Catálogo de publicaciones - libros
The Intelligent Enterprise: Theoretical Concepts and Practical Implications
Markus J. Thannhuber
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No disponible.
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Disponibilidad
Institución detectada | Año de publicación | Navegá | Descargá | Solicitá |
---|---|---|---|---|
No detectada | 2005 | SpringerLink |
Información
Tipo de recurso:
libros
ISBN impreso
978-3-7908-1555-9
ISBN electrónico
978-3-7908-1607-5
Editor responsable
Springer Nature
País de edición
Reino Unido
Fecha de publicación
2005
Información sobre derechos de publicación
© Physica-Verlag Heidelberg 2005
Cobertura temática
Tabla de contenidos
Introduction
Markus J. Thannhuber
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. 1-12
Background
Markus J. Thannhuber
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. 13-22
The Approach
Markus J. Thannhuber
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. 23-33
Theory of Real Systems
Markus J. Thannhuber
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. 35-52
Theory of System Knowledge
Markus J. Thannhuber
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. 53-66
The Intelligent Enterprise
Markus J. Thannhuber
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. 67-85
Realizing Enterprise Intelligence
Markus J. Thannhuber
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. 87-110
Conclusion
Markus J. Thannhuber
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. 111-113