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This document outlines the construction of a simple microwave noise source, leveraging mixer diodes, potentially from _John Watson, VE3EZP_'s collection. The design provides a basic schematic for a noise generator, primarily intended for go/no-go receiver sensitivity checks and comparative noise figure assessments. It produces noise levels approximately 20 dB above thermal noise, making it suitable for AM/SSB/CW receivers, but it is not calibrated for absolute noise figure measurements. The construction utilizes surface-mount components on 1/16 inch FR4 PC board, demonstrating functionality up to at least 10 GHz. An alternative version incorporating a _1N21_ diode is noted to operate effectively up to 5.76 GHz. The resource specifies that any microwave detector diode with a reverse breakdown voltage of a few volts is suitable for this application, providing practical guidance for replication.

Icom IC-R75 tabletop HF communications receiver came onto the market back in 1999 and was taken out of production in late 2015. Frequency coverage is from 30 hz right to 60 MHz. This allows one to catch the 6 Meter amateur band as well.

Make an otherwise fine radio even better, change one resistor and one capacitor in the audio section

LZ QSL printing serivice have more than 25 years experience with QSL printing. First started as Gold Print Service in 1997 presented by LZ3HI. It provides other printed products for commercial or personal use such as Amateur Radio World Map, Eyeball cards, Business cards, Calendars, Posters, Flyers, Pens etc

Demonstrates a specific impedance matching technique for resistive loads ranging from 22.2 to 45 ohms, connecting them to a 50-ohm transmission line. The method employs series sections of 50-ohm and 75-ohm coaxial cables, with graphical data illustrating the required cable lengths (L1 and L2) in wavelengths for a perfect match. This approach is particularly useful for feeding **vertical** and **Yagi antennas**. The resource provides a practical example of matching a 25-ohm Yagi antenna at 50.150 MHz, specifying the use of RG-58C/U (50 ohms) and RG-59B/U (75 ohms) cables, both with a 66% velocity factor. It calculates the precise physical lengths in centimeters and inches for the required cable sections. Additionally, the document briefly discusses integrating a balun at the load end, suggesting methods such as coiling a cable section or utilizing ferrite beads to create a W2DU-type balun. The presented methodology offers a clear, data-driven solution for common antenna impedance challenges.

The 2026 Sable Island DXpedition (CY0S) announcement details an upcoming 10-12-day operation from March 19-31, 2026, following an invitation from Parks Canada - Sable Island. The team, largely drawn from the 2024 CY9C DXpedition, includes Murray **WA4DAN** and Glenn **WØGJ** as co-leaders, with Larry WØPR managing publicity and fundraising. Bill K5DHY will handle OQRS QSL cards and serve as treasurer, while Chaz W4GKF maintains the CY0S.com website. Logistical information specifies Sable Aviation will provide flights to the island, landing on a suitable south-facing beach area, acknowledging potential flight delays. Sable Island, located approximately 300 km east of Halifax, Nova Scotia, is described as a 40 km long, 1 km wide sand island with no trees, anticipating cold, windy, and snowy conditions during March. The resource also notes the availability of a dedicated Japanese website and accepts donations via the CY0S website.

Details the construction of a **wideband noise source** for HF filter alignment, specifically targeting transceivers such as the Elecraft K2. The design modifies a Down East Microwave (DEMI) MMIC amplifier board, part number MMICPCB, by integrating a 1N4735A zener diode, 560-ohm resistors, and 4.7 nF, 10 nF, and 22 µF capacitors. This modification enables the board, originally configured for a MAR-6 MMIC (with MAR-1 as an alternative), to generate noise suitable for procedures like the K2's "CAL FIL" function. The resource provides a **schematic** and a comprehensive bill of materials, including specific component values for replication. It outlines the practical steps involved, such as removing the input connector and integrating the new components into the existing MMIC amplifier board layout. The output is optimized for wideband HF applications, ensuring compatibility with various filter alignment tasks. This project focuses on practical implementation, demonstrating how to repurpose readily available components for a critical test instrument. It offers a cost-effective alternative to commercial noise sources, leveraging existing amateur radio hardware for enhanced station maintenance and performance.

