||The examples and perspective in this article deal primarily with the United States and do not represent a worldwide view of the subject. (December 2010)|
Just above the mediumwave broadcast band, 160 meters refers to the band of radio frequencies between 1800 to 2000 kHz, which is the lowest radio frequency band allocated for use by amateur radio in most countries. Older amateur operators often refer to 160 meters as the Top Band. It is also sometimes referred to as the "Gentleman's Band" in contrast to the often-freewheeling 80- and 20-meter band activity.
The 160 meter band is the oldest amateur band and was the staple of reliable communication in the earliest days of amateur radio, when almost all communications were over relatively short distances. The band was allocated on a worldwide basis by the International Radiotelegraph Conference in Washington, D.C., on October 4, 1927. The allocation was 1715–2000 kHz. The International Radio Conference of Atlantic City reduced the allocation to 1800–2000 kHz under the provision that amateurs must not interfere with LORAN operation.
As the high frequency bands were developed in mid-1920s — along with their smaller, more convenient antennas — 160 meters fell into a period of relative nonuse. Although there has always been activity on the band, fewer and fewer hams are willing (or able, due to lack of sufficient real estate) to put up the antennas necessary to take advantage of the band's unique properties. For most amateurs, the HF bands are much easier to use and HF antennas need a lot less real estate.
After World War II, the 160 meter band was apparently not coming back. A large part of the U.S. 160 meter band was allocated on a primary basis to the LORAN radio-navigation system that began operating in and around the 160 meter band in 1942. Amateurs were relegated to secondary, non-interfering status, with severe regional power limitations and restricted day/night operations on just a few narrow segments of the band.
Many older hams recall, with no great fondness, the ear-shattering buzz-saw racket of high power LORAN stations that began in 1942 until LORAN-A was phased out in North America on December 31, 1980 and most of the world by 1985. LORAN-A was still operating in China and Japan in 1995.
Great ingenuity was used to eliminate the pulse noise of the powerful LORAN-A transmitters through such famous circuitry as the "Select-O-Ject" of the late 1950s. The technology was adapted to modern noise blanking circuits used in current amateur receivers and transceivers.
Despite many obstacles and threats from commercial and military spectrum users, the efforts of a small number of determined 160 meter operators enabled the band to survive. In the UK it was the primary band for mobile operation for many years. The band experienced a rebirth with the demise of LORAN-A in the United States in December, 1980 and the removal of power restrictions below 1900 kHz soon thereafter. Power restrictions above 1900 kHz were removed in March 1984. 160 meters was then no longer regarded as the "orphan" band as it had been for more than half a century.
Effective 160 meter operation can be particularly challenging, as full sized antennas (on the order of a quarter-wavelength or more) are difficult to erect for many amateurs with limited space. Nevertheless, many radio amateurs successfully communicate over very long distances with relatively small antennas. 160 meters is populated by many highly dedicated experimenters, as it is a proving ground for ingenuity in antenna design and operating technique.
Propagation is limited to local contacts during the day, but DX contacts are possible at night, especially around sunrise and sunset and during periods of sunspot minima. Much about ionospheric and propagation on 160 meters is still not completely understood. Phenomena such as "chordal hop" propagation are frequently observed, as well as other unexplained long-distance propagation mechanisms. Inexplicable radio blackouts — sometimes encountered on the AM broadcast band — also occur on 160 meters. Many of these phenomena have been investigated in the scientific community also. The original "magic of radio" is very much alive and well on 160 meters.
The International Telecommunication Union allocated the frequencies from 1810 - 2000 kHz to amateur radio operations in ITU Region 1 (Europe, Greenland, Africa, the Middle East west of the Persian Gulf and including Iraq, the former Soviet Union and Mongolia) and 1800 - 2000 kHz in the rest of the world.
- "ARRLWeb: US Amateur Bands" (PDF). Archived from the original on 10 September 2005. Retrieved August 3, 2005.
