E3 - RADIO WAVE PROPAGATION [3 Exam Questions - 3 Groups] 40 Questions Flashcards
(39 cards)
“What is the approximate maximum separation measured along the surface of the Earth between two stations communicating by EME?”
A. 500 miles, if the moon is at perigee
B. 2000 miles, if the moon is at apogee
C. 5000 miles, if the moon is at perigee
D. 12,000 miles, if the moon is visible by both stations
D. 12,000 miles, if the moon is visible by both stations
“What characterizes libration fading of an EME signal?”
A. A slow change in the pitch of the CW signal
B. A fluttery irregular fading
C. A gradual loss of signal as the sun rises
D. The returning echo is several hertz lower in frequency than the transmitted signal
B. A fluttery irregular fading
“When scheduling EME contacts, which of these conditions will generally result in the least path loss?”
A. When the moon is at perigee
B. When the moon is full
C. When the moon is at apogee
D. When the MUF is above 30 MHz
A. When the moon is at perigee
“What do Hepburn maps predict?”
A. Sporadic E propagation
B. Locations of auroral reflecting zones
C. Likelihood of rain scatter along cold or warm fronts
D. Probability of tropospheric propagation
D. Probability of tropospheric propagation
“Tropospheric propagation of microwave signals often occurs in association with what phenomenon?”
A. Grayline
B. Lightning discharges
C. Warm and cold fronts
D. Sprites and jets
C. Warm and cold fronts
“What might help to restore contact when DX signals become too weak to copy across an entire HF band a few hours after sunset?”
A. Switch to a higher frequency HF band
B. Switch to a lower frequency HF band
C. Wait 90 minutes or so for the signal degradation to pass
D. Wait 24 hours before attempting another communication on the band
B. Switch to a lower frequency HF band
“Atmospheric ducts capable of propagating microwave signals often form over what geographic feature?”
A. Mountain ranges
B. Forests
C. Bodies of water
D. Urban areas
C. Bodies of water
“When a meteor strikes the Earth’s atmosphere, a cylindrical region of free electrons is formed at what layer of the ionosphere?”
A. The E layer
B. The F1 layer
C. The F2 layer
D. The D layer
A. The E layer
“Which of the following frequency ranges is most suited for meteor scatter communications?”
A. 1.8 MHz - 1.9 MHz
B. 10 MHz - 14 MHz
C. 28 MHz - 148 MHz
D. 220 MHz - 450 MHz
C. 28 MHz - 148 MHz
“Which type of atmospheric structure can create a path for microwave propagation?”
A. The jet stream
B. Temperature inversion
C. Wind shear
D. Dust devil
B. Temperature inversion
“What is a typical range for tropospheric propagation of microwave signals?”
A. 10 miles to 50 miles
B. 100 miles to 300 miles
C. 1200 miles
D. 2500 miles
B. 100 miles to 300 miles
“What is the cause of auroral activity?”
A. The interaction in the F2 layer between the solar wind and the Van Allen belt
B. An extreme low-pressure area in the polar regions
C. The interaction in the E layer of charged particles from the Sun with the Earth’s magnetic field
D. Meteor showers concentrated in the extreme northern and southern latitudes
C. The interaction in the E layer of charged particles from the Sun with the Earth’s magnetic field
“Which of these emission modes is best for auroral propagation?”
A. CW
B. SSB
C. FM
D. RTTY
A. CW
“What is meant by circularly polarized electromagnetic waves?”
A. Waves with an electric field bent into a circular shape
B. Waves with a rotating electric field
C. Waves that circle the Earth
D. Waves produced by a loop antenna
B. Waves with a rotating electric field
“What is transequatorial propagation?”
A. Propagation between two mid-latitude points at approximately the same distance north and south of the magnetic equator
B. Propagation between points located on the magnetic equator
C. Propagation between a point on the equator and its antipodal point
D. Propagation between points at the same latitude
A. Propagation between two mid-latitude points at approximately the same distance north and south of the magnetic equator
“What is the approximate maximum range for signals using transequatorial propagation?”
A. 1000 miles
B. 2500 miles
C. 5000 miles
D. 7500 miles
C. 5000 miles
“What is the best time of day for transequatorial propagation?”
A. Morning
B. Noon
C. Afternoon or early evening
D. Late at night
C. Afternoon or early evening
“What is meant by the terms “extraordinary” and “ordinary” waves?”
A. Extraordinary waves describe rare long-skip propagation compared to ordinary waves, which travel shorter distances
B. Independent waves created in the ionosphere that are elliptically polarized
C. Long-path and short-path waves
D. Refracted rays and reflected waves
B. Independent waves created in the ionosphere that are elliptically polarized
“Which amateur bands typically support long-path propagation?”
A. Only 160 meters to 40 meters
B. Only 30 meters to 10 meters
C. 160 meters to 10 meters
D. 6 meters to 2 meters
C. 160 meters to 10 meters
“Which of the following amateur bands most frequently provides long-path propagation?”
A. 80 meters
B. 20 meters
C. 10 meters
D. 6 meters
B. 20 meters
“What happens to linearly polarized radio waves that split into ordinary and extraordinary waves in the ionosphere?”
A. They are bent toward the magnetic poles
B. They become depolarized
C. They become elliptically polarized
D. They become phase locked
C. They become elliptically polarized
“Why is chordal hop propagation desirable?”
A. The signal experiences less loss compared to multi-hop using Earth as a reflector
B. The MUF for chordal hop propagation is much lower than for normal skip propagation
C. Atmospheric noise is lower in the direction of chordal hop propagation
D. Signals travel faster along ionospheric chords
A. The signal experiences less loss compared to multi-hop using Earth as a reflector
“At what time of day can sporadic E propagation occur?”
A. Only around sunset
B. Only around sunset and sunrise
C. Only in hours of darkness
D. Any time
D. Any time
“What is the primary characteristic of chordal hop propagation?”
A. Propagation away from the great circle bearing between stations
B. Successive ionospheric refractions without an intermediate reflection from the ground
C. Propagation across the geomagnetic equator
D. Signals reflected back toward the transmitting station
B. Successive ionospheric refractions without an intermediate reflection from the ground