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Amateur radio frequency allocation is done by national telecommunication authorities. Globally, theInternational Telecommunication Union (ITU) oversees how muchradio spectrum is set aside foramateur radio transmissions. Individual amateur stations are free to use any frequency within authorized frequency ranges; authorized bands may vary by the class of the station license.

Radio amateurs use a variety of transmission modes, includingMorse code,radioteletype, data, and voice. Specificfrequency allocations vary from country to country and betweenITU regions as specified in the current ITU HF frequency allocations for amateur radio.^[1] The list of frequency ranges is called aband allocation, which may be set by international agreements, and national regulations. The modes and types of allocations within each frequency band is called abandplan; it may be determined by regulation, but most typically is set by agreements between amateur radio operators.

National authorities regulate amateur usage of radio bands. Some bands may not be available or may have restrictions on usage in certain countries or regions. International agreements assign amateur radio bands which differ by region.^[2][3]

• 2200 metres – 135.7–137.8 kHz

Just below theAsian and Europeanlongwave broadcast band andfar below thecommercial AM broadcast band.

• 630 metres – 472–479 kHz

Justbelow thecommercial AM broadcast band and themaritime radio band.

• 160 metres –1 800–2 000 kHz (1.800–2.000 MHz)

Justabove thecommercial AM broadcast band. Allocations in this band vary widely from country to country; it was formerly shared with the largely defunctLoran-A radionavigation system.

This band is often taken up as a technical challenge, since long distance (DX) propagation tends to be more difficult due to higherD layer ionospheric absorption. Long-distance propagation tends to occur only at night, and the band can be notoriously noisy particularly in the summer months.

160 metres is also known as the"top band". For many years it was the longest-wavelength amateur band; although often included among theshortwaves, it is actually located near the top end of themedium frequency band.

Most of the customary band names given below are onlynominal wavelengths, notactual wavelengths. For example:

• In the western hemisphere the nominal 80 m band actually ranges between about 85.7–74.9 m, and the international portion from 85.7–83.3 m.
• The nominal "17 m" band actually covers 16.6–16.5 m.
• The nominal "15 m" band actually ranges from 14.28–13.98 m. By common sense, the "15 m" band ought to be called "14 m", but that name has been in longtime use for ashortwave broadcast band.

• 80 metres or80 / 75 meters –3 500–4 000 kHz – 85.65–74.95 m actual

Best at night, with significant daytime signal absorption. Works best in winter, due to atmospheric noise from hemispheric thunder storms during summer. Only countries in the Americas and few others have access to all of this band; in other parts of the world amateurs are limited to the bottom 300 kHz (or less) (85.65–83.28 m).

In the US and Canada the portion of the band from 3.600–4.000 MHz, regulation permits use of single-sideband voice as well asAM voice; this sub-band is often referred to as "the 75 metre band", in part to distinguish it from the internationally available frequencies below it.

• 60 metres – 5 MHz region – around 56 m

A relatively new allocation and originally only available in a small number of countries such as the United States,United Kingdom,Ireland,Norway,Denmark, andIceland, but now continuing to expand. In most (but not all) countries, the allocation is broken into channels and may require a special licensing request.

Five 2.8 kHz-wide channels are available in the U.S., centered on 5.332, 5.348, 5.368, 5.373, and 5.405 MHz. Since most radios inSSB mode display the (suppressed) carrier frequency, inUSB mode the dial frequencies would all need to be set 1.5 kHzlower. Voice operation is generally inupper sideband mode, which is mandatory in the U.S. . The U.S. and Canada allow 100 Watts in the currently available channels.

The 2015ITUWorld Radiocommunication Conference (WRC-15) approved a new worldwide frequency allocation of 5.351.5–5.366.5 MHz to the amateurs on a secondary basis. The allocation limits amateur stations to 15 wattseffective isotropic radiated power (EIRP); however some locations will be permit up to 25 WEIRP.

• 40 metres – 7.000–7.300 MHz – 42.83–41.51 m actual

Considered the most reliable all-season long distance (DX) band. Popular for DX at night, 40 metres is also reliable for medium distance (1,500 km / 1,000 miles) contacts during the day. Much of this band was shared with broadcasters, and in most countries the bottom 100 kHz or 200 kHz are available to amateurs. However, due to the high cost of running high-power commercial broadcasting facilities, decreased listenership, and increasing competition from Internet-based international broadcast services, manyshortwave broadcasting services are being shut down, leaving the 40 metre band free of other users for amateur radio use.

