Original mission objectives
Originally Argus was designated Hardtack-Argus, and later FLORAL. For reasons of security, both names were dropped in favor of the independent name, Argus. Funding was provided by the Armed Forces Special Weapons Project (AFSWP), the predecessor of today's Defense Threat Reduction Agency (DTRA). Total funds allotted for the project were US$ 9,023,000. Task Force 88The United States Navy Task Force 88 (or TF-88), was formed 28 April 1958. TF-88 was organized solely to conduct Operation Argus. Once Argus was completed, the task force was dissolved, and its records dispersed. Some of these records have been destroyed or lost in the intervening time period. Of particular note among the missing documents were the film records (which recorded radiation levels during the Argus tests). This has proved contentious due to the higher-than-normal number of leukemia claims among TF-88 participants to the Veterans Administration. Because of this, it has been difficult to resolve just how much radiation participants were exposed to. The Norton Sound was responsible for missile-launching functions. She also served as a training facility for crews involved in the testing. The X-17A missiles to be used in the test were unfamiliar to those conducting the tests. Exercises including assembly and repair of dummy missiles were conducted aboard the Norton Sound. She also carried a 27-MHz COZI radar, which was operated by Air Force Cambridge Research Center, which was used to monitor effects of the shots. The Albermarle, fresh out of an overhaul, was not listed on the TF-88 order. She set out to the Atlantic, supposedly on shakedown. She, too, mounted a COZI radar and other instrumentation for detecting man-made ionization. The Tarawa served as overall command of the operation, with her commander serving as Task Group Commander. She carried an Air Force MSQ-1A radar and communication system for missile tracking. She also housed VS-32 aircraft for search and security operations as well as scientific measurement, photographic, and observer missions for each shot. The Warrington, in conjunction with the Bearss, Hammerberg, and Courtney maintained a weather picket 463 km west of the task force, provided a plane guard for the Tarawa during flight operations, and carried out standard destroyer functions (such as surface security and search and rescue). The Warrington also carried equipment for launching Loki Dart rockets. The Neosho refueled task for ships during the operation. She was also outfitted with Air Force MSQ-1A radar. The Salamonie returned to the United States upon arrival at TF-88, and did not participate in any shots. The testsAbout 1800 km southwest of Cape Town, South Africa, USS Norton Sound launched three modified X-17A missiles armed with 1.7 kt W-25 nuclear warheads into the upper atmosphere, where high altitude nuclear explosions took place. The (extreme) altitude of the tests was chosen so as to prevent personnel involved in the test from being exposed to any ionizing radiation [1]. Coordinated measurement programs involving satellite, rocket, aircraft, and surface stations were employed by the services as well as other government agencies and various contractors worldwide. The tests were proposed by Nicholas Christofilos of what was then the Livermore branch of the Lawrence Radiation Laboratory (now Lawrence Livermore National Laboratory) as a means to verify the Christofilos theory, which argued that high-altitude nuclear detonations would create a radiation belt in the extreme upper regions of the Earth's atmosphere. Such belts would be similar in effect to the Van Allen radiation belts. Such radiation belts were viewed as having possible tactical use in war. Prior to Argus, Hardtack Teak had shown disruption of radio communications from a nuclear blast. However, this was not due to the creation of radiation belts. The Argus explosions created artificial electron belts resulting from the β-decay of fission fragments. These lasted for several weeks. Such radiation belts affect radio and radar transmissions, damage or destroy arming and fusing mechanisms of intercontinental ballistic missile warheads, and endanger crews of orbiting space vehicles. Argus proved the validity of Christofilos theory: the establishment of an electron shell derived from neutron and β-decay of fission products and ionization of device materials in the upper atmosphere was demonstrated. It not only provided data on military considerations, but produced a "great mass" of geophysical data. The tests were first reported by the New York Times on March 19, 1959, headlining it as the "greatest scientific experiment ever conducted." Approximately nine ships and 4,500 people participated in the operation. After the completion of testing, the task force departed for the United States via Rio de Janeiro, Brazil. Followed the Hardtack I series, but preceded Hardtack II. While the tests were announced the following year, the full results and documentation of the tests were not declassified until 30 April 1982. List of Argus Launches
Source: [2] List of ships involved in Operation Argus
See alsoReferences
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