Chelmsford Amateur Radio Society Advanced Course (6) Propagation Part-1: Electromagnetic Waves - PowerPoint PPT Presentation

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Chelmsford Amateur Radio Society Advanced Course (6) Propagation Part-1: Electromagnetic Waves

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Title: Propagation Part-1 - EM Waves Subject: Advanced Course Author: Christopher Chapman G0IPU Description: EM Graphic By M Niman G6JYB Others by Andrew Chapman G7TKK – PowerPoint PPT presentation

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Title: Chelmsford Amateur Radio Society Advanced Course (6) Propagation Part-1: Electromagnetic Waves


1
Chelmsford Amateur Radio Society Advanced
Course(6) Propagation Part-1 Electromagnetic
Waves
2
Electromagnetic Waves
  • Electromagnetic radiation comprises both an
    Electric and a Magnetic Field
  • The two fields are at right-angles to each other,
    and the direction of propagation is at
    right-angles to both fields
  • The Plane of the Electric Field defines the
    Polarisation of the wave
  • The relationship between the magnitudes of the E
    and H fields is constant

3
EM Wave Fronts head-on
Electric Field (E)
Magnetic Field (H)
4
EM Wave Fronts head-on
Electric Field (E)
Magnetic Field (H)
5
Electromagnetic Radiation
  • In free space conditions Electro-Magnetic (EM)
    waves travelin straight lines and spread out
  • Both Power Flux Density (PFD) in W/m2 and Field
    Strength in V/m, drop with distance
  • Double the distance from an antenna and you
    willhalve the field strength, but also quarter
    the Power Flux Density (PFD), according to an
    inverse square law

6
EM Field vs Distance
Rx
Tx
7
Inverse Square Law forDistance and Intensity
  • Relationship between distance and intensity of
    electromagnetic radiation (rf or light)
  • Inverse square gives a 1/d2 reduction
  • Example
  • D 1m - Intensity 1
  • D 2m - Intensity ¼
  • Doubling the distance spreads same amount of
    energy over four times the area

8
Another PFD Example
9
Velocity Of Propagation
  • Propagation velocity depends on the medium in
    which EM waves travel
  • Free Space ? Maximum velocity
  • Air ? slightly less than free space and dependent
    on water vapour
  • Coax ? 0.66 Times that of Free Space
  • Water ? far less, and lossy
  • v f . ?
  • v is the speed of radio waves light - v
    300,000,000 m/s
  • f is the frequency in Hz.
  • ? is the wavelength in metres
  • For l /4 for 2m
  • 300 /145.5 x 0.66 / 4 Coax length 340.2mm

10
Linear Polarisation
  • Transmit and receive antennas should have the
    same polarisation
  • To be efficient...
  • Otherwise, signal strength may be reduced by up
    to 32dB
  • Polarisation losses can be up to 5 S-points
  • Note that after travelling through the
    ionosphere, the polarisation may have changed
    significantly

11
Circular Polarisation
  • The E-field of the wave rotates as it propagates,
    with either
  • Left-handed polarisation (LHCP) (anticlockwise
    from behind) as shown, or
  • Right-Handed polarisation (RHCP) (clockwise from
    behind)

Electric Field, E
Magnetic Field, H
Direction of Propagation
  • Used for satellite comms where the orientation
    of the EM field from the satellite is
    indeterminate
  • Make sure you receive correct circular
    orientation or high polarisation losses will
    result

12
Helical Antennas for Circular Polarisation
  • 2.4 GHz Helical Antenna
  • Designed for OSCAR 40
  • Omni-directional Quadrifilar Helical RHCP
    antenna
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