Catálogo de publicaciones - libros
Scientific detectors for astronomy 2005: Explorers of the Photon Odyssey
Jenna E. Beletic ; James W. Beletic ; Paola Amico (eds.)
Resumen/Descripción – provisto por la editorial
No disponible.
Palabras clave – provistas por la editorial
No disponibles.
Disponibilidad
Institución detectada | Año de publicación | Navegá | Descargá | Solicitá |
---|---|---|---|---|
No detectada | 2006 | SpringerLink |
Información
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
2006
Información sobre derechos de publicación
© Springer 2006
Cobertura temática
Tabla de contenidos
Orthogonal Transfer Array
John L. Tonry; Barry Burke; Peter M. Onaka; Gerard A. Luppino
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. 281-292
A pnCCD Detector System for High Speed Optical Applications
Robert Hartmann; Hubert Gorke; Norbert Meidinger; Heike Soltau; Lothar Strüder
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. 293-302
L3 CCD Wavefront Sensor Developments at the ING
Simon Tulloch
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. 303-314
Zero Noise Wavefront Sensor Development within the Opticon European Network
Philippe Feautrier; Thierry Fusco; Mark Downing; Norbert Hubin; Jean-Luc Gach; Philippe Balard; Christian Guillaume; Eric Stadler; Olivier Boissin; Paul Jorden; José Javier Diaz
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. 315-320
A Dedicated L3Vision CCD for Adaptive Optics Applications
Mark Downing; Norbert Hubin; Markus Kasper; Paul Jorden; Peter Pool; Sandy Denney; Wolfgang Suske; David Burt; Pat Wheeler; Kevin Hadfield; Philippe Feautrier; Jean-Luc Gach; Javier Reyes; Manfred Meyer; Dietrich Baade; Philippe Balard; Christian Guillaume; Eric Stadler; Olivier Boissin; Thierry Fusco; José Javier Diaz
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. 321-328
The Ultimate CCD for Laser guide star wavefront sensing on Extremely Large Telescopes
James W. Beletic; Sean Adkins; Barry Burke; Robert Reich; Bernie Kosicki; Vyshnavi Suntharalingham; Charlie Bleau; Ray DuVarney; Richard Stover; Jerry Nelson; Francois Rigaut
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. 329-336
The MMT Megacam
Brian McLeod; John Geary; Mark Ordway; Steven Amato; Maureen Conroy; Thomas Gauron
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. 337-344
The OmegaCAM 16K×16K CCD Detector System for the ESO VLT Survey Telescope (VST)
Olaf Iwert; Dietrich Baade; Andrea Balestra; Andrea Baruffolo; Alessandro Bortolussi; Fabrice Christen; Claudio Cumani; Sebastian Deiries; Mark Downing; Christoph Geimer; Guy Hess; Joachim Hess; Koen Kuijken; Jean-Louis Lizon; Harald Nicklas; Roland Reiss; Javier Reyes; 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 III - CCDs | Pp. 345-352
CCD Mosaics at CTIO and SOAR
Ricardo E. Schmidt
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. 353-360
Focal Plane Detectors for the Dark Energy Survey
Juan Estrada; Ricardo E. Schmidt
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. 361-368