TAS 1 - radiowave propagation

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Last updated 1:22 PM on 1/8/26
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127 Terms

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4 elements of communication

transmitter

receiver

channel

message

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Why is distance near the skip distance should be used for sky-wave propagation?

To prevent sky wave and upper ray interference

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Window

A range of microwave frequency more easily passed by the atmosphere than the other

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Radio wave Propagation

behavior of radio waves as they travel from one point to another

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Wave Propagation

transfer of electromagnetic waves from one point to another

can be perpendicular, right, normal, or 90 degrees

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Electromagnetic Waves (EM waves)

Also called radio waves

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2 types of waves (wrt DIRECTION)

transverse and longitudinal

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transverse waves

PERPENDICULAR (light, em waves) propagation to its direction

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longitudinal waves

PARALLEL (sound waves) propagation to its direction

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elements of a wave

peak-to-peak

crest (+ peak)

trough (- peak)

wavelength

alternation (at x axis)

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frequency

#of cycles per second of a wave

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wavelength

distance that wave travels in time of 1 cycle

λ = c / f

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wave velocity

speed of wave depends on the type and nature of propagation of the medium

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Electromagnetic Spectrum

the complete range of electromagnetic radiation, arranged by wavelength or frequency, from radio waves to gamma rays

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isotropic antenna

can radiate uniformly in all direction

ideal antenna/radiator/reference (hypothetical)

gain = 1 (0db)

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wave impedance

also called characteristic impedance for w/c medium is air

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wavelength

λ = c / f

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power density

ratio of tx power over area w/c it is distributed

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field intensity/field strength

quality of electric field at any given point (volt/m)

potential of 1 volt induced in a 1m antenna wire

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E and H fields

perpendicular to each other and direction

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poynting vector

quantifies energy flow of EM wave

energy per unit area, per unit time

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how does electric field intensity (E) affects the power density (Pd) when it is doubled?

the power density will quadruple

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polarization

orientation of E-field wrt Earth’s surface

linear, circular, elliptic, random

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linear polarization

defined by direction of the electric field vector

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circular polarization

electric vector rotates in horizontal + vertical (equal in magnitude)

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elliptical polarization

electric vector rotates about the axis of direction, but amplitude of its 2 linearly polarized components is not equal

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random polarization

stochastic

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random polarization

no fixed pattern of polarization variation

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attenuation

attenuates the EM waves as it travels outward from its source

proportional to the square of distance travelled

dB

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reflection

bouncing of waves as it strikes conductive surface

180 degrees phase shift

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refraction

bending of waves as it passes boundary of 2 media having diff density

HLA LHT

uses Snell’s law and refractive index

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diffraction

ability of an EM wave to pass through obstacles

bends around obstacle

low freq - bass

high freq - mid treble

low freq diffract more than high freq

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scattering

diffusion of signal when it encounters an uneven surface of the object

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absorption

signal is absorbed & converted to heat

source of energy of waves is transferred to atoms and molecules of space

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interference

occurs when 2 waves combine which results to degraded performance

(collision of waves)

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absorption loss increases with freq due to

molecular resonance

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Rayleigh fading assumes

multipath interference, no LOS

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Rayleigh fading

statistical model for wireless comms

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phase shift upon reflection from denser medium is

180 deg

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at grazing incidence on sea water, vertical polarization reflection coefficient approaches

-1

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increases the attenuation of a radio signal

high freq of signal

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critical angle occurs when refracted ray is

90 deg

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surface wave

travels around curvature of earth, sometimes right around the globe

soil conductivity

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surface wave

vertical polarization to reduce attenuation

freq below HF

loss with increase freq

high freq short wavelength

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AM

535-1605 kHz

(Marconi Antenna)

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surface wave

VLF

3-30 kHz

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sky wave

HF

3-30 MHz

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space wave

SHF

3-30 GHz

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space wave

SHF

microwave

GHz

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space wave

LOS & P2P

travels in troposphere (atm portion closest to the ground)

caused by varying density of atm due to diffraction around curvature of earth

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sky wave

HF

3-30 MHz

FM/TV

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sky wave

strikes at the ionosphere and refracted back to the ground

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Increasing Ionization

Bends waves toward Earth.

