Home >Documents >Intermediate Course (6) Propagation Karl Davies Intermediate Course (6) Propagation Karl Davies East...

Intermediate Course (6) Propagation Karl Davies Intermediate Course (6) Propagation Karl Davies East...

Date post:01-Apr-2015
View:214 times
Download:0 times
Share this document with a friend
  • Slide 1

Intermediate Course (6) Propagation Karl Davies Intermediate Course (6) Propagation Karl Davies East Kent Radio Society EKRS 1 Slide 2 Velocity of Propagation Candidates should know the formula v = f x. Try to remember another triangle formula. vis the speed of radio waves / light :- v = 300,000,000 m/s. f is the frequency in Hz. is the wavelength in metres. v f Example: What's f = 3.7MHz = 300,000,000 3,700,000 Or 300 3.7 Thus = 81.08 metres 2 Slide 3 11 Year Sunspot Cycle 11 year sunspot cycle; more sunspots leads to higher ionisation. More sunspots gives better HF propagation as a result of increased ionisation. The higher the ionisation, the better the reflection, and the higher the HF frequencies can be reflected. 3 Slide 4 Ionosphere D,E and F1/F2 The basic structure of the ionosphere: D, E and F1 & F2 layers Ionisation is caused mainly by ultraviolet rays from the sun Ionisation makes the gasses partially conduct which causes the refraction (bending back) of HF radio waves. 4 Slide 5 Ionosphere Day and Night The F layer is the main layer reflecting HF signals. The level of ionisation changes with the time of day and the time of the year. Ionisation greatest during the day/early afternoon. Because its colder the F layer remains more ionised in the winter. F1/F2 merge layers and remain ionised overnight, but is much weaker. Night-time Daytime 5 Slide 6 Propagation Day and Night F1/F2, E, D layers are ionised during the sunlight hours. HF propagation over great distance is possible. On LF bands range is relatively similar. F1 /F2 (no E, D) layers merge and remain ionised overnight but are much weaker. HF propagation over great distances reduces. On LF bands range is better. < Daytime Night-time > 6 Slide 7 Ground Wave, Skip Distance & Skip Zone Ground wave hugs earth but quickly gets weaker, range only a few km at best. Skip distance is measured from transmitter to first point of skywave return. Skip zone is annulus between ground wave coverage and return of sky wave. No signal is received in the skip zone. 7 Slide 8 Propagation at VHF VHF signals can occasionally be increased by reflection of highly ionised areas in the E layer (Sporadic E). Small areas of the E layer can become very highly ionised so that VHF signals can be reflected. This allows the signals to be received at distances up to 2000km. Sporadic E is the most common mode of VHF dx communication. 8 Slide 9 VHF & UHF Signals VHF and UHF normally go through ionosphere and can reach satellites or the moon. Signals from satellites (satellite TV) travel down through the ionosphere. Sporadic E is as its name suggests - sporadic and unusual. At these frequencies propagation is within the troposphere, which is situated below the ionosphere. 9 Slide 10 Tropospheric Ducting High atmospheric pressure can cause tropospheric ducting to extend the range of VHF and UHF signals to beyond the normal line of sight. The basis of ducting is that the wave is trapped vertically either between two atmospheric layers or between the ground and a layer. This occurs at relatively low heights. Tropospheric ducting is the most common mode of dx communication for UHF signals. 10 Slide 11 Attenuated UHF and Higher Frequency Signals Snow and ice and heavy rain can attenuate UHF and higher frequency signals. Even professional microwave links can drop out if the rain is very heavy. Heavy rain can affect satellite TV downlinks. 11 Slide 12 Other Mode of Propagation Not for the Exam Aurora On SSB, no tonal content to voice, whisper-like sound 12

Popular Tags:

Click here to load reader

Reader Image
Embed Size (px)