Canadian Amateur Radio Basic License Study Guide
Mapleham
π
Sign in
β°
Home
Present Mode
Voice Mode
Practice
Loading chaptersβ¦
Radio Wave Propagation
Introduction
Radio Wave Propagation β ground wave, sky wave, ionospheric layers, MUF, solar activity, sporadic-E, and scatter propagation
Radio Wave Propagation β Three Modes
Ground Wave β follows Earth surface, most effective at MF and lower HF (such as 160 m and 80 m)
Sky Wave β reflects off ionosphere back to Earth, enables long-distance communication on HF
The Ionosphere
Ionosphere β region of upper atmosphere from 60 to 600 km ionized by solar UV and X-ray radiation
Ionospheric Layers β D, E, and F layers; D absorbs lower HF by day and disappears at night
Day vs Night Ionospheric Conditions
Day versus Night β propagation changes from day to night on HF bands
Skip Zone, Skip Distance, and Multi-Hop
Skip Distance β minimum distance from transmitter where sky wave returns to Earth
Skip Distance Factors β greatest when MUF is just above the operating frequency; higher MUF means shorter skip for a fixed frequency; multi-hop extends range
MUF and LUF
MUF β Maximum Usable Frequency, the highest frequency that returns to Earth via sky wave at a given angle
MUF Variation β varies with ionization, at solar maximum MUF can reach 30 MHz or more, check by listening for signals on the band
D-Layer Absorption and Fading
D-Layer Absorption β absorbs lower HF by day, 160 and 80 metres have no long-distance sky wave during daylight
Fading β signal strength variation caused by multi-path, multiple signal paths arriving at different times
Solar Activity and the Sunspot Cycle
Sunspots β dark regions indicating high solar magnetic activity, more sunspots mean more ionization and better HF
Solar Cycle β approximately 11 years, solar maximum gives high MUF and good DX on high bands, solar minimum gives lower MUF and better low bands
VHF Propagation β Sporadic-E and Tropospheric Ducting
Sporadic-E β patches of intense E-layer ionization that enable VHF skip on 6 metres and sometimes 2 metres
Tropospheric Ducting β VHF and UHF signals trapped in temperature inversion layer, extends range beyond line of sight
Scatter Propagation
Scatter Propagation β small fraction of signal scattered by irregularities in the ionosphere or troposphere, weak but usable
Chapter 7 β Key Takeaways
Ground Wave β follows Earth surface, best on low HF, limited range. Sky wave refracted by ionosphere for DX. Line of sight primary on VHF and above
Ionosphere Layers β D absorbs day only, E occasional 6 metre skip, F1 and F2 for HF DX, F2 most important
Skip Zone β dead zone between ground wave limit and sky wave first return point. Lower radiation angle produces longer skip distance.
MUF and LUF β MUF is highest frequency returning to Earth, LUF is lowest usable before D-layer absorption, listen for signals to check MUF
D Layer and Fading β D layer absorbs lower HF by day, fading from multi-path, SID from solar flare shuts down HF for minutes to hours
Sunspots and Solar Cycle β sunspots increase solar radiation, raise MUF, improve HF. 11-year cycle with solar max opening high bands
Sporadic-E and Tropospheric Ducting β Es provides VHF skip on 6 metres, tropospheric ducting extends VHF and UHF range
Scatter Propagation β weak signals heard in skip zone, works above MUF, includes auroral scatter on VHF with distorted signal
×
Search Results
×
Cookies help to make this site better. 🍪
Learn more
Accept
Reject