Initial commit
This commit is contained in:
78
pages/T3C.md
Normal file
78
pages/T3C.md
Normal file
@ -0,0 +1,78 @@
|
||||
T3C - Propagation modes: sporadic E, meteor scatter, auroral propagation, tropospheric ducting; F region skip; Line of sight and radio horizon
|
||||
|
||||
- [[T3C01]] (C)
|
||||
Why are simplex UHF signals rarely heard beyond their radio horizon? #card
|
||||
- A. They are too weak to go very far
|
||||
- B. FCC regulations prohibit them from going more than 50 miles
|
||||
- C. UHF signals are usually not propagated by the ionosphere
|
||||
- D. UHF signals are absorbed by the ionospheric D region
|
||||
|
||||
- [[T3C02]] (C)
|
||||
What is a characteristic of HF communication compared with communications on VHF and higher frequencies? #card
|
||||
- A. HF antennas are generally smaller
|
||||
- B. HF accommodates wider bandwidth signals
|
||||
- C. Long-distance ionospheric propagation is far more common on HF
|
||||
- D. There is less atmospheric interference (static) on HF
|
||||
|
||||
- [[T3C03]] (B)
|
||||
What is a characteristic of VHF signals received via auroral backscatter? #card
|
||||
- A. They are often received from 10,000 miles or more
|
||||
- B. They are distorted and signal strength varies considerably
|
||||
- C. They occur only during winter nighttime hours
|
||||
- D. They are generally strongest when your antenna is aimed west
|
||||
|
||||
- [[T3C04]] (B)
|
||||
Which of the following types of propagation is most commonly associated with occasional strong signals on the 10, 6, and 2 meter bands from beyond the radio horizon? #card
|
||||
- A. Backscatter
|
||||
- B. Sporadic E
|
||||
- C. D region absorption
|
||||
- D. Gray-line propagation
|
||||
|
||||
- [[T3C05]] (A)
|
||||
Which of the following effects may allow radio signals to travel beyond obstructions between the transmitting and receiving stations? #card
|
||||
- A. Knife-edge diffraction
|
||||
- B. Faraday rotation
|
||||
- C. Quantum tunneling
|
||||
- D. Doppler shift
|
||||
|
||||
- [[T3C06]] (A)
|
||||
What type of propagation is responsible for allowing over-the-horizon VHF and UHF communications to ranges of approximately 300 miles on a regular basis? #card
|
||||
- A. Tropospheric ducting
|
||||
- B. D region refraction
|
||||
- C. F2 region refraction
|
||||
- D. Faraday rotation
|
||||
|
||||
- [[T3C07]] (B)
|
||||
What band is best suited for communicating via meteor scatter? #card
|
||||
- A. 33 centimeters
|
||||
- B. 6 meters
|
||||
- C. 2 meters
|
||||
- D. 70 centimeters
|
||||
|
||||
- [[T3C08]] (D)
|
||||
What causes tropospheric ducting? #card
|
||||
- A. Discharges of lightning during electrical storms
|
||||
- B. Sunspots and solar flares
|
||||
- C. Updrafts from hurricanes and tornadoes
|
||||
- D. Temperature inversions in the atmosphere
|
||||
|
||||
- [[T3C09]] (A)
|
||||
What is generally the best time for long-distance 10 meter band propagation via the F region? #card
|
||||
- A. From dawn to shortly after sunset during periods of high sunspot activity
|
||||
- B. From shortly after sunset to dawn during periods of high sunspot activity
|
||||
- C. From dawn to shortly after sunset during periods of low sunspot activity
|
||||
- D. From shortly after sunset to dawn during periods of low sunspot activity
|
||||
|
||||
- [[T3C10]] (A)
|
||||
Which of the following bands may provide long-distance communications via the ionosphere’s F region during the peak of the sunspot cycle? #card
|
||||
- A. 6 and 10 meters
|
||||
- B. 23 centimeters
|
||||
- C. 70 centimeters and 1.25 meters
|
||||
- D. All these choices are correct
|
||||
|
||||
- [[T3C11]] (C)
|
||||
Why is the radio horizon for VHF and UHF signals more distant than the visual horizon? #card
|
||||
- A. Radio signals move somewhat faster than the speed of light
|
||||
- B. Radio waves are not blocked by dust particles
|
||||
- C. The atmosphere refracts radio waves slightly
|
||||
- D. Radio waves are blocked by dust particles
|
Reference in New Issue
Block a user