Sporadic E propagation: Difference between revisions

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[[File:SporadicE-NPS.gif|thumb|Ray diagram of sporadic E event]]
[[File:SporadicE-NPS.gif|thumb|Ray diagram of sporadic E event]]


'''Sporadic E''' (abbreviated '''E{{sub|s}}''' 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''' (abbreviated '''E{{sub|s}}''' 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 (50–75 miles). The more conventional forms of [[skywave]] propagation in the ionosphere's higher [[F region]] refract off layers of electrons knocked off of gas atoms and molecules by intense [[UV light]], which are renewed on a regular repeating daily cycle. In both cases, the electrons, when present, refracts (or "bends") radio signals back toward the Earth's surface creating a "bent pipe" path for radio signals.
Sporadic E propagation reflects signals off relatively small ionization patches in the lower [[E region]] located at altitudes of about {{convert|95|–|120|km|mi|abbr=on}}. The more conventional forms of [[skywave]] propagation in the ionosphere's higher [[F region]] refract off layers of electrons knocked off of gas atoms and molecules by intense [[UV light]], which are renewed on a regular repeating daily cycle. In both cases, the electrons, when present, refracts (or "bends") radio signals back toward the Earth's surface creating a "bent pipe" path for radio signals.


The E{{sub|s}} propagation often supports occasional long-distance communication during the approximately 6&nbsp;weeks centered on summer solstice at [[Very high frequency|very high frequencies (VHF)]], which under normal conditions can usually propagate mostly by [[Line-of-sight propagation|line-of-sight]].<ref>{{cite web |title=Sporadic&nbsp;E reference and resources |website=amfmdx.net |url=http://www.amfmdx.net/fmdx/sporadic-e.html |access-date=2008-07-03 |url-status=dead |archive-url=https://web.archive.org/web/20070624122447/http://www.amfmdx.net/fmdx/sporadic-e.html |archive-date=2007-06-24}}</ref>
The E{{sub|s}} propagation often supports occasional long-distance communication during the approximately 6&nbsp;weeks centered on summer solstice at [[Very high frequency|very high frequencies (VHF)]], which under normal conditions can usually propagate mostly by [[Line-of-sight propagation|line-of-sight]].<ref>{{cite web |title=Sporadic&nbsp;E reference and resources |website=amfmdx.net |url=http://www.amfmdx.net/fmdx/sporadic-e.html |access-date=2008-07-03 |url-status=dead |archive-url=https://web.archive.org/web/20070624122447/http://www.amfmdx.net/fmdx/sporadic-e.html |archive-date=2007-06-24}}</ref>
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As its name suggests, sporadic&nbsp;E is an unpredictable event that can happen at almost any time; it does, however, display strong seasonal and diurnal patterns. Sporadic&nbsp;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.<ref name="notes">{{cite web |title=Using Sporadic E, Es Propagation for Ham Radio » Electronics Notes |url=https://www.electronics-notes.com/articles/ham_radio/amateur-propagation/sporadic-e-es.php |website=www.electronics-notes.com |access-date=30 October 2023}}</ref>
As its name suggests, sporadic&nbsp;E is an unpredictable event that can happen at almost any time; it does, however, display strong seasonal and diurnal patterns. Sporadic&nbsp;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.<ref name="notes">{{cite web |title=Using Sporadic E, Es Propagation for Ham Radio » Electronics Notes |url=https://www.electronics-notes.com/articles/ham_radio/amateur-propagation/sporadic-e-es.php |website=www.electronics-notes.com |access-date=30 October 2023}}</ref>