The Alfa Alfa (AA) DX Group, established on March 1, 1974, in the Netherlands, is presented as the pioneering Dutch 27mc DX group. It details the group's historical significance, particularly its revolutionary use of the '000' club callsign (19AA000) which influenced international 11-meter group callsign structures. The resource outlines the group's re-establishment in 2024, inviting new active CB operators and _Short Wave Listeners_ (SWL) to join its ranks, emphasizing a free worldwide membership model. Membership requirements are specified, focusing on active participation with an assigned AA callsign. The group provides QSL card management services, with options for direct QSL requests requiring **3 USD** and a Self-Addressed Envelope, or **4 USD** via PayPal for expenses. It also mentions upcoming initiatives like an _AA DX Contest_ and an award program, with sections for certificates and plaques currently under construction. The site also lists useful CB resources, including an 11M DX Cluster and an 11M Callsign Database, and provides contact information for the founder, 19AA001 Mr. Theo, and the Worldwide QSL Manager, 178AA001 Mr. Emil, based in Bulgaria.

This project describes a high-performance EME antenna array consisting of two home-designed 9-element Yagis, each about 2.5 wavelengths long, combined into a 25-ohm system and matched to 100 ohms using 9/4λ sections of 50-ohm coax. The array supports rotatable polarity from 0° to 180°, allowing both horizontal and vertical polarization to optimize moonbounce performance under varying conditions. Despite operating for years without a balun—something another designer called “disastrous”—the system has delivered strong results, including copying very weak DX such as VK3KH at about -25 dB with only 120 W (around 2 kW ERP). The builder continues to refine the mechanics, having installed new gear motors and an upgraded follow-up control system in 2011.

Since 1988 and after few decades of activities, Romeo Charlie is an International DX group and counts more than 1700 members in 150 divisions. Serious QSL management * Unique eQSL system, cluster & spot-push-notifications. * Online logs monitors. * Free contests, trophies & Challenges. * Activations all around the world. * Free fee for most of divisions. * Personal web page for members. * One of the most active DX group on 11m band. It's time for a change... Join a modern DX group... Looking to the future !

This resource details **cooling modifications** for Ameritron AL82, AL1200, and AL1500 HF amplifiers, specifically addressing heat issues encountered during high-duty-cycle digital mode operation. The author, WD4NGB, observed excessive heat in the tank area and band switch on an AL82, attributing it to insufficient exhaust over the 3-500 tubes and a complete lack of exhaust over the tank area. The modifications aim to prevent common failures such as damaged band switches and deformed insulating materials by increasing airflow and exhaust area. The page describes adding five holes to the chassis for enhanced cooling to the band switch and tank area, alongside enlarging the exhaust area over the inner 3-500 tube and the tank area on the amplifier cover, utilizing expanded metal for safety and RF shielding. The original cover featured 26.25 square inches of exhaust; the modified version significantly increases this to 48.5 square inches over the tubes and introduces an additional 15 square inches over the band switch. These changes are intended to resolve heating problems encountered during heavy, 100% duty cycle use in modes like RTTY or long SSB contests, which typically generate substantial heat. The article also discusses upgrading to a higher output fan, such as the G2E085-AA05-21, and modifying tube sockets for improved airflow and reduced back pressure, citing Tom Rauch (W8JI) of CTR Engineering as a source for parts.

QRZ Label is a Windows application designed for amateur radio operators to generate QSL labels using _Zebra (ZPL)_ label printers. It interfaces directly with QRZ.com to retrieve callsign and address details, and can import QSO log data from the QRZ Logbook. The software then formats this information into various label types, including standard address labels, envelope labels, greeting labels, and multi-QSO confirmation cards, all featuring an on-screen tabbed preview. The application supports the creation of QR-code labels, specifically a "QRZ Link" type, which can streamline the QSL process by providing a scannable link to the contact's QRZ.com page. This functionality enhances the traditional QSL card exchange with modern digital convenience. Developed by K7CTV, QRZ Label offers a practical utility for hams managing their QSLing workflow, providing a **free** solution for printing professional-looking labels directly from their station data. The software is distributed as a signed Windows installer.

