is And How To Work One
Welcome to the chaotic, thrilling world of the HF pileup. Whether you are the one calling CQ from a park in Nebraska or the one hunting a rare DX station, success relies on rhythm, frequency management, and a deep understanding of human behavior.
Here is a proper look at how a pileup appears on a modern display, followed by a complete guide on how to survive it.

A “pileup” on shortwave amateur radio frequencies. The main station is at the low frequency, and stays put. The hunters spread out, above, and call on a single frequency somewhere in the calling window of frequencies (I.e., up five to ten).
Over my decades of working Morse code (CW on amateur radio), I have learned a few critical things about how to navigate the chaotic, thrilling world of the HF pileup. When a rare station or a Parks On The Air (POTA) activator goes on the air, dozens or even hundreds of operators might try to make contact at the exact same time. Working a pileup is an art that takes time to master. Whether you are the one calling CQ from a park in Nebraska or the one hunting a rare DX station, success relies on rhythm, frequency management, and a deep understanding of human behavior.
One of the most important strategies is to determine the operating style of the DX station, specifically discerning how that operator scans the pileup for the next station to work. With modern waterfall displays, that process is MUCH easier. As an example, I worked the Temotu DXpedition (H40RH) that had just started a few hours prior to my attempt. I broke through with only five calls into the pileup, and it took me a mere 60 seconds to call and get an answer. Of course, I first listened and watched the waterfall for about five minutes to get a hang of the operating style of H40RH. This was on 10 Meters where 28.026 MHz was the DX frequency. We callers spread out five to 15 kHz UP in frequency from the DX station because we never want to cover up the DX station with our own signals. Even with a long carrier of intentional interference visible on the waterfall, the visual aid of the SDR made the catch possible. Temotu was a new country for my DXCC, so I am incredibly pleased to have made the contact!
When You Are the Hunted (The Activator)
A Guide To Survive The Pileup
When you are the station that everyone wants in their logbook, you are the conductor of the orchestra. If the pileup senses hesitation, chaos ensues. You must dictate the pace, for both CW and SSB operations.
Controlling the Pileup on CW
Establish a Predictable Rhythm: Your CQ, your exchange, and your QRZ should follow a strict pattern. Consistency allows hunters to time their calls perfectly. If you change your cadence, the pileup gets messy.
Run Split for Large Piles: If the pileup merges into a single continuous drone, go split immediately. You might send “UP 1” to tell callers to transmit one kilohertz above your listening frequency. This spreads the callers out. Send your “UP” frequently enough that the self-appointed pileup police do not take over your transmit frequency. I suggest sending “UP” after each successful logged contact (QSO).
Own the Partials: If you only pull “NW7” out of the noise, send “NW7?”. Do not send “QRZ?” immediately. Stick to that partial call until that specific station finishes the exchange. If they fade out, clearly send “QRZ?” to reset the pile.
Adjust Speed to Control Volume: A slight speed increase (bumping up 3 to 5 WPM) will naturally thin the pileup down to the more experienced operators. Dropping your speed will invite the newer operators back in.
Receiver Management: Back off your RF gain and use a wider filter than you might expect (around 400 to 500 Hz). A filter that is too narrow will cause you to miss the operators who are smartly calling slightly off-frequency.
Controlling the Pileup on SSB
Command with Your Voice: Speak clearly and maintain a steady, authoritative tone. Avoid shouting. Just like in CW, a predictable rhythm helps callers know exactly when to key their microphones.
Use Standard Phonetics: Stick strictly to the standard NATO phonetic alphabet (Alpha, Bravo, Charlie). Cute or custom phonetics confuse operators who do not speak English as their first language.
Acknowledge and Isolate: When multiple voices blur together, listen for the last phonetic letter you can understand. If you hear “Sierra,” say “The station ending in Sierra, go ahead.” Ignore everyone else until that station completes the contact.

My POTA / Portable HF station (a low-power, or, QRP, station).
When You Are the Hunter (The Chaser)
When you are trying to break through a massive wall of sound, raw output power is secondary to timing and sharp observation.
Breaking the Pileup on CW
Listen First, Key Second: Before touching the paddle, listen to three or four complete exchanges. If the activator is working split, figure out their pattern. Are they tuning from the bottom up? Top down? Find where they listened last, and place your transmit frequency just above it.
