Propagation prediction and reporting: radio horizon; effects of space-weather phenomena
E3C01
What is the cause of short-term radio blackouts?
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A
Coronal mass ejections
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B
Sunspots on the solar equator
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C
North-oriented interplanetary magnetic field
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D
Solar flares
E3C02
What is indicated by a rising A-index or K-index?
-
A
Increasing disturbance of the geomagnetic field
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B
Decreasing disturbance of the geomagnetic field
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C
Higher levels of solar UV radiation
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D
An increase in the critical frequency
E3C03
Which of the following signal paths is most likely to experience high levels of absorption when the A-index or K-index is elevated?
-
A
Transequatorial
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B
Through the auroral oval
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C
Sporadic-E
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D
NVIS
E3C04
What does the value of Bz (B sub z) represent?
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A
Geomagnetic field stability
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B
Critical frequency for vertical transmissions
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C
North-south strength of the interplanetary magnetic field
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D
Duration of long-delayed echoes
E3C05
What orientation of Bz (B sub z) increases the likelihood that charged particles from the Sun will cause disturbed conditions?
-
A
Southward
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B
Northward
-
C
Eastward
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D
Westward
E3C06
How does the VHF/UHF radio horizon compare to the geographic horizon?
-
A
It is approximately 15 percent farther
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B
It is approximately 20 percent nearer
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C
It is approximately 50 percent farther
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D
They are approximately the same
E3C07
Which of the following indicates the greatest solar flare intensity?
-
A
Class A
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B
Class Z
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C
Class M
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D
Class X
E3C08
Which of the following is the space-weather term for an extreme geomagnetic storm?
-
A
B9
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B
X5
-
C
M9
-
D
G5
E3C09
What type of data is reported by amateur radio propagation reporting networks?
-
A
Solar flux
-
B
Electric field intensity
-
C
Magnetic declination
-
D
Digital-mode and CW signals
E3C10
What does the 304A solar parameter measure?
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A
The ratio of X-ray flux to radio flux, correlated to sunspot number
-
B
UV emissions at 304 angstroms, correlated to the solar flux index
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C
The solar wind velocity at an angle of 304 degrees from the solar equator, correlated to geomagnetic storms
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D
The solar emission at 304 GHz, correlated to X-ray flare levels
E3C11
What does VOACAP software model?
-
A
AC voltage and impedance
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B
VHF radio propagation
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C
HF propagation
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D
AC current and impedance
E3C12
Which of the following is indicated by a sudden rise in radio background noise across a large portion of the HF spectrum?
-
A
A temperature inversion has occurred
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B
A coronal mass ejection impact or a solar flare has occurred
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C
Transequatorial propagation on 6 meters is likely
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D
Long-path propagation on the higher HF bands is likely