RADIO WAVE PROPAGATION A REFRESHER BRIEFING
BY: RON, KØMAJ
Introduction
• I’m not a genius and I don’t know everything, I’m just the guy who was selected to make a presentation• I’ve tried to minimize the technical theory and focus on:• Practical concepts• Some info not presented in textbooks• Tips • Techniques• Because of limited time, the focus is on HF
http://www.smeter.net/propagation/sunspots/current-sunspot-cycle.php
The good news: Conditions haven’t been better in 8 years!
Not so good news…
Example of actual current propagation
Today on 10 Meters:England station , 100 W, 20-foot beam, S-9 +10(S-3 on dipole)
• “Propagation” refers to the travel of radio waves from point A to B
• A grasp of propagation theory allows you to be a more professional amateur
• If your radio signal does propagate, who’s out there to receive it?
Propagation
Propagation: If you have it, who’s there to hear you?
SEMO ARC Demographics• Extra = 20• Advanced = 6• General = 15• Technician = 12
• Cape = 22• Jax = 20• Scott = 4• Other = 8
(Wikipedia)
• If you aren’t much interested in HF, you might not be Interested in this topic
• Technicians: HF Phone on 28.3 – 28.5 (worldwide)
• Many clubs have their own stations
• If we had a club HF station, who would be interested?
Terminology:• HF = 3.0 – 30 MHz (80 -10 meters)
• VHF = 30 - 300 MHz
• UHF = 300 MHz - 3 GHz
Propagation varies with many factors, including time of year, time of day, geographical location, solar and geomagnetic activity, weather, power,frequency, and antenna type
Propagation
• Radio waves belong to a family of electromagnetic radiation
• Family includes infrared, visible light, ultraviolet, others
• Radio waves, like light waves and allother forms of electromagnetic radiation,normally travel in straight directions and in all directions away from the source
Propagation
• Radio waves weaken as they travel, from thedispersal of radio energy from its source
• Range = distance a radio signal can be received
• Most propagation at VHF and higher frequency is usually line-of-sight, so earth curvature and obstacles are range-limiting factors
• HF can travel along Earth surface, “ground waves”
• The ionosphere (30-260 miles high) is made up mostly of O2 and N2
• Solar energy, in the form of ultraviolet light (UV) and X-rays going thru atmosphere can convert gas atoms toionosphere layers of ions which can refract radio waves
• The ionization plays basic role in long-distance contacts in amateur bands from 1.8 MHz to 30 MHz
• Maximum one-hop skip is about 2500 miles. Beyond that involves multiple bounces off the ionosphere
• VHF and higher usually pass thru ionosphere to space
• D-layer: (lowest region) can absorb HF radio waves, especially 1.8 – 4.0 MHz during day
(DX net example including Louri)
• E-layer: occasionally patches of the E-layer can become overly ionized and refract even VHF and UHF, called “sporadic-E” propagation
• F-layers: (highest region) refracts HF, divided into two sub-groups
• HF refracted back to earth = “sky wave” or “skip”
• Highest frequency that can be refracted = MUF
• Lowest frequency that can be refracted = LUF
• “Band open” means sky waves are possible
Gray line (twilight)
• Radio wave-absorbing D-layer disappears faster than the higher altitude radio wave propagating F2-layer
WWV
Band Plans (ARRL) (Beacons)
• QRP stations with CW ID
• If you need CW help, get a CW program from SEMOARC.net links
Audio splitter to your computer
NY - Corsica
DX Cluster
Contests
DX Nets
• If you can get through to the state-side moderator, you’ll have a good chance with the DX…
1100Z : 14.2385 MHz every day1430Z : 14.2442000Z : 14.247
• Or, call CQDX yourself
ARRL Propagation Charts (solar flux 146)
MUF Line
LUF Line
MHz
Zulu
• Keep in mind that the earth is round when pointing a directional antenna (central Russia is north of here)
• Some times long path works best, due to the ionosphere situation between two stations, especially if short path >
123
Free HRD Bandscope
Various propagation programs available: Google: “radio propagation software”
• I’m out of time (and ideas)
• You can view or download this presentation from the “Links” section of SEMOARC.NET (viewer)
• Questions / Comments / Discussions?
Time Out
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RADIO WAVE PROPAGATION A REFRESHER BRIEFING
BY: RON, KØMAJ
Conclusion
CQ