Propagation Modes & Atmospheric Interactions

0.0(0)
studied byStudied by 0 people
0.0(0)
full-widthCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/49

flashcard set

Earn XP

Description and Tags

Comms 4 Modes of Propagation

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

50 Terms

1
New cards

Terrestrial Propagation

Propagation of radio waves within the Earth's atmosphere between two or more points on the Earth's surface.

2
New cards

Modes of Wave Propagation

  1. Ground/Surface Wave, 2. Sky/Ionospheric Wave, 3. Space/LOS/Tropospheric Wave.

3
New cards

ELF (Extremely Low Frequency)

3-30 Hz.

4
New cards

SLF (Super Low Frequency)

30-300 Hz.

5
New cards

ULF (Ultra Low Frequency)

300-3000 Hz.

6
New cards

VLF (Very Low Frequency)

3-30 kHz; uses Ground Wave propagation.

7
New cards

LF (Low Frequency)

30-300 kHz; uses Ground Wave propagation.

8
New cards

MF (Medium Frequency)

300-3000 kHz; uses Ground Wave propagation; used for AM Broadcasting.

9
New cards

HF (High Frequency)

3-30 MHz; uses Sky Wave propagation.

10
New cards

VHF (Very High Frequency)

30-300 MHz; uses Space Wave propagation.

11
New cards

UHF (Ultra High Frequency)

300-3000 MHz; uses Space Wave propagation.

12
New cards

SHF (Super High Frequency)

3-30 GHz.

13
New cards

EHF (Extremely High Frequency)

30-300 GHz.

14
New cards

Ground Wave Propagation

An Earth-guided electromagnetic wave that travels over the surface of the Earth, following its contour due to diffraction.

15
New cards

Ground Wave Frequency Range

Effective on VLF, LF, and MF bands (frequencies up to 2 MHz).

16
New cards

Ground Wave Polarization

Must be vertically polarized to prevent short-circuiting the electric field component by the ground.

17
New cards

Surface Conductivity for Ground Waves

Sea water is 'Good'; Flat, loamy soil is 'Fair'; Jungle is 'Unusable'.

18
New cards

Ground Wave Application

Primarily used for AM radio broadcasting.

19
New cards

Ground Wave Disadvantages

Requires relatively high transmission power, large antennas, and ground losses vary with surface materials.

20
New cards

Ground Wave Field Strength Formula

E = (120 * pi * I * ht) / (lambda * d).

21
New cards

Induced Antenna Voltage Formula

Va = E * hr (Electric field * height of receive antenna).

22
New cards

Sky Wave Propagation (Ionospheric Propagation)

Radio waves strike the ionosphere and are refracted back to the ground; used primarily in the HF band.

23
New cards

Cause of Ionization

Ultraviolet radiation from the sun is the primary cause of ionization in the atmosphere.

24
New cards

Troposphere

The lowest layer of the atmosphere (8-10 miles high) where weather disturbances take place.

25
New cards

Stratosphere

The isothermal region of the atmosphere located above the troposphere with constant temperature.

26
New cards

Ionosphere

The region of the atmosphere containing ionized layers and low-density gas.

27
New cards

D Layer

The lowest ionospheric layer (30-55 miles); exists only during the day; absorbs MF and attenuates HF.

28
New cards

E Layer (Kennelly-Heaviside Layer)

Exists 55-90 miles high; refracts HF waves during the day; disappears by midnight; can refract signals up to 20 MHz.

29
New cards

F Layer

Exists 90-240 miles high; splits into F1 and F2 during the day; responsible for HF long-distance transmission.

30
New cards

Daily Variations

Variations in the ionosphere resulting from the 24-hour rotation of the Earth.

31
New cards

Seasonal Variations

Variations resulting from the Earth revolving around the sun and the relative position of the sun.

32
New cards

11-Year Sunspot Cycle

A cycle of minimum and maximum sunspot activity affecting ionization levels every 11 years.

33
New cards

27-Day Sunspot Cycle

Variations caused by the rotation of the sun on its own axis, making sunspots visible at 27-day intervals.

34
New cards

Sporadic E

Irregular cloud-like patches of unusually high ionization forming near the normal E layer.

35
New cards

Sudden Ionospheric Disturbances (SID)

Disturbances caused by gigantic emissions of hydrogen (solar flares) from the sun; can last minutes to hours.

36
New cards

Ionospheric Storms

Disturbances caused by particle radiation from the sun, which moves slower than UV light.

37
New cards

Index of Refraction in Ionosphere (n)

Formula: n = square root of (1 - (81 * N) / f^2); where N is electron density.

38
New cards

Critical Frequency (fc)

The highest frequency that will be returned to earth when beamed vertically upward.

39
New cards

Critical Frequency Formula

fc = square root of (81 * Nmax).

40
New cards

Maximum Usable Frequency (MUF)

The highest frequency returned to earth at a given distance when beamed at a specific angle (Secant Law).

41
New cards

MUF Formula

MUF = fc / cos(theta) = fc * sec(theta).

42
New cards

Optimum Working Frequency (OWF/FOT)

The frequency that gives the most consistent communication; chosen to be 15% lower than MUF.

43
New cards

OWF Formula

OWF = 0.85 * MUF.

44
New cards

Virtual Height

The apparent height of the ionized layer measured by sending a wave vertically and timing its return.

45
New cards

Skip Zone

The zone of silence between the point where the ground wave becomes too weak and the point where the sky wave first returns.

46
New cards

Skip Distance

The distance from the transmitter to the point where the sky wave is first returned to Earth.

47
New cards

Space Wave Propagation (LOS)

Line-of-Sight or Tropospheric propagation; composed of a direct wave and a reflected wave.

48
New cards

Radio Horizon

The boundary beyond which direct rays cannot be propagated; it is approximately 4/3 times the optical horizon.

49
New cards

Radio Horizon Formula (Metric)

D(km) = sqrt(17 * htmeters) + sqrt(17 * hrmeters).

50
New cards

Radio Horizon Formula (English)

D(miles) = sqrt(2 * htfeet) + sqrt(2 * hrfeet).