Use XIT (The Golden Rule): Never perfectly zero-beat the DX station if others are calling. To the activator, three zero-beat stations merge into a single tone. Use your Transmitter Incremental Tuning (XIT) to shift your transmit frequency by 30 to 50 Hz. This slight difference in pitch makes your signal pop out of the receiver passband.
Time the Tail-End: Wait for the massive wall of sound to begin fading, and send your call exactly as the main group finishes. A perfectly timed tail-end call lets your suffix ring out in the clear.
Send Once: When the DX sends “QRZ?”, send your callsign exactly once and listen. Sending your call multiple times just causes interference and slows down the entire operation.
Follow Instructions: If the DX sends “NW7?”, and that is not you, keep your hand off the key. Transmitting over the station they are trying to work only prolongs the pileup for everyone.
Breaking the Pileup on SSB
Study the Cadence: Just like with Morse code, listen to the activator to find the rhythm. Wait for the exact moment the activator stops speaking before you key up.
Drop Your Call and Wait: Say your full callsign once using standard phonetics, then unkey and listen. If you are tail-ending, you might just drop the last two letters of your callsign precisely as the noise floor drops.
Adjust Your Pitch: If you have equalization controls on your radio, boost the mid-to-high frequencies on your microphone audio. A slightly punchy and higher-pitched voice will cut through the bass-heavy rumble of a dozen other stations calling at once.
Working a pileup tests your patience and your ear. Whether you are tapping out Morse code or speaking into a microphone, the operator who listens more than they transmit almost always makes the contact first.
Propagation and the Pile-Up
As many of you know, I was the space weather and radio propagation columnist in CQ Amateur Radio Magazine from 2001 through its demise. I strongly advocate for all HF radio operators to understand the basics of radio wave propagation on shortwave frequencies. There are a lot of myths and frankly, horrific theories on how radio waves propagate.
Understanding how the ionosphere refracts radio waves is a crucial tactical advantage. The behavior of a pile-up changes dramatically based on the frequency band you choose and the current mood of our sun.
The Sun Dictates the Rules
The ionosphere is charged by solar radiation. When solar activity is high, higher frequencies become usable for long distances.
Solar Flux Index: The SFI is a great indicator of overall ionization. A higher SFI means better conditions for the higher HF bands. When the SFI climbs, bands like 15, 12, and 10 meters open up globally.
Geomagnetic Storms: Measured by the K-index, these storms can disrupt communications entirely. A high K-index often absorbs signals crossing the polar regions. This can suddenly mute a massive European pile-up for North American operators.
Fading: The ionosphere is always shifting. Signals will constantly rise and fall in strength, which is known as QSB. A smart chaser listens for the rhythm of this fade and throws their callsign into the pile-up exactly when the band peaks for their specific location.
How Bands Shape the Pile-Up
Every amateur radio band has its own personality. The pile-ups you encounter will reflect these differences perfectly.
10, 12, and 15 Meters: These high bands are daytime frequencies that thrive on high solar activity. When 10 meters opens up, signals can be astonishingly loud with very low atmospheric noise. Pile-ups here can ignite suddenly and stretch very wide across the frequency spectrum.
20 Meters: This is the traditional workhorse band for global communication. Pile-ups on 20 meters are massive, sustained, and densely packed. You will often compete with high-power stations and massive beam antennas on this frequency day or night.
40 and 80 Meters: These low bands come alive at night. They are heavily affected by atmospheric noise and static crashes. Breaking a pile-up here requires an exceptionally well-tuned ear and the ability to pull faint CW tones or muffled voices out of a very high noise floor.
The Skip Zone Effect

The propagation of radio waves.
One of the most confusing aspects of a pile-up for a new operator is the skip zone. Radio waves bounce off the ionosphere and return to earth far away, which means they skip right over the geographic areas in between. You might hear the DX station perfectly, but you might not hear the hundreds of other operators calling them because those callers are inside your skip zone. This phenomenon is exactly why you must rely on the DX station’s cadence rather than waiting to hear the pile-up clear.
While raw power is often cited as the key to breaking a pile-up, your antenna system plays a far more decisive role in your overall effectiveness. A directional antenna, like a Yagi or a hexbeam, not only focuses your transmitted energy directly toward the DX station but also actively rejects interfering signals from other directions. However, do not be discouraged if you are running a simple wire antenna. A well-placed dipole or end-fed half-wave can still break monumental pile-ups if you leverage good timing, exploit the skip zone, and listen closely to the DX operator. Ultimately, the best antenna in the world cannot compensate for poor operating habits.