Communication distances of 800–2,200&nbsp;km (500–1,400&nbsp;miles) can occur using a single E{{sub|s}} cloud. This variability in distance depends on a number of factors, including cloud height and density. The [[Maximum usable frequency|maximum usable frequency (MUF)]] also varies widely, but most commonly falls in the 25–150&nbsp;[[Megahertz|MHz]] range, which includes the band&nbsp;II [[FM broadcast band]] (87.5–108&nbsp;MHz), band&nbsp;I [[VHF]] [[television]] (American TV channels&nbsp;A2–A6, Russian channels&nbsp;R1–R5, and European channels&nbsp;E2–E4, which are no longer used in Western Europe), [[CB radio]] (27&nbsp;MHz), and the [[amateur radio]] [[2-meter band|2&nbsp;meter]], [[4-metre band|4&nbsp;m]], [[6-meter band|6&nbsp;m]], and [[10-meter band|10&nbsp;m]] bands. On very rare occasions, a MUF of 225&nbsp;MHz can be attained.<ref name="notes" />
Communication distances of {{convert|800|–|2,200|km|mi|abbr=on}} can occur using a single E{{sub|s}} cloud. This variability in distance depends on a number of factors, including cloud height and density. The [[Maximum usable frequency|maximum usable frequency (MUF)]] also varies widely, but most commonly falls in the 25–150&nbsp;[[Megahertz|MHz]] range, which includes the band&nbsp;II [[FM broadcast band]] (87.5–108&nbsp;MHz), band&nbsp;I [[VHF]] [[television]] (American TV channels&nbsp;A2–A6, Russian channels&nbsp;R1–R5, and European channels&nbsp;E2–E4, which are no longer used in Western Europe), [[CB radio]] (27&nbsp;MHz), and the [[amateur radio]] [[2-meter band|2&nbsp;meter]], [[4-metre band|4&nbsp;m]], [[6-meter band|6&nbsp;m]], and [[10-meter band|10&nbsp;m]] bands. On very rare occasions, a MUF of 225&nbsp;MHz can be attained.<ref name="notes" />


No conclusive theory has yet been formulated as to the origin of sporadic&nbsp;E. Attempts to connect the incidence of sporadic&nbsp;E with the eleven-year [[Sunspot cycle]] have provided tentative correlations. There seems to be a positive correlation between sunspot maximum and E{{sub|s}} activity in Europe. Conversely, there seems to be a negative correlation between maximum sunspot activity and E{{sub|s}} activity in [[Australasia]]. Harrison <ref>{{cite web |author=Harrison, Roger |title=Sporadic E - Stardust Propagation |publisher=Amateur Radio Magazine Volume 91 Number 1 2023|url=https://www.wia.org.au/members/armag/2023/january/}}</ref> implies that there is a correlation between the formation of sporadic&nbsp;E and iron/magnesium micrometeoroid ablation in the ablation zone, 100 to 140&nbsp;km (60 to 90 miles) above the earth surface. Maruyama discusses this possibility further.<ref>{{cite journal |author=Maruyama, Takashi |title=Meteor-induced transient sporadic E as inferred from rapid-run ionosonde observations at midlatitudes |year=2008 |journal=Journal of Geophysical Research: Space Physics|volume=113 |issue=A9 |doi=10.1029/2008JA013362 |bibcode=2008JGRA..113.9308M |doi-access=free }}</ref>
No conclusive theory has yet been formulated as to the origin of sporadic&nbsp;E. Attempts to connect the incidence of sporadic&nbsp;E with the eleven-year [[Sunspot cycle]] have provided tentative correlations. There seems to be a positive correlation between sunspot maximum and E{{sub|s}} activity in Europe. Conversely, there seems to be a negative correlation between maximum sunspot activity and E{{sub|s}} activity in [[Australasia]]. Harrison <ref>{{cite web |author=Harrison, Roger |title=Sporadic E - Stardust Propagation |publisher=Amateur Radio Magazine Volume 91 Number 1 2023|url=https://www.wia.org.au/members/armag/2023/january/}}</ref> implies that there is a correlation between the formation of sporadic&nbsp;E and iron/magnesium micrometeoroid ablation in the ablation zone, {{convert|100|to|140|km|mi|abbr=on}} above the earth surface. Maruyama discusses this possibility further.<ref>{{cite journal |author=Maruyama, Takashi |title=Meteor-induced transient sporadic E as inferred from rapid-run ionosonde observations at midlatitudes |year=2008 |journal=Journal of Geophysical Research: Space Physics|volume=113 |issue=A9 |doi=10.1029/2008JA013362 |bibcode=2008JGRA..113.9308M |doi-access=free }}</ref>


==Characteristic distances==
==Characteristic distances==
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===Equatorial sporadic&nbsp;E===
===Equatorial sporadic&nbsp;E===
{{no sources|section|date=March 2025}}
{{unreferenced section|date=March 2025}}
[[Equator]]ial sporadic&nbsp;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.
[[Equator]]ial sporadic&nbsp;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.


