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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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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

Detector Systems for the MODS Spectrograph

Bruce Atwood; Daniel Pappalardo; Mark A. Derwent; Thomas P. O'Brien

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. 109-116

Recent Photon Counting Developments at the Observatoire de Marseille

Philippe Balard; Philippe Amram; Olivier Boissin; Jacques Boulesteix; Olivier Daigle; Jean-Luc Gach; Olivia Garrido; Olivier Hernandez; Michel Marcelin

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. 117-122

A CMOS Sensor for Solar Observation

Francis Beigbeder; Sylvain Rondi; Nadège Meunier; Michel Rieutord

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. 123-128

Plasma Cleaning

Sebastian Deiries; Armin Silber; Olaf Iwert; Evi Hummel; Jean Louis Lizon

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. 129-136

Thermal Modeling of the Wide-Field Infrared Camera for the CFHT

Philippe Feautrier; Eric Stadler; Pascal Puget

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. 137-142

Cooling System for the OmegaCAM CCD Mosaic

Jean Louis Lizon; Armin Silber

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. 143-146

Bonn Shutters for the Largest Mosaic Cameras

Klaus Reif; Günther Klink; Philipp Müller; Henning Poschmann

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. 147-152

Slicing the Universe - CCDs for MUSE

Roland Reiss; Sebastian Deiries; Jean Louis Lizon; Manfred Meyer; Javier Reyes; Roland Bacon; François Hénault; Magali Loupias

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. 153-158

On-Chip Guiding with a Mosaic of HAWAII-2RG Infrared Detectors

Martin Riopel; Douglas Teeple; Jeff Ward

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. 159-164

The Blue Channel of the Large Binocular Camera

Roberto Speziali; Fernando Pedichini; Andrea Di Paola; Emanuele Giallongo; Roberto Ragazzoni; Andrea Baruffolo; E. Diolaiti; C. De Santis; J. Farinato; Adriano Fontana; S. Gallozzi; F. Gasparo; F. Pasian; R. Smareglia; E. Vernet

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. 165-170