Over to You
Working a pile-up is one of the most rewarding challenges in amateur radio. It tests your patience, refines your ear, and forces you to understand both the science of radio wave propagation and the psychology of your fellow operators. Every massive wall of sound is a puzzle waiting to be solved.
Now, I would love to hear from you. What was your most memorable pile-up experience? Do you have a specific tactic that consistently helps you break through the noise, or perhaps a frustrating moment that taught you a valuable lesson? Drop your stories and questions in the comments below, and let us keep the conversation going.
From my shack to yours, 73 de NW7US.
Powerhouse History: WLW, W8XAL, WSAI
The photograph, below, captures a compelling moment of technical mastery during the formative years of American broadcasting, set deep within the inner workings of the Crosley Radio operation in Cincinnati, Ohio, during the 1930s. This was not just a studio but a nerve center for one of the most ambitious radio experiments in history. In the frame, an unidentified announcer sits with a quiet, practiced focus before a sensitive microphone, his presence framed by a formidable wall of equipment that served as the control interface for Powel Crosley Jr.’s broadcasting empire.

WLW, W8XAL, and WSAI
The machinery in front of him represents the sophisticated control panels for three distinct stations, labeled for WLW, W8XAL, and WSAI. These panels were the operational gateway to a signal that redefined the reach of radio. WLW, in particular, earned the nickname The Nation’s Station, and for a brief but legendary period in the mid-1930s, it was granted special authorization by the Federal Communications Commission to experiment with a massive power output of 500,000 watts. This made it the most powerful radio station in the United States, a true technological titan of the era. The signal was so incredibly potent that listeners across North America and beyond often reported hearing the broadcast under unusual circumstances, such as through the metal teeth of fillings, in the coils of mattress springs, or even through the humming of household plumbing.
Beyond the standard AM broadcast of WLW, the inclusion of W8XAL in this control room highlights the critical role shortwave technology played in the Crosley vision. While the standard AM signal was meant for domestic reach, W8XAL served as an experimental shortwave companion, designed to project the Cincinnati broadcasts far beyond the limitations of local and regional airwaves. Shortwave radio waves possess the unique ability to bounce off the ionosphere, allowing signals to travel thousands of miles and transcend national borders. Through W8XAL, the Crosley organization was testing the feasibility of true international broadcasting, turning the modest studios in Cincinnati into a point of origin for listeners located as far away as South America or Europe.
This shortwave capability was a significant leap in the evolution of mass media. It represented a deliberate attempt to overcome the geographical isolation that had defined the earlier, more fragmented era of radio. By operating on shortwave frequencies, the announcers and engineers were participating in a grand experiment to see if a single localized voice could truly become a global one. It was an ambitious pursuit that demanded even greater precision than standard broadcasting, as atmospheric conditions and solar activity could frequently disrupt the long-distance transmission path.
Working in this control room was a task that required both the poise of a performer and the precision of an engineer. Each dial, needle gauge, and switch was a critical element in maintaining the integrity of the broadcast, as the announcer had to carefully monitor the modulation levels to ensure the signal remained clear and stable for millions of listeners. A lapse in focus could mean a technical failure or a broadcast error that reached a massive, dispersed audience in real time. It was a high-stakes, high-pressure environment, yet it functioned as the primary, and often only, window to the wider world for families weathering the depths of the Great Depression.
Powel Crosley Jr. was a man of intense vision, and he understood better than most that radio was the ultimate tool for domestic and international unification. These transmitters were the engine that bridged the vast geographical distance between his studio in Cincinnati and the living rooms of families scattered across the continent and beyond. When people turned their dials to find the station, they were connecting to a piece of engineering that stood at the very cutting edge of the twentieth century. Looking at this image today, it is easy to feel a sense of awe for that era, when the simple act of turning a knob could bring the world into a home, effectively shrinking the vastness of the country and changing the way society experienced culture, news, and shared humanity forever.
Yet in Quarantine, Life Blossoms!
About a month ago, I asked,
“What is going on with you during this challenging situation?” and, “How do you use amateur radio, now that we are all stuck at home? Are you using ham radio more, now? Less?“
I am moved to say, “Thank you, to each of you who commented and even those who made a video response. I sure appreciate it!“
During that video blog (or, Vlog), back a month ago (link: Chat From a Quarantined Software Engineer – Welfare Check!), I mentioned my need for dental surgery.
