SUBELEMENT G3 - RADIO WAVE PROPAGATION Flashcards
G3A01 (A)
What is the significance of the sunspot number with regard to HF propagation?
A. Higher sunspot numbers generally indicate a greater probability of good propagation at higher frequencies
G3A02 (B)
What effect does a Sudden Ionospheric Disturbance have on the daytime ionospheric propagation of HF radio waves?
B. It disrupts signals on lower frequencies more than those on higher frequencies
G3A03 (C)
Approximately how long does it take the increased ultraviolet and X-ray radiation from solar flares to affect radio propagation on the Earth?
C. 8 minutes
G3A04 (D)
Which of the following are least reliable for long distance communications during periods of low solar activity?
D. 15 meters, 12 meters and 10 meters
G3A05 (D)
What is the solar flux index?
D. A measure of solar radiation at 10.7 centimeters wavelength
G3A06 (D)
What is a geomagnetic storm?
D. A temporary disturbance in the Earth’s magnetosphere
G3A07 (D)
At what point in the solar cycle does the 20-meter band usually support worldwide propagation during daylight hours?
D. At any point in the solar cycle
G3A08 (B)
Which of the following effects can a geomagnetic storm have on radio propagation?
B. Degraded high-latitude HF propagation
G3A09 (C)
What effect does a high sunspot number have on radio communications?
C. Long-distance communication in the upper HF and lower VHF range is enhanced
G3A10 (C)
What causes HF propagation conditions to vary periodically in a 28 day cycle?
C. The Sun’s rotation on its axis
G3A11 (D)
Approximately how long is the typical sunspot cycle?
D. 11 years
G3A12 (B)
What does the K-index indicate?
B. The short term stability of the Earth’s magnetic field
G3A13 (C)
What does the A-index indicate?
C. The long term stability of the Earth’s geomagnetic field
G3A14 (B)
How are radio communications usually affected by the charged particles that reach the Earth from solar coronal holes?
B. HF communications are disturbed
G3A15 (D)
How long does it take charged particles from coronal mass ejections to affect radio propagation on the Earth?
D. 20 to 40 hours
G3A16 (A)
What is a possible benefit to radio communications resulting from periods of high geomagnetic activity?
A. Auroras that can reflect VHF signals