Analysis of Temporal Variations in Failed Missile Launches in the Soviet Union (Russia) and the United States
- Authors: Veniaminov S.S.1, Klyushnikov V.Y.2, Kozlov S.I.1,3, Nagorskiy P.M.4
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Affiliations:
- Research Testing Center, Central Research Institute, Aerospace Defense Forces
- Central Research Institute of Machine Building
- Institute of Geosphere Dynamics, Russian Academy of Sciences
- Institute of Monitoring of Climatic and Ecological Systems, Siberian Branch, Russian Academy of Sciences
- Issue: Vol 56, No 6 (2018)
- Pages: 480-487
- Section: Article
- URL: https://journal-vniispk.ru/0010-9525/article/view/153472
- DOI: https://doi.org/10.1134/S0010952518060102
- ID: 153472
Cite item
Abstract
Temporal variations in the relative number of failed rocket launches in Russia (Soviet Union) and the United States have been compared to reveal that these variations are antipersistent. The accident rates of rocket and space equipment launches have been analyzed as a function of the level and phase of solar activity cycle. The relative number of failed launches in Russia (Soviet Union) and the United States for the growth phase of solar activity has been shown to exceed the number for the phase of solar activity decline, although no clear correlation between solar activity and the number of failed launches has been detected.
About the authors
S. S. Veniaminov
Research Testing Center, Central Research Institute, Aerospace Defense Forces
Author for correspondence.
Email: npm_sta@mail.ru
Russian Federation, Moscow
V. Yu. Klyushnikov
Central Research Institute of Machine Building
Email: npm_sta@mail.ru
Russian Federation, Korolev, Moscow oblast
S. I. Kozlov
Research Testing Center, Central Research Institute, Aerospace Defense Forces; Institute of Geosphere Dynamics, Russian Academy of Sciences
Email: npm_sta@mail.ru
Russian Federation, Moscow; Moscow
P. M. Nagorskiy
Institute of Monitoring of Climatic and Ecological Systems, Siberian Branch, Russian Academy of Sciences
Email: npm_sta@mail.ru
Russian Federation, Tomsk
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