General exam G3: Radio Wave Propagation
All 37 questions in subelement G3. The exam asks 3 of them, one from each group (G3A, G3B, G3C). Answers are hidden until you open them.
G3A
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G3A01 How does a higher sunspot number affect HF propagation?
- Higher sunspot numbers generally indicate a greater probability of good propagation at higher frequencies
- Lower sunspot numbers generally indicate greater probability of sporadic E propagation
- A zero sunspot number indicates that radio propagation is not possible on any band
- A zero sunspot number indicates undisturbed conditions
Show answer
A. Higher sunspot numbers generally indicate a greater probability of good propagation at higher frequencies
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G3A02 What effect does a sudden ionospheric disturbance have on the daytime ionospheric propagation?
- It enhances propagation on all HF frequencies
- It disrupts signals on lower frequencies more than those on higher frequencies
- It disrupts communications via satellite more than direct communications
- None, because only areas on the night side of the Earth are affected
Show answer
B. It disrupts signals on lower frequencies more than those on higher frequencies
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G3A03 Approximately how long does it take the increased ultraviolet and X-ray radiation from a solar flare to affect radio propagation on Earth?
- 28 days
- 1 to 2 hours
- 8 minutes
- 20 to 40 hours
Show answer
C. 8 minutes
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G3A04 Which of the following are the least reliable bands for long-distance communications during periods of low solar activity?
- 80 meters and 160 meters
- 60 meters and 40 meters
- 30 meters and 20 meters
- 15 meters, 12 meters, and 10 meters
Show answer
D. 15 meters, 12 meters, and 10 meters
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G3A05 What is the solar flux index?
- A measure of the highest frequency that is useful for ionospheric propagation between two points on Earth
- A count of sunspots that is adjusted for solar emissions
- Another name for the American sunspot number
- A measure of solar radiation with a wavelength of 10.7 centimeters
Show answer
D. A measure of solar radiation with a wavelength of 10.7 centimeters
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G3A06 What is a geomagnetic storm?
- A sudden drop in the solar flux index
- A thunderstorm that affects radio propagation
- Ripples in the geomagnetic force
- A temporary disturbance in Earth’s geomagnetic field
Show answer
D. A temporary disturbance in Earth’s geomagnetic field
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G3A07 At what point in the solar cycle does the 20-meter band usually support worldwide propagation during daylight hours?
- At the summer solstice
- Only at the maximum point
- Only at the minimum point
- At any point
Show answer
D. At any point
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G3A08 How can a geomagnetic storm affect HF propagation?
- Improve high-latitude HF propagation
- Degrade ground wave propagation
- Improve ground wave propagation
- Degrade high-latitude HF propagation
Show answer
D. Degrade high-latitude HF propagation
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G3A09 How can high geomagnetic activity benefit radio communications?
- Creates auroras that can reflect VHF signals
- Increases signal strength for HF signals passing through the polar regions
- Improve HF long path propagation
- Reduce long delayed echoes
Show answer
A. Creates auroras that can reflect VHF signals
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G3A10 What causes HF propagation conditions to vary periodically in a 26- to 28-day cycle?
- Long term oscillations in the upper atmosphere
- Cyclic variation in Earth’s radiation belts
- Rotation of the Sun’s surface layers around its axis
- The position of the Moon in its orbit
Show answer
C. Rotation of the Sun’s surface layers around its axis
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G3A11 How long does it take a coronal mass ejection to affect radio propagation on Earth?
- 28 days
- 14 days
- 4 to 8 minutes
- 15 hours to several days
Show answer
D. 15 hours to several days
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G3A12 What does the K-index measure?
- The relative position of sunspots on the surface of the Sun
- The short-term stability of Earth’s geomagnetic field
- The short-term stability of the Sun’s magnetic field
- The solar radio flux at Boulder, Colorado
Show answer
B. The short-term stability of Earth’s geomagnetic field
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G3A13 What does the A-index measure?
- The relative position of sunspots on the surface of the Sun
- The amount of polarization of the Sun’s electric field
- The long-term stability of Earth’s geomagnetic field
- The solar radio flux at Boulder, Colorado
Show answer
C. The long-term stability of Earth’s geomagnetic field
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G3A14 How is long distance radio communication usually affected by the charged particles that reach Earth from solar coronal holes?
- HF communication is improved
- HF communication is disturbed
- VHF/UHF ducting is improved
- VHF/UHF ducting is disturbed
Show answer
B. HF communication is disturbed
G3B
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G3B01 What is a characteristic of skywave signals arriving at your location by both short-path and long-path propagation?
- Periodic fading approximately every 10 seconds
- Signal strength increased by 3 dB
- The signal might be cancelled causing severe attenuation
- A slightly delayed echo might be heard
Show answer
D. A slightly delayed echo might be heard
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G3B02 What factors affect the MUF?
- Path distance and location
- Time of day and season
- Solar radiation and ionospheric disturbances
- All these choices are correct
Show answer
D. All these choices are correct
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G3B03 Which frequency will have the least attenuation for long-distance skip propagation?
- Just below the MUF
- Just above the LUF
- Just below the critical frequency
- Just above the critical frequency
Show answer
A. Just below the MUF
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G3B04 Which of the following is a way to determine current propagation on a desired band from your station?
- Use a network of automated receiving stations on the internet to see where your transmissions are being received
- Check the A-index
- Send a series of dots and listen for echoes
- All these choices are correct
Show answer
A. Use a network of automated receiving stations on the internet to see where your transmissions are being received
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G3B05 How does the ionosphere affect radio waves with frequencies below the MUF and above the LUF?