• 30 metres – 10.100–10.150 MHz – 29.68–29.54 m actual

A very narrow band, which is shared with non-amateur services. It is recommended that onlyMorse code and data transmissions be used here, and in some countries amateur voice transmission is actually prohibited.

For example, in the US, data,RTTY, andCW are the only modes allowed at a maximum 200 Wpeak envelope power (PEP) output. Not released for amateur use in a small number of countries.

Due to its location in the centre of the shortwave spectrum, this band provides significant opportunities for long-distance communication at all points of the solar cycle. 30 metres is aWARC band. "WARC" bands are so called due to the 1979 specialWorld Administrative Radio Conference allocation of these newer bands to amateur radio use. Amateur radio contests are not run on the WARC bands.

• 20 metres – 14.000–14.350 MHz – 21.41–20.89 m actual

Considered the most popularDX band; usually most popular during daytime.QRP operators recognize 14.060 MHz as their primary calling frequency within the band. Users of thePSK31 data mode tend to congregate around 14.070 MHz. AnalogSSTV activity centers on 14.230 MHz.

• 17 metres – 18.068–18.168 MHz – 16.6–16.5 m actual

Similar to 20 metres, but more sensitive to solar propagation minima and maxima. 17 metres is aWARC band.

• 15 metres – 21.000–21.450 MHz – 14.28–13.98 m actual

Most useful during solar maximum, and generally a daytime band. Daytimesporadic E propagation (1,500 km / 1,000 miles) occasionally occurs on this band.

• 12 metres – 24.890–24.990 MHz – 12.04–12.00 m actual

Mostly useful during daytime, but opens up forDX activity at night, during solar maximum. 12 metres is one of theWARC bands. Propagates viasporadic E and byF2 propagation.

• 10 metres – 28.000–29.700 MHz – 10.71–10.08 m actual

Best long distance (e.g., across oceans) activity is duringsolar maximum; during periods of moderate solar activity the best activity is found at low latitudes. The band offers useful short to medium rangegroundwave propagation, day or night.

Due toSporadic E propagation during the late spring and most of the summer, regardless of sunspot numbers, afternoon short band openings into small geographic areas of up to 1,500 km (1,000 miles) occur.Sporadic E is caused by areas of intense ionization in the E layer of the ionosphere. The causes of sporadic E are not fully understood, but these "clouds" of ionization can provide short-term propagation from 17 metres all the way up to occasional 2 metre openings. FM operations are normally found at the high end of the band (Also repeaters are in the 29.500–29.700 MHz segment in many countries).

Frequencies above 30 MHz are referred to asVery High Frequency (VHF) region and those above 300 MHz are calledUltra High Frequency (UHF). The allocated bands for amateurs are manymegahertz wide, allowing for high-fidelity audio transmission modes (FM) and very fast data transmission modes that are unfeasible for thekilohertz-wide allocations in theHF bands.

VHF
8 metres	40–45 MHz	in parts of ITU Region 1
6 metres	50–54 MHz
	50–52 MHz	In parts of ITU Region 1
5 metres	58.0–60.1 MHz	in parts of ITU Region 1
4 metres	70–70.5 MHz	in parts of ITU Region 1
2 metres	144–148 MHz
	144–146 MHz	ITU Region 1
1.25 metres	219–220 MHz	Fixed digital message forwarding systems
	222–225 MHz	US & Canada
UHF
70 centimetres	420–450 MHz
	430–440 MHz	in ITU Region 1
33 centimetres	902–928 MHz	in ITU Region 2
23 centimetres	1 240–1 300 MHz
	1 240–1 325 MHz	in UK
13 centimetres	2 300–2 310 MHz	lower segment
	2 390–2 450 MHz	upper segment

While"line of sight" propagation is a primary factor for range calculation, much of the interest in the bands above HF comes from use of other propagation modes. A signal transmitted on VHF from a hand-held portable will typically travel about5–10 km (3–6 miles) depending on terrain. With a low power home station and a simple antenna, range would be around50 km (30 miles).

With a large antenna system like a longyagi, and higher power (typically 100 watts or more) contacts of around1 000 km (600 miles) using the Morse code (CW) and single-sideband (SSB) modes are common. Ham operators seek to exploit the limits of the frequencies usual characteristics looking to learn, understand, and experiment with the possibilities of these enhanced propagation modes.

