Bhangmeter

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A bhangmeter is a non-imaging radiometer installed on reconnaissance and navigation satellites to detect atmospheric nuclear detonations and determine the yield of the nuclear weapon.[1]

History[edit]

The bhangmeter was invented, and the first proof-of-concept device was built, in 1948 to measure the nuclear test detonations of Operation Sandstone. Prototype and production instruments were later built by EG&G, and the name “bhangmeter” was coined in 1950.[2] Bhangmeters became standard instruments used to observe US nuclear tests. A Mod II bhangmeter was developed to observe the detonations of Operation Buster-Jangle (1951) and Operation Tumbler-Snapper (1952).[3]

US president John F. Kennedy and the First Secretary of the Communist Party of the Soviet Union Nikita Khrushchev signed the Partial Test Ban Treaty on August 5, 1963,[4] under the condition that each party could use its own technical means to monitor the ban on nuclear testing in the atmosphere or in outer space.[5]

Bhangmeters were first installed, in 1961, aboard a modified US KC-135A aircraft monitoring the pre-announced Soviet test of Tsar Bomba.[6]

The Vela satellites were the first space-based observation devices jointly developed by the U.S. Air Force and the Atomic Energy Commission. The first generation of Vela satellites were not equipped with bhangmeters but with X-ray sensors to detect the intense single pulse of X-rays produced by a nuclear explosion.[7] The first satellites which incorporated bhangmeters were the Advanced Vela satellites.

Since 1980 bhangmeters are part of US GPS navigation satellites.[8][9][10]

Description[edit]

The silicon photodiode sensors are designed to detect the distinctive bright double pulse of visible light that is emitted from atmospheric nuclear weapons explosions. This signature consists of a short and intense flash lasting around 1 millisecond, followed by a second much more prolonged and less intense emission of light taking a fraction of a second to several seconds to build up.[11] This signature, with a double intensity maximum, is characteristic of atmospheric nuclear explosions and is the result of the Earth atmosphere becoming opaque to visible light and transparent again as the explosion's shock wave travels through it.[9]

The effect occurs because the surface of the early fireball is quickly overtaken by the expanding atmospheric shock wave composed of ionised gas. Although it emits a considerable amount of light itself, it is opaque and prevents the far brighter fireball from shining through. The net result recorded is a decrease of the light visible from outer space as the shock wave expands, producing the first peak recorded by the bhangmeter.

As it expands, the shock wave cools off and becomes less opaque to the visible light produced by the inner fireball. The bhangmeter starts eventually to record an increase in visible light intensity. The expansion of the fireball leads to an increase of its surface area and consequently an increase of the amount of visible light radiated off to space. The fireball continuing to cool down, the amount of light eventually starts to decrease, causing the second peak observed by the bhangmeter. The time between the first and second peaks can be used to determine its nuclear yield.[12]

The effect is unambiguous for explosions below about 30 kilometres (19 mi) altitude, but above this height a more ambiguous single pulse is produced.[13]

Origin of the name[edit]

The name of the detector is a playful pun,[2] which was bestowed upon it by Fred Reines, one of the scientists working on the project. The name is derived from the Indian word "bhang", a locally grown variety of cannabis which is smoked or drunk to induce intoxicating effects, the joke being that one would have to be on drugs to believe the bhangmeter detectors would work properly. This is in contrast to a "bangmeter" one might associate with detection of nuclear explosions.[2]

See also[edit]

References[edit]

  1. ^ "Bulletin of Science, Technology & Society". Pergamon Press. 1985. 
  2. ^ a b c Ogle, William E. (October 1985). "Bhangmeter — Prologue". An account of the return to Nuclear Weapons testing by the United States after the test moratorium 1958-1961. United States Department of Energy — NV 291. p. 67. Archived from the original on 19 January 2009. Retrieved 18 December 2008. 
  3. ^ Grier, Herbert (1953). "Operation Tumbler-Snapper, Nevada Proving Grounds, April–June 1952, Project 12.1 — Bhangmeter Mod II". EG&G. 
  4. ^ "Limited Test Ban Treaty". U.S. Department of State. 1963. 
  5. ^ Bell, Aaron J. (2002). Analysis of GPS Satellite Allocation for The United States Nuclear Detonation Detection System (USNDS). Air Force Institute Of Technology. 
  6. ^ Johnston, Robert (2009). "Multimegaton Weapons". Retrieved 19 June 2012. 
  7. ^ Gruntman, Mike (2004). Blazing the trail: the early history of spacecraft and rocketry. American Institute of Aeronautics and Astronautics, Inc. ISBN 1-56347-705-X. 
  8. ^ Richelson, Jeffrey (November–December 1998). "Verification: the ways and means". Bulletin of Atomic Scientists. p. 54. 
  9. ^ a b Goldblat, Jozef; Cox, David (1988). "Means of nuclear test ban verification". Nuclear weapon tests: prohibition or limitation?. Oxford: Oxford University Press. p. 239. ISBN 9780198291206. Retrieved 16 June 2012. 
  10. ^ "GPS timeline". Retrieved 16 June 2012. 
  11. ^ Hafemeister, David. "Science and Society Test IX: Technical Means of Verification". Retrieved 16 June 2012. 
  12. ^ Forden, Geoffrey (2006). "A Constellation of Satellites for Shared Missile Launch Surveillance". MIT’s Program on Science, Technology, and Society. Retrieved 17 June 2012. 
  13. ^ Angelo, Josepha A. Jr. (2004). Nuclear Technology. Greenwood Press. pp. 304–306. ISBN 9781573563369. 

Further reading[edit]