B-007
B-007
Section B-007-007
Which ionospheric region most affects sky-wave propagation on the 6-metre band?
At 50 MHz to 54 MHz, a 6-metre signal normally escapes into space. However, 'Sporadic E' ( intense but temporary ionization of patches in the upper reaches of the E region ) can provide refraction paths for 6 metres.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
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What effect does tropospheric bending have on 2-metre radio waves?
Key word: BENDING. Tropospheric bending : refraction occurs when a wave travels through masses of differing densities (humidity content) in the troposphere. The wave travels further rather than escape right away into space.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
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What causes tropospheric ducting of radio waves?
Key word: DUCTING. Wave gets caught (like in a waveguide) between sandwiched masses of different humidity contents. A 'temperature inversion', where hot air masses find themselves riding over cooler air, leads to conditions supporting 'Ducting'. Except for 'Tropo Ducting', common troposcatter (scattering through the troposphere) opens VHF paths out to 500 km for well-equipped stations (800 at the most). 'Tropospheric Ducting' permits distances beyond 800 km.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
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What term describes that portion of a transmitted wave kept close to the Earth's surface due to bending in the atmosphere?
Key word: BENDING. Tropospheric bending : refraction occurs when a wave travels through masses of differing densities (humidity content) in the troposphere. The wave travels further rather than escape right away into space.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
What is a sporadic-E condition?
At 50 MHz to 54 MHz, a 6-metre signal normally escapes into space. However, 'Sporadic E' ( intense but temporary ionization of patches in the upper reaches of the E region ) can provide refraction paths for 6 metres.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
On which amateur radio band is the extended-distance propagation effect of sporadic-E most often observed?
At 50 MHz to 54 MHz, a 6-metre signal normally escapes into space. However, 'Sporadic E' ( intense but temporary ionization of patches in the upper reaches of the E region ) can provide refraction paths for 6 metres.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
In the northern hemisphere, in which direction should a directional antenna be pointed to take maximum advantage of auroral propagation?
Key word: AURORA. The arrival of high-energy particles from the Sun (e.g., after a solar flare) disturbs the Earth's magnetic field (a geomagnetic storm). The resulting unusual ionization of gases in the E region above the poles produces the visual display known as 'aurora' ("Northern Lights"). Pointing antennas at the aurora front permit oblique paths to distant stations through back scattering.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
Where in the ionosphere does auroral activity occur?
Key word: AURORA. The arrival of high-energy particles from the Sun (e.g., after a solar flare) disturbs the Earth's magnetic field (a geomagnetic storm). The resulting unusual ionization of gases in the E region above the poles produces the visual display known as 'aurora' ("Northern Lights"). Pointing antennas at the aurora front permit oblique paths to distant stations through back scattering.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
Which analog emission mode is the most reliable in auroral propagation?
The unstable front of the ionized regions and the ensuing scattering of the radio wave make for distorted signals, only the smaller bandwidth signals are usable.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
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Excluding enhanced propagation modes, what is the approximate range of normal VHF tropospheric propagation?
Common troposcatter (scattering through the troposphere) opens VHF paths out to 500 km for well-equipped stations (800 at the most). 'Tropospheric Ducting' (where a wave gets caught between sandwiched air masses during a 'temperature inversion') permits distances beyond 800 km.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none
What effect is responsible for propagating a VHF signal over 800 km?
Common troposcatter (scattering through the troposphere) opens VHF paths out to 500 km for well-equipped stations (800 at the most). 'Tropospheric Ducting' (where a wave gets caught between sandwiched air masses during a 'temperature inversion') permits distances beyond 800 km.
Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.
Tags: none