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As of April&nbsp;2010, it was possible for many in the U.S. to see Canadian and Mexican analog in this manner during sporadic&nbsp;E events; this should continue until all parts of those countries complete their own analog TV shutdowns over the succeeding few years.
As of April&nbsp;2010, it was possible for many in the U.S. to see Canadian and Mexican analog in this manner during sporadic&nbsp;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 E{{sub|s}} receptions from well over 1,000&nbsp;miles (1,600&nbsp;km), since even for DTV, some U.S. stations still use band&nbsp;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&nbsp;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.{{citation needed|date=July 2019}}
In some cases it is even possible to get DTV E{{sub|s}} receptions from well over {{convert|1,000|mi|km}}, since even for DTV, some U.S. stations still use band&nbsp;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&nbsp;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.{{citation needed|date=July 2019}}


=== Notable sporadic&nbsp;E DX reception events ===
=== Notable sporadic&nbsp;E DX reception events ===
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* On July 6, 2004, an intense high [[Maximum usable frequency|MUF]] Sporadic-E opening allowed Mike Bugaj of [[Enfield, Connecticut]],<ref>{{Cite web |url=http://pages.cthome.net/fmdx |title=Mike's TV and FM DX page |access-date=February 12, 2008 |archive-url=https://web.archive.org/web/20080130183048/http://pages.cthome.net/fmdx/ |archive-date=January 30, 2008 |url-status=dead }}</ref> to receive [[KATV]] A7<ref>{{cite web | title=High Band E Skip | work=Mike's TV and FM DX Page | url=http://fmdx.usclargo.com/hibandes.html | access-date=April 26, 2005}}</ref> {{convert|1176|mi|km}} from [[Little Rock, Arkansas]].<ref>See [[E-skip#Notable sporadic E DX receptions]]</ref>
* On July 6, 2004, an intense high [[Maximum usable frequency|MUF]] Sporadic-E opening allowed Mike Bugaj of [[Enfield, Connecticut]],<ref>{{Cite web |url=http://pages.cthome.net/fmdx |title=Mike's TV and FM DX page |access-date=February 12, 2008 |archive-url=https://web.archive.org/web/20080130183048/http://pages.cthome.net/fmdx/ |archive-date=January 30, 2008 |url-status=dead }}</ref> to receive [[KATV]] A7<ref>{{cite web | title=High Band E Skip | work=Mike's TV and FM DX Page | url=http://fmdx.usclargo.com/hibandes.html | access-date=April 26, 2005}}</ref> {{convert|1176|mi|km}} from [[Little Rock, Arkansas]].<ref>See [[E-skip#Notable sporadic E DX receptions]]</ref>
* On June 15, 2005, Danny Oglethorpe in [[Shreveport]], [[Louisiana]], received a [[KBEJ-TV]] test signal on channel&nbsp;A2, from [[Fredericksburg, Texas]], by sporadic&nbsp;E, at a very short distance for this propagation mode: {{convert|327|mi|km}}.<ref>{{cite web |title=KBEJ-2 via E{{sub|s}} |website=tvdxtips.com |url=http://www.tvdxtips.com/kbej2es.html}}</ref><ref>{{cite web |title=Short E-skip |website=www.tvdxexpo.com |url=http://www.tvdxexpo.com/usac/shortes.htm}}</ref>
* On June 15, 2005, Danny Oglethorpe in [[Shreveport]], [[Louisiana]], received a [[KBEJ-TV]] test signal on channel&nbsp;A2, from [[Fredericksburg, Texas]], by sporadic&nbsp;E, at a very short distance for this propagation mode: {{convert|327|mi|km}}.<ref>{{cite web |title=KBEJ-2 via E{{sub|s}} |website=tvdxtips.com |url=http://www.tvdxtips.com/kbej2es.html}}</ref><ref>{{cite web |title=Short E-skip |website=www.tvdxexpo.com |url=http://www.tvdxexpo.com/usac/shortes.htm}}</ref>
* On June 26, 2009, Paul Logan, in [[Lisnaskea]], Ireland, had transatlantic sporadic&nbsp;E reception on the FM band from eight US States and one Canadian Province. The most distant signal received was that of 90.7&nbsp;[[WVAS]] radio in [[Montgomery, Alabama]], at 6,456&nbsp;km (4,012&nbsp;miles). This reception was recorded and later confirmed by [[WVAS]] newsreader Marcus Hyles.<ref>{{cite web |title = Transatlantic FM&nbsp;09 |url=https://band2dx.webs.com/tafm09.htm}}</ref>
* On June 26, 2009, Paul Logan, in [[Lisnaskea]], Ireland, had transatlantic sporadic&nbsp;E reception on the FM band from eight US States and one Canadian Province. The most distant signal received was that of 90.7&nbsp;[[WVAS]] radio in [[Montgomery, Alabama]], at {{convert|6,456|km|mi|abbr=on}}. This reception was recorded and later confirmed by [[WVAS]] newsreader Marcus Hyles.<ref>{{cite web |title = Transatlantic FM&nbsp;09 |url=https://band2dx.webs.com/tafm09.htm}}</ref>