I did have to have the tooth removed. It was completely split down the middle (top to bottom), down to the root. There was no justifiable way to save the tooth.
I now am missing two bottom back-most teeth, and one bottom, back-most tooth. I can report that I have healed up nicely. I am starting to enjoy a hamburger or two.
Through all of this, I’ve still been working. Also, I’ve been involved with a LOT more ham radio–especially with Morse code activities.
How has the last month treated you? After watching this new video (below), please leave a comment or two, or three; let hear from you, okay?
More than anything, please leave a comment to let me know how you are doing. I hope to hear from you.
Here’s the video:
[embedyt]https://www.youtube.com/watch?v=vFGbw7d91GA[/embedyt]
73 de NW7US dit dit
System Fusion DR-2X Repeater, Solar Eclipse and More – ETH079

In this episode we talk about the Yaesu System Fusion DR-2X repeater, the upcoming Solar Eclipse and more.
There is some interesting new features on the DR-2X repeater over the DR-1X that came out a couple years ago, but there is also something that it doesn’t have. Some of these features, I wish that we had on our club repeater, but those features are not enough for us to go out and buy this version.
There are a lot of special event stations that are going to be on the air around August 21st this year when the full solar eclipse occurs. This is the first time since 1918 that a full solar eclipse has gone from one side of the US to the other. I unfortunately am to far south to the see the full eclipse, but I should get about a 75% one here in the DFW area.
We also talk about some other stuff, but you are going to have to check out the show notes and listen to the episode to find out what that is.
73s de Curtis, K5CLM
CQ Crossband and … 3 Down, 97 To Go!
Several QSL cards have arrived after the last 630m 'crossband' event ... including one from ZF1EJ in the Cayman Islands confirming our 630m QSO in January.
The contact was made on JT-9, the 'WSPR QSO' mode, and represents DXCC country #3 for me on 630m ... only 97 more to go! ZF1EJ was running just 32 watts output when we had our 630m JT-9 contact but has since cranked his output to around 60 watts. Eden is beaconing most nights on WSPR and puts out a well-heard signal. He is very interested in two-way JT-9 work with other VE stations as well as any Europeans and down-under stations.
From what I can tell, it looks like JT-9 (similar to JT-65 but a much narrower bandwidth of 15.6Hz) is establishing itself as the go-to mode for weak signal two-way work on 630m. It has a couple of things going for it that makes it very attractive for this band ... it can dig way down into the noise (-25 db approximately) and communicate with very weak signals and, it does not require amateurs to know CW, a growing trend with newer operators and a real hindrance to two-way CW work. I suspect, and hope, that there will be much more CW activity on 630m once amateurs in the U.S.A. get the band as the amount of information that can be exchanged per transmission on JT-9 is limited ... time will tell.
In the meantime, here is a request for more two-way 'crossband' CW activity with amateurs in all parts of North America. I have recently totally revised the 'CQ Crossband' page on my website, 'The VE7SL Radio Notebook'. Please note that my web address for well over a decade, is no longer valid and everything has been moved to this new location. If you have the old one bookmarked or are linking to it from your own site, please be aware that previous links will now be dead.
The crossband concept allows amateurs not yet on 630m to still participate in this exciting part of the spectrum ... and to check out their ability to hear anything on MF. If we were to make a schedule for a crossband contact, I would be transmitting on 630m at full ERP while you would be answering on one of the HF bands ... usually 160, 80 or 40m.
I am very much interested in setting up crossband schedules for 630m at any time and can very likely enlist several other VE7s to be there as well so that you can work more than one station. I have full details on my updated 'CQ Crossband' web page but please do not hesitate to give crossband a try!
Roger, VE7VV in Victoria, B.C., recently became the 8th VE7 to muster RF on 630m, with power limited to 1 watt at present. Our contact was on CW while he worked stations in Vancouver on JT-9. Hopefully he will continue to build his station and become more active on the band.
Crossband continues to be a subject of much interest both here and with many U.S. stations that are waiting for the band. Recent cards from Colorado and California, shown below, are the latest to arrive.
K6YK gave me an RST of '519' but explained the reason for this was because he was receiving on his 3 el HF tri-bander which provided the best signal-to-noise value! This is often the case on 630m so try what you have. Many times a 'non-resonant' antenna will pick up less noise and yield the best signal readability.
If you would like to try a crossband QSO, please contact me at VE7SL (at) shaw.ca ... I'll keep the rig warmed up!
















