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This is a theoretical look at propagation on 630-Meters and 2200-Meters using ray tracing software. It expands on the brief discussion in the ARRL Handbooks. The Earth's magnetic field affects 630-Meter and 2200-Meter band propagation. Lower ionization reduces absorption, aiding low-frequency propagation. Differences exist between bands, limited daytime sky-wave propagation. Sunrise/sunset show promise, yet mechanisms are unclear. Ducting possible at night in specific conditions. Negative ions enhance propagation. Inefficient antennas and high man-made noise are anticipated. Groundwave propagation is significant on 2200-Meters.

The author struggled with receiving antennas on his property. After a standard Beverage on Ground (BOG) antenna failed, he built a Reverse Beverage on Ground (RBOG) using telephone cable. He details construction and testing, finding the RBOG outperformed other antennas in noise level, signal strength, and reception pattern. Software modeling helped optimize the antenna length. Unfortunately, the project ended when telephone cable from the second RBOG was stolen.

This article explores Beverage antennas, a type used for low-frequency radio reception. Despite the mystique, they are relatively simple wire antennas placed near the ground. Their key benefit is improved signal-to-noise ratio by rejecting unwanted signals. While lengthier antennas offer better reception, even shorter versions (around 200 feet) can improve DX reception compared to traditional antennas.

Understanding how radio frequency interference (RFI) is coupled into equipment and subsequently detected is crucial for amateur radio operators. This guide delves into the fundamental mechanisms of RFI, particularly focusing on detection at semiconductor junctions and the unintended antenna action of system wiring. It explains that most RFI detection follows a square law, meaning a 6 dB reduction in RF signal can result in a 12 dB drop in detected audio, offering a practical approach to mitigation. The resource also clarifies the concept of common mode versus differential mode signals, detailing how cable imperfections can convert common mode antenna current into differential signals. It addresses the critical "Pin 1 Problem" in audio interfacing, a common design flaw where cable shields connect to the circuit board instead of the shielding enclosure, leading to significant RFI issues. Practical solutions, such as proper shielding, using twisted-pair cables, and strategic bonding of equipment, are discussed to effectively reduce or eliminate RFI. The guide emphasizes the importance of proper filtering and the often-misunderstood concept of "ground" in electrical systems, distinguishing between earth ground, equipment ground, and circuit common. It provides insights into minimizing loop area in wiring to reduce inductively coupled noise and antenna action, drawing on the author's extensive engineering background and ham radio experience.

Demonstrates the construction of an active loop converter specifically designed for the Low Frequency (LF) bands, addressing common localized noise interference in LF reception. The design integrates a sharply tuned circuit and a tuned loop antenna, utilizing the loop as the sole tuned inductive element. By applying positive feedback, the converter significantly increases the loop's effective Q, achieving factors between 1000 and 2000, which sharpens tuning and reduces noise. The circuit employs an _NE602_ mixer stage, feeding its output to an HF receiver, with a crystal-locked local oscillator at 4 MHz. A 20-turn, 0.8-meter square loop antenna with 500 uH inductance is detailed, connected via 2 meters of figure 8 flex cable. The converter offers three selectable frequency bands: 195-490 kHz, 150-220 kHz (including the New Zealand amateur band), and 128-160 kHz (covering the European amateur band). Performance measurements indicate an effective 3dB bandwidth of approximately 100 to 200 hertz at 200 kHz. The article provides insights into component selection, including an _LF353_ op-amp and a trifilar wound transformer on a ferrite core. Sensitivity figures are presented, showing 7.5 uV of converted output per 1 uV/meter signal strength into a 50-ohm load, or 37.5 uV into an _FRG7_ receiver, highlighting its capability to extract weak signals from noise.