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Subelement B-007

B-007

Section B-007-005

Section B-007-005

How do sunspots change the ionization of the atmosphere?

  • The more sunspots there are, the lesser the ionization
  • They have no effect
  • Correct Answer
    The more sunspots there are, the greater the ionization
  • Unless there are sunspots, the ionization is zero

The number of sunspots visible on the surface of the Sun is related to overall solar activity. The higher the sunspot numbers, the higher the emission of Ultraviolet (UV) and particles. Ionization is directly influenced by the level of radiation.

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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How long is an average sunspot cycle?

  • 5 years
  • Correct Answer
    11 years
  • 17 years
  • 7 years

Key word: AVERAGE. The duration of the solar cycles varies from 7 to 17 years but the AVERAGE is 11 YEARS.

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 is solar flux?

  • The number of sunspots on the side of the sun facing the Earth
  • The density of the sun's magnetic field
  • Correct Answer
    The radio frequency energy emitted by the sun
  • A measure of the tilt of the Earth's ionosphere on the side toward the sun

The Sun's activity can be observed by visually counting sunspots but also by measuring noise at a microwave frequency. Sunspot numbers and solar flux are well co-related. The measurement of the solar flux is reported as a Solar Flux Index.

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 is the solar-flux index?

  • A measure of solar activity that is taken annually
  • Another name for the smoothed sunspot number (SSN)
  • Correct Answer
    A measure of solar activity that is taken at a specific frequency
  • A measure of solar activity that compares daily readings with results from the last six months

The Sun's activity can be observed by visually counting sunspots but also by measuring noise at a microwave frequency. Sunspot numbers and solar flux are well co-related. The measurement of the solar flux is reported as a Solar Flux Index.

Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.

Tags: none

What influences all radiocommunication beyond ground wave or line-of-sight ranges?

  • Correct Answer
    Solar radiation
  • The F1 region of the ionosphere
  • Lunar tidal effects
  • The F2 region of the ionosphere

Because the Sun affects the ionosphere and the troposphere (e.g., temperature inversions), it can be said that it has an influence on all radiocommunications.

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 of the sun's activity influences ionospheric propagation on a daily basis?

  • Correct Answer
    Electromagnetic and particle radiation
  • Infrared radiation
  • Solar wind
  • Coronal mass ejections (CME)

Ultraviolet (UV) rays, a form of electromagnetic radiation, and particles [namely alpha and beta] are responsible for ionization in the ionosphere.

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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When sunspot numbers are high, how is propagation affected?

  • High frequency radio signals become weak and distorted
  • High frequency radio signals are absorbed
  • Correct Answer
    Frequencies up to 40 MHz or even higher become usable for long-distance communication
  • Frequencies up to 100 MHz or higher are normally usable for long-distance communication

Maximum Usable Frequencies (MUF) in the range of 30 to 50 MHz become possible during solar cycle peaks. Stronger ionization allows upper regions of the ionosphere to refract higher frequencies rather than let them escape into space (as is the case during solar cycle lows).

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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All communication frequencies throughout the spectrum are affected in varying degrees by:

  • Correct Answer
    the sun
  • the ionosphere
  • auroras
  • meteor showers

Because the Sun affects the ionosphere and the troposphere (e.g., temperature inversions), it can be said that it has an influence on all radiocommunications.

Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.

Tags: none

Average duration of a solar cycle is:

  • 6 years
  • 1 year
  • 3 years
  • Correct Answer
    11 years

Key word: AVERAGE. The duration of the solar cycles varies from 7 to 17 years but the AVERAGE is 11 YEARS.

Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.

Tags: none

The ability of the ionosphere to refract high frequency radio signals depends on:

  • the receiver sensitivity
  • Correct Answer
    the amount of solar radiation
  • the power of the transmitted signal
  • upper atmosphere weather conditions

Ionization makes refraction possible. Ultraviolet (UV) rays, a form of electromagnetic radiation, and particles [namely alpha and beta] are responsible for ionization in the ionosphere.

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 the major cause of cyclical changes in HF propagation?

  • Magnetic pole drift cycle
  • Jet stream cycle
  • Auroral cycle
  • Correct Answer
    Solar cycle

Apart from daily variations in solar radiation, HF propagation is impacted by the solar cycles. The duration of the solar cycles varies from 7 to 17 years but the AVERAGE is 11 YEARS.

Original copyright; explanations transcribed with permission from Francois VE2AAY, author of the ExHAMiner exam simulator. Do not copy without his permission.

Tags: none

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