- They are refracted back to Earth
- They pass through the ionosphere
- They are amplified by interaction with the ionosphere
- They are refracted and trapped in the ionosphere to circle Earth
Show answer
A. They are refracted back to Earth
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G3B06 What usually happens to radio waves with frequencies below the LUF?
- They are refracted back to Earth
- They pass through the ionosphere
- They are attenuated before reaching the destination
- They are refracted and trapped in the ionosphere to circle Earth
Show answer
C. They are attenuated before reaching the destination
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G3B07 What does LUF stand for?
- The Lowest Usable Frequency for communications between two specific points
- The Lowest Usable Frequency for communications to any point outside a 100-mile radius
- The Lowest Usable Frequency during a 24-hour period
- The Lowest Usable Frequency during the past 60 minutes
Show answer
A. The Lowest Usable Frequency for communications between two specific points
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G3B08 What does MUF stand for?
- The Minimum Usable Frequency for communications between two points
- The Maximum Usable Frequency for communications between two points
- The Minimum Usable Frequency during a 24-hour period
- The Maximum Usable Frequency during a 24-hour period
Show answer
B. The Maximum Usable Frequency for communications between two points
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G3B09 What is the approximate maximum distance along the Earth’s surface normally covered in one hop using the F2 region?
- 180 miles
- 1,200 miles
- 2,500 miles
- 12,000 miles
Show answer
C. 2,500 miles
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G3B10 What is the approximate maximum distance along the Earth’s surface normally covered in one hop using the E region?
- 180 miles
- 1,200 miles
- 2,500 miles
- 12,000 miles
Show answer
B. 1,200 miles
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G3B11 What happens to HF propagation when the LUF exceeds the MUF?
- Propagation via ordinary skywave communications is not possible over that path
- HF communications over the path are enhanced
- Double-hop propagation along the path is more common
- Propagation over the path on all HF frequencies is enhanced
Show answer
A. Propagation via ordinary skywave communications is not possible over that path
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G3B12 Which of the following is typical of the lower HF frequencies during the summer?
- Poor propagation at any time of day
- World-wide propagation during daylight hours
- Heavy distortion on signals due to photon absorption
- High levels of atmospheric noise or static
Show answer
D. High levels of atmospheric noise or static
G3C
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G3C01 Which ionospheric region is closest to the surface of Earth?
- The D region
- The E region
- The F1 region
- The F2 region
Show answer
A. The D region
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G3C02 What is meant by the term “critical frequency” at a given incidence angle?
- The highest frequency which is refracted back to Earth
- The lowest frequency which is refracted back to Earth
- The frequency at which the signal-to-noise ratio approaches unity
- The frequency at which the signal-to-noise ratio is 6 dB
Show answer
A. The highest frequency which is refracted back to Earth
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G3C03 Why is skip propagation via the F2 region longer than that via the other ionospheric regions?
- Because it is the densest
- Because of the Doppler effect
- Because it is the highest
- Because of temperature inversions
Show answer
C. Because it is the highest
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G3C04 What does the term “critical angle” mean, as applied to radio wave propagation?
- The long path azimuth of a distant station
- The short path azimuth of a distant station
- The lowest takeoff angle that will return a radio wave to Earth under specific ionospheric conditions
- The highest takeoff angle that will return a radio wave to Earth under specific ionospheric conditions
Show answer
D. The highest takeoff angle that will return a radio wave to Earth under specific ionospheric conditions
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G3C05 Why is long-distance communication on the 40-, 60-, 80-, and 160-meter bands more difficult during the day?
- The F region absorbs signals at these frequencies during daylight hours
- The F region is unstable during daylight hours
- The D region absorbs signals at these frequencies during daylight hours
- The E region is unstable during daylight hours
Show answer
C. The D region absorbs signals at these frequencies during daylight hours
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G3C06 What is a characteristic of HF scatter?
- Phone signals have high intelligibility
- Signals have a fluttering sound
- There are very large, sudden swings in signal strength
- Scatter propagation occurs only at night
Show answer
B. Signals have a fluttering sound
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G3C07 What makes HF scatter signals often sound distorted?
- The ionospheric region involved is unstable
- Ground waves are absorbing much of the signal
- The E region is not present
- Energy is scattered into the skip zone through several different paths
Show answer
D. Energy is scattered into the skip zone through several different paths
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G3C08 Why are HF scatter signals in the skip zone usually weak?
- Only a small part of the signal energy is scattered into the skip zone
- Signals are scattered from the magnetosphere, which is not a good reflector
- Propagation is via ground waves, which absorb most of the signal energy
- Propagation is via ducts in the F region, which absorb most of the energy
Show answer
A. Only a small part of the signal energy is scattered into the skip zone
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G3C09 What type of propagation allows signals to be heard in the transmitting station’s skip zone?
- Faraday rotation
- Scatter
- Chordal hop
- Short-path
Show answer
B. Scatter
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G3C10 What is near vertical incidence skywave (NVIS) propagation?
- Propagation near the MUF
- Short distance MF or HF propagation at high elevation angles
- Long path HF propagation at sunrise and sunset
- Double hop propagation near the LUF
Show answer
B. Short distance MF or HF propagation at high elevation angles
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G3C11 Which ionospheric region is the most absorbent of signals below 10 MHz during daylight hours?
- The F2 region
- The F1 region
- The E region
- The D region
Show answer
D. The D region