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Scientific detectors for astronomy 2005: Explorers of the Photon Odyssey

Jenna E. Beletic ; James W. Beletic ; Paola Amico (eds.)

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Disponibilidad
Institución detectada Año de publicación Navegá Descargá Solicitá
No detectada 2006 SpringerLink

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Tipo de recurso:

libros

ISBN impreso

978-1-4020-4329-1

ISBN electrónico

978-1-4020-4330-7

Editor responsable

Springer Nature

País de edición

Reino Unido

Fecha de publicación

Información sobre derechos de publicación

© Springer 2006

Cobertura temática

Tabla de contenidos

Radiation Damage in HST Detectors

Marco Sirianni; Max Mutchler

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section I - Observatory Status and Plans | Pp. 171-178

An EUV Image Detector for the Space Solar Telescope

Qian Song; Binxun Ye; Zhaowang Zhao

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section I - Observatory Status and Plans | Pp. 179-186

The Camera of the Corot Space Experiment: Design, Tests and Results

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section I - Observatory Status and Plans | Pp. 187-192

Second Generation IR Detectors for the Wide Field Camera 3

Massimo Robberto; Sylvia Baggett; Rebecca Blackmon; Tom Brown; Howard Bushouse; Gregory Delo; Donald Figer; Roger Foltz; George Hartig; Bryan Hilbert; Robert J. Hill; Scott D. Johnson; Randy A. Kimble; John W. Mackenty; Eliot M. Malumuth; Elizabeth Polidan; Sam Reed; Anne Marie Russell; Augustyn Waczynski; Yiting Wen

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section I - Observatory Status and Plans | Pp. 193-198

Imaging Technique of the DISR Camera on the Huygens Lander

J. Rainer Kramm; Horst Uwe Keller; Richard Bredthauer; Martin Tomasko

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section I - Observatory Status and Plans | Pp. 199-204

Advanced Detector and Optical Fabrication Technologies for Implementing Improved Spectroscopic Instrumentations

M. Bonner Denton; Andrew K. Knight; Roger P. Sperline

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section II - Non-Astronomical Applications | Pp. 207-216

CCD Detector Systems for “Semiconductor Nanostructures” Optical Properties Research

David Darson; Pascal Morfin; Martial Nicolas; Guillaume Cassabois; JérÔme Tignon; Ivan Favero; Philippe Pace; Laurent Rea; Philippe Rossignol; Claude Delalande

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section II - Non-Astronomical Applications | Pp. 217-222

- CCD Technology

Barry Burke; Paul Jorden; Paul Vu

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section III - CCDs | Pp. 225-264

Siliconus Maximus

Richard Bredthauer; Michael Lesser

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section III - CCDs | Pp. 265-272

CCD Development Progress at Lawrence Berkeley National Laboratory

William F. Kolbe; Steve E. Holland; Christopher J. Bebek

The Earth is the most geologically active of the terrestrial planets and it has retained the poorest sample of the record of hypervelocity impact by interplanetary bodies throughout geologic time. Although the surviving sample of impact structures is small, the terrestrial impact record has played a major role in understanding and constraining cratering processes, as well as providing important ground-truth information on the three dimensional lithological and structural character of impact structures (). Recently, there has been a growing awareness in the earth-science community that impact is also potentially important as a stochastic driving force for changes to the terrestrial environment. This has stemmed largely from: the discovery of chemical and physical evidence for the involvement of impact at the Cretaceous-Tertiary (K/T) boundary and the associated mass extinction event (e.g. ; ; ), and their relation to the Chicxulub impact structure in the Yucatan Peninsula, Mexico (), the recognition of the resource potential of impact structures, some of which are related to world-class ore deposits, both spatially and genetically (; ), and the recognition of the potentially disastrous consequences of impacts for human civilization ().

Section III - CCDs | Pp. 273-280