High-altitude nuclear explosion

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Hardtack Teak, 1958 Hardtack I Teak 002.jpg
Hardtack Teak, 1958
Frame of the Starfish Prime nuclear test Starfish prime 35mm frame.jpg
Frame of the Starfish Prime nuclear test

High-altitude nuclear explosions are the result of nuclear weapons testing within the upper layers of the Earth's atmosphere and in outer space. Several such tests were performed at high altitudes by the United States and the Soviet Union between 1958 and 1962.

Contents

The Partial Test Ban Treaty was passed in October 1963, ending atmospheric and exoatmospheric nuclear tests. The Outer Space Treaty of 1967 banned the stationing of nuclear weapons in space, in addition to other weapons of mass destruction. The Comprehensive Nuclear-Test-Ban Treaty of 1996 prohibits all nuclear testing; whether over- or underground, underwater or in the atmosphere.

EMP generation

The strong electromagnetic pulse (EMP) that results has several components. In the first few tenths of nanoseconds, about a tenth of a percent of the weapon yield appears as powerful gamma rays with energies of one to three mega-electron volts (MeV, a unit of energy). The gamma rays penetrate the atmosphere and collide with air molecules, depositing their energy to produce huge quantities of positive ions and recoil electrons (also known as Compton electrons). These collisions create MeV-energy Compton electrons that then accelerate and spiral along the Earth's magnetic field lines. The resulting transient electric fields and currents that arise generate electromagnetic emissions in the radio frequency range of 15 MHz to 250MHz. This high-altitude EMP occurs between 30 and 50 kilometers (19 and 31 miles) above the Earth's surface. The potential as an anti-satellite weapon became apparent in August 1958 during Hardtack Teak . The EMP observed at the Apia Observatory at Samoa was four times more powerful than any created by solar storms, [1] while in July 1962 the Starfish Prime test, damaged electronics in Honolulu and New Zealand (approximately 1,300 kilometres (810 mi) away), fused 300 street lights on Oahu (Hawaii), set off about 100 burglar alarms, and caused the failure of a microwave repeating station on Kauai, which cut off the sturdy telephone system from the other Hawaiian islands. The radius for an effective satellite kill for the various 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 a Department of Defense program, Program 437 .

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. EMP mechanism.png
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

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 an artificial radiation belt in space that soon destroyed three satellites (Ariel, TRAAC, and Transit 4B all failed after traversing the radiation belt, while Cosmos V, Injun I and Telstar 1 suffered minor degradation, due to some radiation damage to solar cells, etc.). The radiation dose rate was at least 0.6 Gy/day at four months after Starfish for a well-shielded satellite or crewed capsule in a polar circular earth orbit, which caused NASA concern with regard to its crewed space exploration programs.

Differences from atmospheric tests

Late phases of TEAK fireball and formation of Northern Branch of Aurora as viewed from aircraft flying northwest of explosion. HD.10.069 (10562002014).jpg
Late phases of TEAK 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 characteristic mushroom-shaped cloud, high-altitude and space explosions tend to manifest a spherical 'cloud,' reminiscent of other space-based explosions[ example needed ] until distorted by Earth's magnetic field. The charged particles resulting from the blast are accelerated along the Earth's magnetic field lines to create an auroral display at the conjugate point, [2] which has led documentary maker Peter Kuran to characterize these detonations as 'the rainbow 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 the Bluegill Triple Prime shot, at an altitude of 50 kilometers (31 miles), was felt by personnel on the ground at Johnston Atoll, and this test caused retina burns to two personnel at ground zero who were not wearing their safety goggles.

Soviet high-altitude tests

The Soviets detonated four high-altitude tests in 1961 and three in 1962. During the Cuban 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 the Soviet Project K nuclear tests (ABM System A proof tests) when a 300 kt missile-warhead detonated near Dzhezkazgan at 290-kilometre (180 mi) altitude. The EMP fused 570 kilometres (350 mi) of overhead telephone line with a measured current of 2,500  A , started a fire that burned down the Karaganda power plant, and shut down 1,000 kilometres (620 mi) of shallow-buried power cables between Tselinograd and Alma-Ata.

List of high-altitude nuclear explosions

Hardtack I Orange Hardtack I Orange 002.jpg
Hardtack I Orange
View of Starfish Prime through thin cloud, as seen from Honolulu, 1,300 km away. Starfish5.JPG
View of Starfish Prime through thin cloud, as seen from Honolulu, 1,300 km away.
The debris fireball and aurora created by the Starfish Prime test, as seen from a KC-135 aircraft at 3 minutes. Operation Dominic Starfish-Prime nuclear test from plane.jpg
The debris fireball and aurora created by the Starfish Prime test, as seen from a KC-135 aircraft at 3 minutes.
MissionDateYieldAltitude
Flag of the United States.svg  US Hardtack I – (Operation Newsreel) – Johnston Atoll, Pacific Ocean
Yucca28 April 19581.7 kt26.2 km
Teak 1 August 19583.8 Mt76.8 km
Orange12 August 19583.8 Mt34 km
Flag of the United States.svg  US Argus – South Atlantic Ocean
Argus I27 August 19581.7 kt200 km
Argus II30 August 19581.7 kt240 km
Argus III6 September 19581.7 kt540 km
Flag of the Soviet Union.svg  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
Flag of the United States.svg  US Dominic 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 9 July 19621.4 Mt400 km
Checkmate20 October 19627 kt147 km
Kingfish1 November 1962410 kt97 km
Tightrope4 November 1962<5 kt30–80 km
Flag of the Soviet Union.svg  Soviet Union Project 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

  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.

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