Ray diagram of sporadic E event

Sporadic E (abbreviated Es or SpE) is an unusual form of radio propagation using a low level of the Earth's ionosphere that normally does not refract radio waves.

Sporadic E propagation reflects signals off relatively small "clouds" in the lower E region located at altitudes of about 95~150 km (50~100 miles). The more conventional forms of skywave propagation in the ionosphere's higher F region refract off layers of electrons knocked off of gases by intense UV light, which are renewed on a fairly regular daily cycle. In both cases, the ionized material, when present, refracts (or "bends") 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 can only propagate by line-of-sight.[1]

Overview

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 May, with the peak most noticeable from early June. It begins trailing off through late July and into early August. A much smaller peak occurs around the winter solstice. For the mid-latitudes of the Southern Hemisphere, the timeframes are inversed; the highest activity occurring during the Winter Solstice.[2]

Communication distances of 800–2,200 km (500–1,400 miles) 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, which includes the FM broadcast band (87.5–108 MHz), band I VHF television (American TV channels 2–6, Russian channels 1–5, and European channels 2–4, which are no longer used in Western Europe), 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.[2]

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 [3] implies that there is a correlation between the formation of sporadic E and iron/magnesium meteor ablation in the ablation zone, 100 to 140km above the earth surface. Maruyama discusses this possibility further.[4]

Characteristic distances

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.

Sporadic E usually affects the lower VHF band I (TV channels 2–6, E2–E4, and R1–R5) and band II (88–108 MHz FM broadcast band). A 1945 FCC engineering study concluded that Es caused interference issues 1% of the time for a station broadcasting at 42 MHz, but only 0.01% for one at 84 MHz.[5]

The typical expected distances are about 600 to 1,400 miles (970 to 2,250 km). However, under exceptional circumstances, a highly ionized Es cloud can propagate band I VHF signals down to approximately 350 miles (560 km). When short-skip Es reception occurs, i.e., under 500 miles (800 km) in band I, there is a greater possibility that the ionized sporadic E cloud will be capable of reflecting a signal at a much higher frequency – i.e., a VHF band 3 channel – since a sharp reflection angle (short skip) favours low frequencies, a shallower reflection angle from the same ionized cloud will favour a higher frequency. In this case even Es DVB-T reception might be possible if a MUX uses VHF band 3, preferably channel E5, especially if QPSK mode is used, due to its low signal requirements. In addition to that, band 3 signals are more affected by tropospheric propagation which may indirectly increase the actual MUF because the signals only need to be refracted to low enough elevations that they get refracted towards the ground by the troposphere.

Equatorial sporadic E

Equatorial sporadic E is a regular daytime occurrence over the equatorial regions. For stations located within ±10° of the geomagnetic equator, equatorial E-skip can be expected on most days throughout the year, peaking around midday local time.

Auroral sporadic E

At polar latitudes, sporadic E can accompany auroras and associated disturbed magnetic conditions and is called auroral E.

Unlike equatorial or mid-latitude Es, sporadic E propagation over high latitude paths is rare, and supports unexpected contacts between locations surrounding the Arctic, even during periods of low solar activity.[6]

Occasional "bonanza" events

On 12 June 2009, sporadic E allowed some television viewers in the eastern United States to see VHF analog TV stations from other states at great distances, in places and on TV channels where local stations had already done their permanent analog shutdown on the final day of the DTV transition in the United States. This was possible because VHF has been mostly avoided by digital TV stations, leaving the analog stations the last ones on the band.

As of April 2010, it was possible for many in the U.S. to see Canadian and Mexican analog in this manner during sporadic E events; this should continue until all parts of those countries complete their own analog TV shutdowns over the succeeding few years.

In some cases it is even possible to get DTV Es receptions from well over 1,000 miles (1,600 km), since even for DTV, some U.S. stations still use band 1. These signals are characterized for being either extremely clear, or extremely blocky. They are also much easier to identify. Furthermore, ATSC 3.0 could make sporadic E DTV reception easier, due to its usual modulation scheme being more resistant to multipath propagation, as well as impulse noise encountered on those frequencies.