- "ARRLWeb: ARRL Band Plans". Archived from the original on 3 August 2005. Retrieved August 3, 2005.
- "RAC Web: Canada HF Band Plan" (PDF). Retrieved July 8, 2008.
- "Ham Radio QRP". Retrieved August 3, 2005.
- "UK Amateur Radio Band Plans". Retrieved February 3, 2010. Click the 160 Meter button at the bottom of the page
- "ITU Frequency Allocations: HF Amateur Bands". Retrieved January 1, 2008.
- "IARU Region 1 Bandplan" (PDF). Retrieved July 31, 2013.
- "IARU Region 2 Bandplan" (PDF). Retrieved January 1, 2008.
- "IARU Region 3 Bandplan" (PDF). Retrieved October 16, 2009.
- "Japan Bandplan" (PDF). Retrieved March 30, 2009.
- "NZ4O 160 Meter Propagation Theory Notes". A website dedicated to layman level explanations of "seemingly" mysterious 160 Meter (MF) propagation occurrences. Retrieved 17 August 2009.
|International amateur radio frequency allocations|
|Range||Band||ITU Region 1||ITU Region 2||ITU Region 3|
|LF||2200 m||135.7 kHz - 137.8 kHz|
|MF||600 m||472 kHz - 479 kHz|
|160 m||1.810 MHz - 1.850 MHz||1.800 MHz - 2.000 MHz|
|HF||80 / 75 m||3.500 MHz - 3.800 MHz||3.500 MHz - 4.000 MHz||3.500 MHz - 3.900 MHz|
|60 m1||5.250 MHz - 5.450 MHz|
|40 m||7.000 MHz - 7.200 MHz||7.000 MHz - 7.300 MHz||7.000 MHz - 7.200 MHz|
|30 m2||10.100 MHz - 10.150 MHz|
|20 m||14.000 MHz - 14.350 MHz|
|17 m2||18.068 MHz - 18.168 MHz|
|15 m||21.000 MHz - 21.450 MHz|
|12 m2||24.890 MHz - 24.990 MHz|
|10 m||28.000 MHz - 29.700 MHz|
|VHF||6 m||50.000 MHz - 52.000 MHz1||50.000 MHz - 54.000 MHz|
|4 m1||70.000 MHz - 70.500 MHz|
|2 m||144.000 MHz - 146.000 MHz||144.000 MHz - 148.000 MHz|
|1.25 m||220.000 MHz - 225.000 MHz|
|UHF||70 cm||430.000 MHz - 440.000 MHz||430.000 - 440.000 MHz
(420.000 - 450.000 MHz)3
|33 cm||902.000 MHz - 928.000 MHz|
|23 cm||1.240 GHz - 1.300 GHz|
|13 cm||2.300 GHz - 2.450 GHz|
|SHF||9 cm||3.400 GHz - 3.475 GHz3||3.300 GHz - 3.500 GHz|
|5 cm||5.650 GHz - 5.850 GHz||5.650 GHz - 5.925 GHz||5.650 GHz - 5.850 GHz|
|3 cm||10.000 GHz - 10.500 GHz|
|1.2 cm||24.000 GHz - 24.250 GHz|
|EHF||6 mm||47.000 GHz - 47.200 GHz|
|4 mm3||75.500 GHz1 - 81.500 GHz||76.000 GHz - 81.500 GHz|
|2.5 mm||122.250 GHz - 123.000 GHz|
|2 mm||134.000 GHz - 141.000 GHz|
|1 mm||241.000 GHz - 250.000 GHz|
|THF||Sub-mm||Some administrations have authorized spectrum for amateur use in this region.|
1 This is not mentioned in the ITU's Table of Frequency Allocations, but individual administrations may make allocations under Article 4.4 of the ITU Radio Regulations. See the appropriate Wiki page for further information.
|See also: Radio spectrum · Electromagnetic spectrum|