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Extra Class Exam Question Pool

effective 7/01/2008 thru 6/30/2012

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E3A: Earth-Moon-Earth communications; meteor scatter

E3A01: What is the approximate maximum separation along the surface of the Earth between two stations communicating by moonbounce?

12,000 miles, as long as both can “see” the moon

500 miles if the moon is at perigee

2000 miles, if the moon is at apogee

5000 miles, if the moon is at perigee



E3A02: What characterizes libration fading of an earth-moon-earth signal?

A fluttery irregular fading

A slow change in the pitch of the CW signal

A gradual loss of signal as the sun rises

The returning echo is several Hertz lower in frequency than the transmitted signal



E3A03: When scheduling EME contacts, which of these conditions will generally result in the least path loss?

When the moon is at perigee

When the moon is full

When the moon is at apogee

When the MUF is above 30 MHz



E3A04: What type of receiving system is desirable for EME communications?

Equipment with very low noise figures

Equipment with very wide bandwidth

Equipment with very low dynamic range

Equipment with very low gain



E3A05: What transmit and receive time sequencing is normally used on 144 MHz when attempting an EME contact?

Two-minute sequences, where one station transmits for a full two minutes and then receives for the following two minutes

One-minute sequences, where one station transmits for one minute and then receives for the following one minute

Two-and-one-half minute sequences, where one station transmits for a full 2.5 minutes and then receives for the following 2.5 minutes

Five-minute sequences, where one station transmits for five minutes and then receives for the following five minutes



E3A06: What transmit and receive time sequencing is normally used on 432 MHz when attempting an EME contact?

Two-and-one-half minute sequences, where one station transmits for a full 2.5 minutes and then receives for the following 2.5 minutes

Two-minute sequences, where one station transmits for a full two minutes and then receives for the following two minutes

One-minute sequences, where one station transmits for one minute and then receives for the following one minute

Five-minute sequences, where one station transmits for five minutes and then receives for the following five minutes



E3A07: What frequency range would you normally tune to find EME stations in the 2 meter band?

144.000 - 144.100 MHz

144.000 - 144.001 MHz

144.100 - 144.300 MHz

145.000 - 145.100 MHz



E3A08: What frequency range would you normally tune to find EME stations in the 70 cm band?

432.000 - 432.100 MHz

430.000 - 430.150 MHz

430.100 - 431.100 MHz

431.100 - 431.200 MHz



E3A09: When a meteor strikes the Earth's atmosphere, a cylindrical region of free electrons is formed at what layer of the ionosphere?

The E layer

The F1 layer

The F2 layer

The D layer



E3A10: Which range of frequencies is well suited for meteor-scatter communications?

28 - 148 MHz

1.8 - 1.9 MHz

10 - 14 MHz

220 - 450 MHz



E3A11: What transmit and receive time sequencing is normally used on 144 MHz when attempting a meteor-scatter contact?

15-second sequences, where one station transmits for 15 seconds and then receives for the following 15 seconds

Two-minute sequences, where one station transmits for a full two minutes and then receives for the following two minutes

One-minute sequences, where one station transmits for one minute and then receives for the following one minute

30-second sequences, where one station transmits for 30 seconds and then receives for the following 30 seconds





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