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- Channel_37 abstract "Channel 37 is an unused television channel in countries using the M and N broadcast television system standards. Channel 37 occupies a band of UHF frequencies from 608 to 614 MHz, frequencies that are particularly important to radio astronomy because they allow observations at a frequency between the dedicated frequency allocations near 410 MHz and 1.4 GHz. One radio astronomy application in this band is for Very-long-baseline interferometry. In 1963, when there were very few stations in the UHF band, the US Federal Communications Commission (FCC) adopted a 10-year moratorium on any allocation of stations to Channel 37. A new ban on such stations took effect at the beginning of 1974, and was made permanent by a number of later FCC actions. As a result of this, and similar actions by the Canadian Radio-television and Telecommunications Commission, Channel 37 has never been used by any over-the-air television station in Canada or the United States.".
- Channel_37 wikiPageExternalLink ra_freqs.html.
- Channel_37 wikiPageExternalLink 4.
- Channel_37 wikiPageExternalLink tvq?chan=37&cha2=37&serv=&type=0&list=1&slon2=&size=9.
- Channel_37 wikiPageExternalLink Long_Term_Digital_TV_Frequency_Plan.pdf.
- Channel_37 wikiPageExternalLink 0,9171,830284,00.html.
- Channel_37 wikiPageExternalLink 216031.
- Channel_37 wikiPageExternalLink tvdbweir.htm.
- Channel_37 wikiPageID "4354277".
- Channel_37 wikiPageRevisionID "538646323".
- Channel_37 hasPhotoCollection Channel_37.
- Channel_37 subject Category:Broadcast_engineering.
- Channel_37 subject Category:Fictional_telecom_protocols.
- Channel_37 subject Category:History_of_television.
- Channel_37 subject Category:TV_stations_by_channel_number.
- Channel_37 comment "Channel 37 is an unused television channel in countries using the M and N broadcast television system standards. Channel 37 occupies a band of UHF frequencies from 608 to 614 MHz, frequencies that are particularly important to radio astronomy because they allow observations at a frequency between the dedicated frequency allocations near 410 MHz and 1.4 GHz. One radio astronomy application in this band is for Very-long-baseline interferometry.".
- Channel_37 label "Channel 37".
- Channel_37 sameAs m.0bysb7.
- Channel_37 sameAs Q5072296.
- Channel_37 sameAs Q5072296.
- Channel_37 wasDerivedFrom Channel_37?oldid=538646323.
- Channel_37 isPrimaryTopicOf Channel_37.