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Decreasing Ionization

Bends waves away from Earth.

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Highly Dense Center

Refraction happens slowly.

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Refraction Process

Change in velocity causing a change in direction.

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Lower Frequency

Refracts faster; covers shorter distances.

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Higher Frequency

Refracts slower; covers longer distances.

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100 MHz (VHF/UHF)

Passes straight through (too fast to bend).

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Lower Radiation Angle

Creates a longer skip distance.

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Higher Radiation Angle

Creates a shorter skip distance.

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Skip Distance

The distance between the transmitter and the point where the sky wave first returns.

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High Frequency + Low Angle

Maximum Distance

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Low Frequency + High Angle

Minimum Distance

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Skip Zone

A location (the empty "hole" on the map where you can't hear anything)

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D-Layer

lowest, h=70km, thickness=10km

least important

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D-Layer

ability to refract signals of low freq

high freq pass thru and attenuated

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E-Layer

h=100km, thickness=25km

also known as KENELLY-HEAVISIDE LAYER

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E-Layer

ability to refract signals as high as 20MHz

used for comm ranges up to 1500 miles

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Es-Layer Sporadic

very high ionization density

occurs during the night

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F2-Layer

most important for HF radiowaves

height=250km to 400km (daytime)

thickness=200km

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F2-Layer

at night, height=300km and combines with F1 layer

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F1-Layer

height=180km, thickness=20km (daytime)

combines with F2 layer at night

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F1-Layer

more absorption for HF waves

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ground waves are attenuated by:

ground conductivity

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primary freq range for reliable ground wave

MF (300kHz-3MHz)

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surface wave component of ground wave uses

earth’s curvature as waveguide

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UHF frequencies primarily use:

space waves

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when LOS antennas see each other, mode is

space/direct wave

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sky wave is reliable during

nighttime (f-layer)

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tropospheric ducting

rise in temp in the atm, instead of normal decrease (known as tem inversion) the higher refractive index of the atm there will cause the signal to be bent

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tropospheric scattering

when a radio wave passing through the trophosphere meets a turbulence, it makes an abrupt change in velocity

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virtual height

height of projected path of sky waves

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virtual height

measured by sending a wave vertical to the layer and measuring the time it takes to come back to the receiver

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critical frequency

highest freq that will be returned down to earth by certain layer after having been beamed vertically upward

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maximum usable frequency (MUF)

highest freq that will be returned down to earth at given distance when beamed at a specific angle other than the normal

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optimum working frequency (OWF)

freq chosen by practical to avoid irregularities of ionosphere

15% lower than MUF

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frequency of optimum transmission (FOT)

other term for optimum working frequency (OWF)

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optimum usable frequency

other term for optimum working frequency (OWF)

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interference fading

mixing two or more signal components propagating along diff paths

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absorption fading

caused by solar flare activities and particularly affects the lower freqs

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polarization fading

caused by the so-called Faraday Effect or Faraday Rotation

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selective fading

fading having diff effects on diff freq ranges

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11-year sunspot cycle

sun’s magnetic field doesn’t flip

north pole becomes the south pole, and vice versa

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27-day sunspot cycle

visible at 27 day intervals, approx period req for the sun to make one complete rotation

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maximum usable frequency (MUF) defined as

highest frequency for given path

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skip distance increases with

high frequency and lower take-off angle

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why is the MUF generally higher during the day than at night?

ionization density in the f2-layer is higher during the day due to solar radiation

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f2 layer provides longest

skip distances (300-4000 km)

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tropospheric ducting occurs when:

warm air traps signals above cool layer (VHF/UHF)

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