propagation of radio waves

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Propagation of radio waves

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Propagation of radio waves. Ways of travelling. Propagation in ionosphere Propagation in troposphere Special ways of reflecting Propagation depends on the properties of the medium frequency weather, time of day, sun activity. Propagation in ionosphere. - PowerPoint PPT Presentation

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Page 1: Propagation of radio waves

Propagation of radio waves

Page 2: Propagation of radio waves

Ways of travelling

• Propagation in ionosphere• Propagation in troposphere• Special ways of reflecting• Propagation depends on

– the properties of the medium – frequency– weather, time of day, sun activity

Page 3: Propagation of radio waves

Propagation in ionosphere

• Solar radiation (UV, X-ray) partially ionize the atmosphere

• Ionization depends on the density of the gases• Waves reflect (refract) from the ionized layers• Directly dependent

– on day of time, most neutralized just before sunrise– actitivity of sun

• sun spot number• solar flux

Page 4: Propagation of radio waves

• Ionization level and reflection properties divide the ionosphere in different layers:– D: 55-90 km– E: 90-150 km– F: 150-400 km

Page 5: Propagation of radio waves

D layer

• lowest layer: exist only during daylight• unsuitable for contacts, absorbs radio

energy• 7 & 10 MHz can travel through at high

angles

Page 6: Propagation of radio waves

E layer

• A bit more stable layer, disappears at night• Skip from E layer is limited by D

– hard to distinguish from F layer propagation– longest one skip range is ~2000 km

• home for other interesting ways of propagation– Es– Aurora, meteor scatter

Page 7: Propagation of radio waves

F layer

• Divided in two during daytime F1, F2– F2 more important, never absent– one skip almost 4000 km, multihops even

longer• reflects from ground, E-layer once or several times

• Controlled by sun activity

Page 8: Propagation of radio waves

Propagation in troposphere

• VHF, UHF & microwaves• weather effects• tropospheric scattering primary form

– rain, fog, dust, snow, clouds• ducting• Radiation inversions:

– air layers with different temperatures and dew points– can travel long (1500 km)– calm summer evenings

Page 9: Propagation of radio waves

Other forms of propagation

• Aurora• EME• Meteors• Sporadic E• Satellites

Page 10: Propagation of radio waves

Aurora

• High-energy particles flow into ionosphere during geomagnetic storm ionize E layer

• 28 – 432 MHz• K index: magnetic activity 0-9• Signals sound distorted, sometimes only

CW at VHF-UHF (A=Aurora)

Page 11: Propagation of radio waves

EME

• Earth-Moon-Earth• 50 MHz to 10 GHz• Free space loss, ½ degree target, Doppler

shift, Faraday rotation... not that easy• eFFe-mobiili

Page 12: Propagation of radio waves

Meteor scatter

• Ionize a column of air at E layer– stays ionized for a few seconds to a minute

just enough time for brief contacs• 50 MHz, 144 MHz• High speed Morse code, pieced together

Page 13: Propagation of radio waves

Sporadic E

• Ionization level gets abnormally high• 28, 50, 144 MHz• Usually at summer time at morning and

again at early evening• Might dissipate quickly or move

Page 14: Propagation of radio waves

Satellites

• Works as repeater station