The Spartan Sprint Special 40m CW Transceiver, originally documented in 2002 and reproduced in 2019, details a **QRP** direct conversion rig designed for portable operation. This project evolved from an experimental CMOS digital IC receiver, which proved too noisy for weak signals, into a dedicated 40-meter CW transceiver. The author, VE3SMA, aimed for reduced size, lower weight, and decreased receive current drain compared to earlier iterations, drawing on his extensive contesting experience and even his time operating million-watt transmitters at Radio Canada International. This compact transceiver delivers approximately 200 mW output, VFO-tunable over 15 kHz within the 40m band, and weighs a mere 73 grams (0.16 lb) including its balsa wood case. It features fast semi-break-in and sidetone, with a receive current draw of about 14 mA (no signal) and transmit current draw around 125 mA key down. The design incorporates various construction techniques, including knife-cut surface mount boards and through-hole components, often salvaged from junked cordless phones and cellphones. Despite its direct conversion architecture, which offers usable but not superheterodyne-level selectivity, the rig proved effective, achieving a fourth-place finish in a June 2001 Spartan Sprint contest when paired with a 26-foot vertical antenna. The article provides comprehensive circuit details, including an unconventional VFO using a high-speed CMOS inverter chip and a balanced mixer utilizing a 74HC4053.

The HD8G DXpedition will take place in the stunning Galapagos Islands from April 18 to April 26, 2025. This operation will involve 26 dedicated amateur radio operators activating the islands, which are designated as IOTA SA-004. The team aims to make a significant number of contacts, providing an exciting opportunity for DXers and enthusiasts to work this unique location. With a rich history and diverse wildlife, the Galapagos Islands offer a picturesque backdrop for this event. Participants can expect to engage in various modes of operation, including SSB and CW, as the team works to log as many QSOs as possible. The DXpedition is anticipated to generate a high volume of activity, with operators from multiple countries contributing to the effort. This is a prime opportunity for those looking to add a rare entity to their DXCC list or simply enjoy the thrill of working a special event from a remote location.

QSL cards remain the preferred method for confirming QSOs, especially when received free via bureau. They capture the personality of the station operator and offer varied designs. Proper sorting by country and correct card dimensions are crucial for efficiency. Despite modern alternatives, QSL cards retain their charm, but ensuring compliance with bureau requirements and understanding international practices is essential.

Home page of CE3SAD with information on his activity and progress expecially on the six meters band with audio recordings of some 50 MHz QSOs.

Demonstrates the conversion of an _Elecraft K2_ QRP HF transceiver to serve as a 2-meter Intermediate Frequency (IF) rig for microwave transverters, addressing the obsolescence of older _Yaesu FT-290R_ units. The project integrates a _DEMI 144-28DC_ transverter board, configured for a 28 MHz IF, and details the necessary modifications to the K2, including the installation of the K160M module for a separate receive-only antenna input and the KSB2 SSB module for voice operation. The modified K2 provides a stable 1-watt output for the 2m IF, utilizing the QRP antenna jack for transmit and the K160M input for receive, with a custom PTT control circuit. The article outlines the physical integration and electrical interfacing, including the design of an internal attenuator for the 28 MHz IF output and a control circuit for the 144 MHz interface. It also covers the construction of a medium power amplifier using an _MGA-31389 MMIC_ to boost the 2m output to 100 mW, matching the original FT-290R performance. Performance measurements for the amplifier, including output power versus input power and gain versus frequency, are presented. The project culminates in a fully integrated solution, with schematics and photos illustrating the internal wiring and external connectors. The modified K2, dubbed the "K290R," was successfully deployed in the 2017 _ARRL 10 GHz and Up Contest_ with a _Kuhne 10 GHz_ transverter, demonstrating reliable operation for CW and SSB modes.

QSL card printer service based in Spain