terrestrial propagation
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Terrestrial Propagation
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Terrestrial Waves- electromagnetic waves
traveling within Earths
atmosphere.
Terrestrial Radio
Communication
- communication between two ormore points on Earth.
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General Classifcation oRadio waves
Ground
Waves
Space
Waves
Sky
Waves
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AtmosphericLayer
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Ground Waves/ SurfaceWaves Propagation
Travel around the curvature of the earth, sometimes right around the
globe
tili!es fre"uencies belo# $% range
Propagates best over a good conductor &sea#ater' and highest
attenuation is over (ungle areas)
Progress along the surface of the earth and must be vertically polari!ed
to prevent short circuiting the electric component)
Wave induces current to the ground* some of its energy is lost due to
absorption)
With enough po#er transmitted, #ave front could propagate around the
+arth
Travel around the curvature of the earth, sometimes right around the
globe
tili!es fre"uencies belo# $% range
Propagates best over a good conductor &sea#ater' and highest
attenuation is over (ungle areas)
Progress along the surface of the earth and must be vertically polari!ed
to prevent short circuiting the electric component)
Wave induces current to the ground* some of its energy is lost due to
absorption)
With enough po#er transmitted, #ave front could propagate around the
+arth
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Ground Waves/ SurfaceWaves Propagation
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Space Waves/Tropospheric Propagation
Travel in the troposphere* the portion of the atmosphere closest to
the ground)
tili!es fre"uencies above $% range
nclude both direct and ground-reflected #aves.
irect #aves / Line of Sight 0 travels in straight line bet#een
the transmit and receive antenna
- limited by the curvature of +arth
Ground-reflected #aves - reflected by earth1s surface as they
propagate bet#een transmit and receive antenna
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Space Waves/Tropospheric Propagation
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Sky Waves/ onosphericPropagation
The #ave strikes the ionosphere and is refracted back to the
ground)
tili!es fre"uencies in the $% range and sometimes fre"uencies
(ust above or belo# it)
onosphere is a region in the earth1s atmosphere #here the air
pressure is so lo# that the free electrons and ions can move
about for some time #ithout getting close enough to recombine
into neutral atoms) t absorbs large "ualities of radiant energy
from the sun, becoming heated and ioni!ed) oni!ation is the
result of the bombardment of the sun1s rays by a variety of #ave
from heat and light to cosmic rays) 2ost important ioni!ing agents
are ultraviolet, alpha, beta and gamma rays coming from the sun,
cosmic rays and meteors)
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onospheric
Layers
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Sky Waves/ onosphericPropagation
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-Layer
The lo#est, e3isting at an average height
of 45 km, #ith an average thickness of 65
kmLeast important layer in $% propagation7eflects some 8L% and L% #aves and
absorbs 2% and $% #aves to a certain
e3tent
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+-Layer
+3isting at about 655km in height, #ith
thickness of 9:km
isappears at night)Aid 2% surface propagation a little and
reflects some $% #aves in daytimeThis layer is also kno#n as KENELLY-
HEAVISIDE LAYER
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+s Layer/
SporadicThin layer of very high ioni!ation density,
sometimes making an appearance #ith the
+ layer)When it occurs, it often persists during the
night)
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%-Layer
+3istataheightof6;5kmindaytimeand combines#iththe%9layeratnight)ts
daytimethicknessisabout95km2ain+ffectistoprovidemoreabsorption
for$%#aves
!
la"er
Themostimportantreflectingmediumfor$%radio#aves)
Appro3imatethicknessis955kmanditsheightrangesfrom9:5to