Occasionally, several different ionospheric conditions allow signals to travel beyond the ordinary line-of-sight limits. Some amateurs on VHF seek to take advantage of "band openings" where natural occurrences in the atmosphere and ionosphere extend radio transmission distances well over their normal range. Many hams listen for hours hoping to take advantage of these occasional extended propagation "openings".

The ionospheric conditions are calledsporadic E andanomalous enhancement. Less frequently used anomalous modes aretropospheric scatter andAurora Borealis (Northern Lights).Moon bounce andsatellite relay are also possible.

Some openings are caused by islands of intense ionization of the upper atmosphere, known as the E Layerionosphere. These islands of intense ionization are called "sporadic E" and result in erratic but often strong propagation characteristics on the "low[er] band" VHF radio frequencies.

The 6 metre amateur band falls into this category, often called "the magic band", will often "open up" from one small area into another small geographic area1 000–1 700 km(600–1 000 miles) away during the spring and early summer months. This phenomenon occurs during the fall months, although not as often.

Band openings are sometimes caused by aweather phenomenon known as atropospheric "inversion", where a stagnant high pressure area causes alternating stratified layers of warm and cold air generally trapping the colder air beneath. This may make for smoggy or foggy days, but it also causes VHF and UHF radio transmissions to travel or duct along the boundaries of these warm/cold atmospheric layers. Radio signals have been known to travel hundreds, even thousands of kilometres (miles) due to these unique weather conditions.

For example: The longest distance reported contact due to tropospheric refraction on 2 metres is4 754 km(2 954 miles) betweenHawaii and a ship south ofMexico. There were reports of the reception of one way signals fromRéunion toWestern Australia, a distance of more than6 000 km(4 000 miles).^[4]

Tropo-scatter happens when water droplets and dust particles refract a VHF or UHF signal over the horizon. Using relatively high power and a high gain antenna, this propagation will give marginal enhanced over-the-horizon VHF and UHF communications up to several hundred kilometres (miles). During the 1970s commercial "scatter site" operators using huge parabolic antennas and high power used this mode successfully for telephone communications services into northern remote Alaska and Canadian communities.

Satellite, buried fibre optic, and terrestrial microwave access have relegated commercial use of tropo-scatter to the history books. Because of high cost and complexity this mode is usually out of reach for the average amateur radio operator.

F2 and TE band openings from other ionospheric reflection/refraction modes, orsky-wave propagation as it is known can also occasionally occur on the low band VHF frequencies of 6 or 4 metres, and very rarely on 2 metres (high band VHF) during extreme peaks in the 11 year sunspot cycle.

The longest terrestrial contact ever reported on 2 metres (146 MHz) was between a station in Italy and a station in South Africa, a distance of 7 784 km (4 837 miles), using trans-equatorial anomalous enhancement (TE) of the ionosphere over the geomagnetic equator. This enhancement is known as TE, or trans-equatorial propagation and (usually) occurs at latitudes 2 500–3 000 km (1500–1900 miles) within either side of the equator.^[5]

An intense solar storm causing aurora borealis (northern lights) will also provide occasionalpropagation enhancement to HF-low (6-metre) band radio waves. Aurorae only occasionally affect signals on the2 metre band. Signals are often distorted and on the lower frequencies give a curious "watery sound" to normally propagated HF signals. Peak signals usually come from the north, even if the signal originates from a station to the east or west of the receiver. This effect is most significant in the latitudes north of 45 degrees.

Amateurs do successfully communicate by bouncing their signals off the surface of the Moon, calledEarth-Moon-Earth (EME) transmission.

The mode requires moderately high power (more than 500 watts) and a fairly large,high-gain antenna because round-trip path loss is on the order of 270 dB for 70 cm signals. Return signals are weak and distorted because of the relative velocities of the transmitting station, Moon and the receiving station. The Moon's surface is also very rocky and irregular.

Because of the weak, distorted return signals,Moon bounce communications use digital modes. For example, old-fashionedMorse code or modernJT65, designed for working with weak signals.

Satellite relay is not really a propagation mode, but rather an active repeater system. Satellites have been highly successful in providing VHF/UHF/SHF users "propagation" beyond the horizon.

Amateurs have sponsored the launch of dozens of communications satellites since the 1970s. These satellites are usually known asOSCARs (Orbiting Satellite Carrying Amateur Radio). Also, theISS has amateur radio repeaters and radio location services on board.