Notable sporadic E DX reception events

  • In 1939, there were some news reports of reception of an early Italian television service in England about 900 miles (1,400 km) away.[7]
  • The Medford Mail Tribune in Medford, Oregon reported on 1 June 1953, that KGNC-TV, channel 4 in Amarillo, and KFEL-TV, channel 2 from Denver had been received on the Trowbridge and Flynn Electric Company's television set at their Court Street warehouse, and with a pre-amplifier, a New York station's test pattern was reportedly picked up.[8]
  • In June 1981, Rijn Muntjewerff, in the Netherlands, received 55.25 MHz TV-2 Guaiba, Porto Alegre, Brazil, via a combination of sporadic E and afternoon TEP at a distance of 6,320 miles (10,170 km).[10]
  • On 20 July 2003, Jozsef Nemeth, in Győr, Hungary, received TR3 Radio Miras on OIRT FM 70.61 MHz from Uly Balkan, Türkmenistan, transmitter 1,895 miles or 3,050 kilometres away.[14]
  • On 26 June 2009, Paul Logan, in Lisnaskea, Northern Ireland, had transatlantic sporadic E reception on the FM band from eight US States and one Canadian Province. The most distant signal received was that of 90.7 WVAS radio in Montgomery, Alabama, at 6,456 km (4,012 miles). This reception was recorded and later confirmed by WVAS newsreader Marcus Hyles.[17]
  • On 24 November 2016, many radio listeners from Australia and New Zealand were able to listen to radio stations from other states of Australia, overlapping many radio signals. Many people complained about this, saying that many of their favorite radio stations got replaced by different radio stations from other states. Later, the ACMA confirmed that this was caused by sporadic E.[18]


See also

References

  1. ↑ "Sporadic E reference and resources". amfmdx.net. Archived from the original on 2007-06-24. Retrieved 2008-07-03.
  2. 1 2 "Using Sporadic E, Es Propagation for Ham Radio » Electronics Notes". www.electronics-notes.com. Retrieved 30 October 2023.
  3. ↑ Harrison, Roger. "Sporadic E - Stardust Propagation". Amateur Radio Magazine Volume 91 Number 1 2023.
  4. ↑ Maruyama, Takashi (2008). "Meteor-induced transient sporadic E as inferred from rapid-run ionosonde observations at midlatitudes". Journal of Geophysical Research: Space Physics. 113 (A9). Bibcode:2008JGRA..113.9308M. doi:10.1029/2008JA013362.
  5. ↑ "FCC expected to decide FM's place in spectrum about May 1". Broadcasting. 23 April 1945. p. 20.
  6. ↑ Mezoguchi, Kan (JA1BK) (June 2017). "6 meter polar Es - an underutilized propagation mode". QST. 101 (6): 41–42.{{cite journal}}: CS1 maint: numeric names: authors list (link)
  7. ↑ "Early Television in Italy". 16 March 2007. Archived from the original on 16 March 2007.
  8. ↑ Kramer, Ronald. "History of Television in Southern Oregon". Western States Museum of Broadcasting. Archived from the original on 2016-01-12. Retrieved 2009-08-16.
  9. ↑ "The Brimfield News". Retrieved 2020-08-06.
  10. ↑ "Rijn Muntjewerff's 1961–2005 TV DX". Todd Emslie's TV DX Page. Retrieved August 29, 2005.
  11. ↑ "Welcome to DX FM". Archived from the original on 2009-04-12.
  12. ↑ "Trans-Atlantic FM, 26 June 2003". www.dxradio.co.uk.
  13. ↑ "Transatlantic FM 03".
  14. ↑ Signal from 70.61 MHz (mp3). ucoz.hu (audio recording).
  15. ↑ "KBEJ-2 via Es". tvdxtips.com.
  16. ↑ "Short E-skip". www.tvdxexpo.com.
  17. ↑ "Transatlantic FM 09".
  18. ↑ "Sporadic E causing strange phenomena for Aussie radio stations". Radioinfo.com.au. 24 November 2016. Retrieved 26 November 2016.

Further reading

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