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Analytical Criterion for Aircraft Spin Susceptibility

机译:飞机自旋磁化率的分析标准

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摘要

This paper presents an analytical criterion for spin susceptibility of airplanes based on the occurrence of a second SNB point at high angles of attack and large yaw rates signifying incipient spin. This approach is a significant departure from previous ones, which focused on either identifying low-α instabilities that may lead to spin onset or on explicitly seeking spin equilibria. Consequently, the analytical criterion could be obtained in a simple form, which is presented in two complementary ways: one, in terms of the zeros of a simple algebraic expression as a function of angle of attack, and alternatively as a composite plot of SNB points and accessible regions in r - α space. The composite plot simultaneously considers limits on all control deflections, identifies unconnected SNB points, and is likely to be more useful to the designer. The prediction by either form of the criterion is seen to match extremely well with spin onset observed in computations and in the spin tunnel for the F-18 HARV. The criterion needs to be tested against further sets of aircraft data; nevertheless, the present results are a significant achievement for the complex, longstanding and formidable problem of aircraft spin.
机译:本文基于高迎角和大偏航率下第二个SNB点的出现,提出了一种飞机自旋敏感性的分析标准,这表示初始自旋。该方法与以前的方法大不相同,后者侧重于确定可能导致自旋发作的低α不稳定性,或明确寻求自旋平衡。因此,可以以一种简单的形式获得分析标准,该标准以两种互补的方式表示:一种是根据简单的代数表达式的零点作为迎角的函数,另一种是作为SNB点的合成图和r-α空间中的可及区域。合成图同时考虑了所有控制偏差的限制,识别了未连接的SNB点,这可能对设计人员更有用。通过两种形式的准则进行的预测都被认为与F-18 HARV在计算中和在自旋隧道中观察到的自旋开始非常匹配。该标准需要与其他飞机数据集进行测试;然而,目前的结果对于飞机旋转的复杂,长期和艰巨的问题是一项重大成就。

著录项

  • 来源
    《Journal of Aircraft》 |2010年第5期|p.1804-1807|共4页
  • 作者单位

    University of Illinois at Urbana-Champaign, Urbana, Illinois 61801;

    rnKorea Advanced Institute of Science and Technology, Daejeon 305-701, Republic of Korea Division of Aerospace Engineering, KAIST, 373-1 Guseong-dong, Yuseong-gu;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-18 02:30:23

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