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Sporadic E propagation
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Sporadic E propagation
Sporadic E (abbreviated Es or SpE) is an uncommon form of radio propagation using a low level of the Earth's ionosphere that normally does not refract radio waves above about 15 MHz.
Sporadic E propagation reflects signals off relatively small ionization patches in the lower E region located at altitudes of about 95–120 km (59–75 mi). The more conventional forms of skywave propagation in the ionosphere's higher F region refract off layers of electrons that are knocked off gas atoms and molecules by intense UV light, which are renewed on a regular repeating daily cycle. In both cases, the electrons, when present, refract (or "bend") radio signals back toward the Earth's surface creating a "bent pipe" path for radio signals.
The Es propagation often supports occasional long-distance communication during the approximately 6 weeks centered on summer solstice at very high frequencies (VHF), which under normal conditions propagate mostly by line-of-sight.
As its name suggests, sporadic E is an unpredictable event that can happen at almost any time; it does, however, display strong seasonal and diurnal patterns. Sporadic E activity peaks predictably near the solstices in both hemispheres. In the mid-latitude of the Northern Hemisphere, activity usually begins in mid-May, with the peak most noticeably beginning in early June. It begins trailing off after mid-July and becomes much less reliable by early August. A much smaller sporadic-E peak occurs during the winter solstice. For the mid-latitudes of the Southern Hemisphere, the timeframes are inversed; the highest activity occurring during their summer solstice.
Communication distances of 800–2,200 km (500–1,370 mi) can occur using a single Es cloud. This variability in distance depends on a number of factors, including cloud height and density. The maximum usable frequency (MUF) also varies widely, but most commonly falls in the 25–150 MHz range. This includes the band II FM broadcast band (87.5–108 MHz), band I VHF television (former American analog TV channels A2–A6, Russian channels R1–R5, and former European analog channels E2–E4), CB radio (27 MHz), and the amateur radio 2 meter, 4 m, 6 m, and 10 m bands. On very rare occasions, a MUF of 225 MHz can be attained.
No conclusive theory has yet been formulated as to the origin of sporadic E. Attempts to connect the incidence of sporadic E with the eleven-year Sunspot cycle have provided tentative correlations. There seems to be a positive correlation between sunspot maximum and Es activity in Europe. Conversely, there seems to be a negative correlation between maximum sunspot activity and Es activity in Australasia. Harrison implies that there is a correlation between the formation of sporadic E and iron/magnesium micrometeoroid ablation in the ablation zone, 100 to 140 km (62 to 87 mi) above the earth surface. Maruyama discusses this possibility further.
Television and FM signals received via sporadic E can be extremely strong and range in strength over a short period from just detectable to overloading. Although polarisation shift can occur, single-hop Es signals tend to remain in the original transmitted polarization. Long single-hop (900–1,500 miles or 1,400–2,400 kilometres) sporadic E television signals tend to be more stable and relatively free of multipath images.
Shorter-skip (400–800 miles or 640–1,290 kilometres) signals tend to be reflected from more than one part of the sporadic E layer, resulting in multiple images and ghosting, with phase reversal at times. Picture degradation and signal-strength attenuation worsens with each subsequent sporadic E hop.
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Sporadic E propagation
Sporadic E (abbreviated Es or SpE) is an uncommon form of radio propagation using a low level of the Earth's ionosphere that normally does not refract radio waves above about 15 MHz.
Sporadic E propagation reflects signals off relatively small ionization patches in the lower E region located at altitudes of about 95–120 km (59–75 mi). The more conventional forms of skywave propagation in the ionosphere's higher F region refract off layers of electrons that are knocked off gas atoms and molecules by intense UV light, which are renewed on a regular repeating daily cycle. In both cases, the electrons, when present, refract (or "bend") radio signals back toward the Earth's surface creating a "bent pipe" path for radio signals.
The Es propagation often supports occasional long-distance communication during the approximately 6 weeks centered on summer solstice at very high frequencies (VHF), which under normal conditions propagate mostly by line-of-sight.
As its name suggests, sporadic E is an unpredictable event that can happen at almost any time; it does, however, display strong seasonal and diurnal patterns. Sporadic E activity peaks predictably near the solstices in both hemispheres. In the mid-latitude of the Northern Hemisphere, activity usually begins in mid-May, with the peak most noticeably beginning in early June. It begins trailing off after mid-July and becomes much less reliable by early August. A much smaller sporadic-E peak occurs during the winter solstice. For the mid-latitudes of the Southern Hemisphere, the timeframes are inversed; the highest activity occurring during their summer solstice.
Communication distances of 800–2,200 km (500–1,370 mi) can occur using a single Es cloud. This variability in distance depends on a number of factors, including cloud height and density. The maximum usable frequency (MUF) also varies widely, but most commonly falls in the 25–150 MHz range. This includes the band II FM broadcast band (87.5–108 MHz), band I VHF television (former American analog TV channels A2–A6, Russian channels R1–R5, and former European analog channels E2–E4), CB radio (27 MHz), and the amateur radio 2 meter, 4 m, 6 m, and 10 m bands. On very rare occasions, a MUF of 225 MHz can be attained.
No conclusive theory has yet been formulated as to the origin of sporadic E. Attempts to connect the incidence of sporadic E with the eleven-year Sunspot cycle have provided tentative correlations. There seems to be a positive correlation between sunspot maximum and Es activity in Europe. Conversely, there seems to be a negative correlation between maximum sunspot activity and Es activity in Australasia. Harrison implies that there is a correlation between the formation of sporadic E and iron/magnesium micrometeoroid ablation in the ablation zone, 100 to 140 km (62 to 87 mi) above the earth surface. Maruyama discusses this possibility further.
Television and FM signals received via sporadic E can be extremely strong and range in strength over a short period from just detectable to overloading. Although polarisation shift can occur, single-hop Es signals tend to remain in the original transmitted polarization. Long single-hop (900–1,500 miles or 1,400–2,400 kilometres) sporadic E television signals tend to be more stable and relatively free of multipath images.
Shorter-skip (400–800 miles or 640–1,290 kilometres) signals tend to be reflected from more than one part of the sporadic E layer, resulting in multiple images and ghosting, with phase reversal at times. Picture degradation and signal-strength attenuation worsens with each subsequent sporadic E hop.
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