Amateur television (ATV) is thehobby of transmittingbroadcast-compatiblevideo andaudio by amateur radio. It also includes the study and building of suchtransmitters andreceivers and thepropagation between these two.

InNTSC countries, ATV operation requires the ability to use a 6 MHz wide channel. All bands atVHF or lower are less than 6 MHz wide, so ATV operation is confined toUHF and up. Bandwidth requirements will vary from this forPAL andSECAM transmissions.

ATV operation in the 70 cm band is particularly popular, because the signals can be received on any cable-ready television. Operation in the 33 cm and 23 cm bands is easily augmented by the availability of various varieties of consumer-grade wireless video devices that exist and operate in unlicensed frequencies coincident to these bands.

Repeater ATV operation requires specially-equipped repeaters.

Historically, amateur stations have rarely been allowed to operate on frequencies lower than themedium-wavebroadcast band, but in recent times, as the historic users of these low frequencies have been vacating the spectrum, limited space has opened up to allow for new amateur radio allocations and special experimental operations.

Since parts of the 500 kHz band are no longer used for regular maritime communications,^{[citation needed]} some countries permit amateur radio radiotelegraph operations in that band. Many countries, however, continue to restrict these frequencies which were historically reserved for maritime and aviation distress calls.^[6]

The2 200 metre band is available for use in several countries, and the 2007World Radiocommunication Conference (WRC-07) recommended it as a worldwide amateur allocation. Before the introduction of the2 200 metre band in the U.K. in 1998, operation on the even lower frequency of 73 kHz, in the LFtime signal band, was allowed from 1996–2003.

ITU Region 1 corresponds to Europe, Russia, Africa and the Middle East. For ITU region 1,Radio Society of Great Britain'sband plan will be more definitive (click on the buttons at the bottom of the page).

• Low Frequency (LF) (30 to 300 kHz)
  • 2200 metres (135.7 to 137.8 kHz)
• Medium Frequency (MF) (0.3 to 3 MHz)
  • 630 metres (472 to 479 kHz)
• High Frequency (HF) (3 to 30 MHz)
  • see Table of amateur MF and HF bandplans
• Very High Frequency (VHF) (30 to 300 MHz)
  • 8 metres (39.9 to 40.7 MHz), Republic of Ireland, Slovenia and South Africa. Beacons in UK and Denmark
  • 6 metres (50 to 52/54 MHz)
  • 5 metres (59.5 to 60.1 MHz), Republic of Ireland. The Beacon in UK
  • 4 metres (69.9 to 70.5 MHz), Some ITU Region 1 countries
  • 2 metres (144 to 146 MHz)
• Ultra High Frequency (UHF) (300 MHz to 3 GHz)
  • 70 cm (430 MHz)
  • 23 cm (1.3 GHz)
  • 13 cm (2.3 GHz)
• Microwave frequencies
  • 9 cm (3.4 GHz)
  • 6 cm (5.7 GHz)
  • 3 cm (10 GHz)
  • 12 mm (24 GHz)
  • 6 mm (47 GHz)
  • 4mm (76 GHz)
  • <2 mm (134 and 247 GHz)

The following charts show the voluntary bandplans used by amateurs in ITU Region 1. Unlike the US, slots for the various transmission modes are not set by the amateur's license but most users do follow these guidelines.

ITU Region 2 consists of the Americas, including Greenland.

The frequency allocations for hams in ITU Region 2 are:

(ARRL 60 meter operations[1])

The primary (first priority) user of thechannelled 60 meter band is the U.S.National Telecommunications and Information Administration (NTIA). Effective 5 March 2012 the FCC permits CW, USB, and certain digital modes on these frequencies by amateurs on a secondary basis.

The FCC Report and Order permits the use of digital modes that comply withemission designator “60H0J2B”, which includesPSK31 as well as anyRTTY signal with a bandwidth of less than 60 Hz. The Report and Order also allows the use of modes that comply with emission designator “2K80J2D”, which includes any digital mode with a bandwidth of 2.8 kHz or less whose technical characteristics have been documented publicly, per Part 97.309(4) of the FCC Rules. Such modes would includePACTOR I, II, or III, 300 baud packet,MFSK,MT63,Contestia,Olivia, DominoEX, and others.

On60 meters, hams are restricted to only one signal per channel, and automatic operation is not permitted. In addition, the FCC continues to require that all digital transmissions be centred on the channel-centre frequencies, which the Report and Order defines as being 1.5 kHz above the suppressedcarrier frequency of a transceiver operated in the upper side-band (USB) mode. As amateur radio equipment displays the carrier frequency, it is important for operators to understand correct frequency calculations for digital "sound-card" modes to ensure compliance with the channel-center requirement.

