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Wire Ropes: Tension, Endurance, Reliability

K. Feyrer

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Institución detectada Año de publicación Navegá Descargá Solicitá
No detectada 2007 SpringerLink

Información

Tipo de recurso:

libros

ISBN impreso

978-3-540-33821-5

ISBN electrónico

978-3-540-33831-4

Editor responsable

Springer Nature

País de edición

Reino Unido

Fecha de publicación

Información sobre derechos de publicación

© Springer-Verlag Berlin Heidelberg 2007

Cobertura temática

ingenieria

Ingeniería y tecnología

Tabla de contenidos

doi: 10.1007/978-3-540-33831-4_1

Wire Ropes, Elements and Definitions

K. Feyrer

The Sun is at the origin of the energy we receive, the very origin of life. We believe we know it well and yet it has only been a short time since we first became fully aware of its behavior! The first spectral studies to determine its chemical composition were carried out during the nineteenth century. In 1945, the appendix to the Manhattan project concerning the first atom bomb provided an explanation for the internal source of the Sun's energy. Finally, in 1995, the SOHO satellite (SOlar Heliospheric Observatory, ESA/NASA) was launched. Since then, findings have accumulated. So where do we go from here?

Pp. 1-59

doi: 10.1007/978-3-540-33831-4_2

Wire Ropes under Tensile Load

K. Feyrer

The Sun is at the origin of the energy we receive, the very origin of life. We believe we know it well and yet it has only been a short time since we first became fully aware of its behavior! The first spectral studies to determine its chemical composition were carried out during the nineteenth century. In 1945, the appendix to the Manhattan project concerning the first atom bomb provided an explanation for the internal source of the Sun's energy. Finally, in 1995, the SOHO satellite (SOlar Heliospheric Observatory, ESA/NASA) was launched. Since then, findings have accumulated. So where do we go from here?

Pp. 61-171

doi: 10.1007/978-3-540-33831-4_3

Wire Ropes Under Bending and Tensile Stresses

K. Feyrer

The Sun is at the origin of the energy we receive, the very origin of life. We believe we know it well and yet it has only been a short time since we first became fully aware of its behavior! The first spectral studies to determine its chemical composition were carried out during the nineteenth century. In 1945, the appendix to the Manhattan project concerning the first atom bomb provided an explanation for the internal source of the Sun's energy. Finally, in 1995, the SOHO satellite (SOlar Heliospheric Observatory, ESA/NASA) was launched. Since then, findings have accumulated. So where do we go from here?

Pp. 173-316