* On May 31, 2010, Mike Fallon, in [[East Sussex]], United Kingdom, received a transatlantic signal from the religious station La Voz de la Luz,<ref>{{Cite web |title=La Luz FM Higüey En Línea RD |url=https://radios.com.do/luz-higuey/ |access-date=2025-01-29 |website=Radios.com.do |language=es-DO}}</ref> in Salvaléon de Higüey,<ref>{{Citation |title=Salvaleón de Higüey |date=2022-07-09 |work=Simple English Wikipedia, the free encyclopedia |url=https://simple.wikipedia.org/wiki/Salvale%C3%B3n_de_Hig%C3%BCey |access-date=2025-01-29 |language=en}}</ref>{{cite needed|date=May 2025}} a radio station in the Dominican Republic on 88.7MHz from 12:48 UTC for approximately 20 minutes at a distance of {{convert|4302|mi|km}} via multihop Sporadic-E. This reception was confirmed via an email from the station.{{cn|date=May 2025}}
* On May 31, 2010, Mike Fallon, in [[East Sussex]], United Kingdom, received a transatlantic signal from the religious station La Voz de la Luz,<ref>{{Cite web |title=La Luz FM Higüey En Línea RD |url=https://radios.com.do/luz-higuey/ |access-date=2025-01-29 |website=Radios.com.do |language=es-DO}}</ref> in Salvaléon de Higüey,<ref>{{Citation |title=Salvaleón de Higüey |date=2022-07-09 |work=Simple English Wikipedia, the free encyclopedia |url=https://simple.wikipedia.org/wiki/Salvale%C3%B3n_de_Hig%C3%BCey |access-date=2025-01-29 |language=en}}</ref>{{citation needed|date=May 2025}} a radio station in the Dominican Republic on 88.7&nbsp;MHz from 12:48 UTC for approximately 20 minutes at a distance of {{convert|4302|mi|km}} via multihop Sporadic-E. This reception was confirmed via an email from the station.{{citation needed|date=May 2025}}
* On November 24, 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 [[Australian Communications and Media Authority|ACMA]] confirmed that this was caused by sporadic&nbsp;E.<ref>{{cite web |title=Sporadic&nbsp;E causing strange phenomena for Aussie radio stations |website=Radioinfo.com.au |date=24 November 2016 |url=https://www.radioinfo.com.au/news/sporadic-e-causing-strange-phenomena-aussie-radio-stations |access-date=26 November 2016}}</ref>
* On November 24, 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 [[Australian Communications and Media Authority|ACMA]] confirmed that this was caused by sporadic&nbsp;E.<ref>{{cite web |title=Sporadic&nbsp;E causing strange phenomena for Aussie radio stations |website=Radioinfo.com.au |date=24 November 2016 |url=https://www.radioinfo.com.au/news/sporadic-e-causing-strange-phenomena-aussie-radio-stations |access-date=26 November 2016}}</ref>



Latest revision as of 11:52, 16 June 2025

Template:Short description Template:More citations needed

File:SporadicE-NPS.gif
Ray diagram of sporadic E event

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 Template:Convert. The more conventional forms of skywave propagation in the ionosphere's higher F region refract off layers of electrons knocked off of gas atoms and molecules by intense UV light, which are renewed on a regular repeating daily cycle. In both cases, the electrons, 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 usually propagate mostly 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 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.[2]

Communication distances of Template:Convert 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 band II FM broadcast band (87.5–108 MHz), band I VHF television (American TV channels A2–A6, Russian channels R1–R5, and European channels E2–E4, 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 micrometeoroid ablation in the ablation zone, Template:Convert 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 (Template:Convert) sporadic E television signals tend to be more stable and relatively free of multipath images.

Shorter-skip (Template:Convert) 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 A2–A6, 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 Template:Convert. However, under exceptional circumstances, a highly ionized Es cloud can propagate band I VHF signals down to approximately Template:Convert. When short-skip Es reception occurs, i.e., under Template:Convert 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

Script error: No such module "Unsubst". 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 Template:Convert, 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.Script error: No such module "Unsubst".

Notable sporadic E DX reception events


See also

References

Template:Reflist

Further reading

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