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High-altitude nuclear explosion

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Nuclear detonations in the upper layers of Earth's atmosphere
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Hardtack Teak, 1958
Frame of theStarfish Prime nuclear test

High-altitude nuclear explosions are the result ofnuclear weapons testing within the upper layers of theEarth's atmosphere and inouter space. Several such tests were performed at high altitudes by theUnited States and theSoviet Union between 1958 and 1962.

ThePartial Test Ban Treaty was passed in October 1963, ending atmospheric and exoatmospheric nuclear tests. TheOuter Space Treaty of 1967 banned the stationing of nuclear weapons in space, in addition to otherweapons of mass destruction. TheComprehensive Nuclear-Test-Ban Treaty of 1996 prohibits all nuclear testing; whether over- or underground, underwater or in the atmosphere, but has yet to enter into force as it has not been ratified by some of the states party to the Treaty.

EMP generation

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The strongelectromagnetic pulse (EMP) that results has several components. In the first few tenths of nanoseconds, about a tenth of a percent of the weaponyield appears as powerfulgamma rays with energies of one to threemega-electron volts (MeV, a unit of energy). The gamma rays penetrate the atmosphere and collide withair molecules, depositing their energy to produce huge quantities of positiveions andrecoil electrons (also known asCompton electrons). These MeV-energy Compton electrons then accelerate and spiral along the Earth's magnetic field lines. The resulting transient electric fields and currents generateelectromagnetic emissions in theradio frequency range of15MHz to250MHz. This high-altitude EMP occurs between 30 and 50 kilometers (19 and 31 miles) above the Earth's surface.The potential as ananti-satellite weapon became apparent in August 1958 duringHardtack Teak. The EMP observed at theApia Observatory atSamoa was four times more powerful than any created bysolar storms,[1] while in July 1962 theStarfish Prime test damaged electronics inHonolulu andNew Zealand (approximately 1,300 kilometres (810 mi) away), fused 300 street lights onOahu (Hawaii), set off about 100burglar alarms, and caused the failure of amicrowaverepeating station onKauai, which cut off the sturdy telephone system from the other Hawaiian islands. The radius for an effective satellite kill for the Compton radiation produced by such a nuclear weapon in space was determined to be roughly 80 kilometres (50 mi). Further testing to this end was carried out, and embodied in aDepartment of Defense program,Program 437.[citation needed]

The mechanism for a 400 kilometres (250 mi) high-altitude burst EMP: gamma rays hit the atmosphere between 20 and 40 kilometres (12 and 25 mi) altitude, ejecting electrons which are then deflected sideways by the Earth's magnetic field

Drawbacks

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There are problems with nuclear weapons carried over to testing and deployment scenarios, however. Because of the very large radius associated with nuclear events, it was nearly impossible to prevent indiscriminate damage to other satellites, including one's own satellites.Starfish Prime produced anartificial radiation belt in space that soon destroyed three satellites (Ariel,TRAAC, andTransit 4B all failed after traversing the radiation belt, whileCosmos V,Injun I andTelstar 1 suffered minor degradation, due to someradiation damage tosolar cells, etc.). Theradiation dose rate was at least 0.6Gy/day at four months afterStarfish for a well-shielded satellite or crewed capsule in apolar circular earth orbit, which caused NASA concern with regard to its crewed space exploration programs.[citation needed]

Differences from atmospheric tests

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Late phases ofTEAK fireball and formation of Northern Branch of Aurora as viewed from aircraft flying northwest of explosion.

In general, nuclear effects in space (or very high altitudes) have a qualitatively different display. While an atmospheric nuclear explosion has a characteristicmushroom-shaped cloud, high-altitude and space explosions tend to manifest a spherical 'cloud' until distorted byEarth's magnetic field. Thecharged particles resulting from the blast are accelerated along the Earth's magnetic field lines to create anauroral display at theconjugate point,[2] which has led documentary makerPeter Kuran to characterize these detonations as 'therainbow bombs'. The visual effects of a high-altitude or space-based explosion may last longer than atmospheric tests, sometimes in excess of 30 minutes. Heat from theBluegill Triple Prime shot, at an altitude of 50 kilometers (31 miles), was felt by personnel on the ground atJohnston Atoll, and this test causedretina burns to two personnel atground zero who were not wearing their safety goggles.[citation needed]

Soviet high-altitude tests

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The Soviets detonated four high-altitude tests in 1961 and three in 1962. During theCuban Missile Crisis in October 1962, both the US and the USSR detonated several high-altitude nuclear explosions as a form of saber rattling.

The worst effects of a Soviet high-altitude test occurred on 22 October 1962, in theSoviet Project K nuclear tests (ABM System A proof tests) when a 300 kt missile-warhead detonated nearDzhezkazgan at 290-kilometre (180 mi) altitude. The EMP fused 570 kilometres (350 mi) of overhead telephone line with a measured current of2,500 A, started a fire that burned down theKaraganda power plant, and shut down 1,000 kilometres (620 mi) of shallow-buriedpower cables betweenTselinograd andAlma-Ata.[citation needed]

List of high-altitude nuclear explosions

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See also:List of artificial radiation belts
Hardtack I Orange
View ofStarfish Prime through thin cloud, as seen fromHonolulu, 1,300 km away.
The debris fireball and aurora created by theStarfish Prime test, as seen from a KC-135 aircraft at 3 minutes.
MissionDateYieldAltitude
USHardtack I – (Operation Newsreel) –Johnston Atoll, Pacific Ocean
Yucca28 April 19581.7 kt26.2 km
Teak1 August 19583.8 Mt76.8 km
Orange12 August 19583.8 Mt34 km
USArgus – South Atlantic Ocean
Argus I27 August 19581.7 kt200 km
Argus II30 August 19581.7 kt240 km
Argus III6 September 19581.7 kt540 km
Soviet Union – 1961 tests –Kapustin Yar
Test #886 September 196110.5 kt22.7 km
Test #1156 October 196140 kt41.3 km
Test #12727 October 19611.2 kt150 km
Test #12827 October 19611.2 kt300 km
USDominic I – (Operation Fishbowl) – Johnston Atoll, Pacific Ocean
Bluegill3 June 1962failed
Bluegill Prime25 July 1962failed
Bluegill Double Prime15 October 1962failed
Bluegill Triple Prime26 October 1962410 kt50 km
Starfish20 June 1962failed
Starfish Prime[3]9 July 19621.4 Mt400 km
Checkmate20 October 19627 kt147 km
Kingfish1 November 1962410 kt97 km
Tightrope4 November 1962<5 kt30–80 km
Soviet UnionProject K – Kapustin Yar
Test #18422 October 1962300 kt290 km
Test #18728 October 1962300 kt150 km
Test #1951 November 1962300 kt59 km

See also

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References

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  1. ^Tinsley, B. A. (December 1962)."Riometer observations of HF noise at Samoa following high-altitude nuclear test".New Zealand Journal of Geology and Geophysics.5 (6):964–968.doi:10.1080/00288306.1962.10420048.ISSN 0028-8306.
  2. ^Keys, J. G. (1964-10-01)."Artificial aurorae from high-altitude nuclear tests".Journal of Atmospheric and Terrestrial Physics.26 (10):979–993.doi:10.1016/0021-9169(64)90173-4.ISSN 0021-9169.
  3. ^Vittitoe, Charles N. (June 1, 1989).Did High-Altitude EMP Cause the Hawaiian Streetlight Incident?(PDF) (Report).Sandia National Laboratories.Archived(PDF) from the original on August 23, 2020. RetrievedSeptember 15, 2020.

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