TheARRL has a"detailed band plan" for US hams showing allocations within each band.

RAC has a"chart showing the frequencies available to amateurs in Canada". 21 June 2017.

160 m	1800 – 2000
Canada
United States	1800 – 2000
General, Advanced, Extra

80 / 75 m	3500 – 4000
Canada
United States	3500 – 3525	3525 – 3600	3600 – 3700	3700 – 3800	3800 – 4000
Novice / Technician
General
Advanced
Extra

60 m	5330 – 5406
Canada	5332.0		5348.0		5358.5		5373.0		5405.0
United States	5332.0		5348.0		5358.5		5373.0		5405.0
General, Advanced, Extra
Basic (hon.), Code, Adv.
Note: US licensees operating 60 m are limited to 100 watts PEP ERP relative to a 1/2 wave dipole. Canadian operators are restricted to 100 watts PEP.[8]

40 m	7000 – 7300
Canada
United States	7000 – 7025	7025 – 7125	7125 – 7175	7175 – 7300
Novice / Technician
General
Advanced
Extra

30 m	10100-10150
Canada
United States
Note: US limited to General, Advanced and Extra licensees; 200 watts PEP

20 m	14000 – 14350
Canada
United States	14000-14025	14025-14150	14150-14175	14175-14225	14225-14350
General
Advanced
Extra

17 m	18068 – 18168
Canada
United States	18068 – 18110	18110 – 18168
General, Advanced, Extra

15 m	21000 – 21450
Canada
United States	21000 – 21025	21025 – 21200	21200 – 21225	21225 – 21275	21275 – 21450
Novice / Technician
General
Advanced
Extra

12 m	24890 – 24990
Canada
United States	24890 – 24930	24930 – 24990
General, Advanced, Extra

10 m	28000 – 29700
Canada
United States	28000 – 28300	28300 – 28500	28500 – 29700
Novice / Technician
General, Advanced, Extra
Note: The 10 metre table is one-third scale, relative to the other tables

ITU region 3 consists of Australia, Indonesia, Japan, New Zealand, the South Pacific, and Asia south of Siberia. The IARU frequency allocations for hams in ITU Region 3^[9] are:

Bands above 1300 MHz: societies should consult with the amateur satellite community for proposed satellite operating frequencies before deciding local bandplans above 1300 MHz.

Not all Member Unions follow this plan. As an example, the ACMA does not allow Australian Amateurs to use 3.700 MHz to 3.768 MHz and 3.800 MHz to 3.900 MHz, allocating this region to Emergency and Ambulatory services (Allocations can be found conducting a search of the ACMA Radcomms register[2]. )

The Wireless Institute of Australia hascharts for Amateur frequencies for Australia.

The New Zealand Association of Radio Transmitters (NZART) hascharts for Amateur frequencies for New Zealand.

The Japanese have charts for Amateur frequencies in Japan^[10]

Radio amateurs may engage insatellite andspace craft communications; however, the frequencies allowed for such activities are allocated separately from more general use radio amateur bands.

Under theInternational Telecommunication Union's rules, all amateur radio operations may only occur within 50 kilometres (31 mi) of the Earth's surface. As such, theAmateur Radio Service is not permitted to engage in satellite operations; however, a sister radio service, called theAmateur Satellite Service, exists which allows satellite operations for the same purposes as theAmateur Radio Service.

In most countries, an amateur radio license conveys operating privileges in both services, and in practice, the legal distinction between the two services is transparent to the average licensee. The primary reason the two services are separate is to limit the frequencies available for satellite operations. Due to the shared nature of the amateur radio allocations internationally, and the nature of satellites to roam worldwide, the ITU does not consider all amateur radio bands appropriate for satellite operations. Being separate from theAmateur Radio Service, theAmateur Satellite Service receives its own frequency allocations. All the allocations are within amateur radio bands, and with one exception, the allocations are the same in all threeITU regions.

Some of the allocations are limited by the ITU in what direction transmissions may be sent (EG: "Earth-to-space" or up-links only). All amateur satellite operations occur within the allocations tabled below, except forAO-7, which has an up-link from 432.125 MHz to 432.175 MHz.

• List of amateur radio frequency bands in India

• Amateur radio bands

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