Result: DOT tomography of the solar atmosphere: I. Telescope summary and program definition
Title:
DOT tomography of the solar atmosphere: I. Telescope summary and program definition
Source:
Astronomy and astrophysics (Berlin. Print). 413(3):1183-1189
Publisher Information:
Les Ulis: EDP Sciences, 2004.
Publication Year:
2004
Physical Description:
print, 56 ref
Original Material:
INIST-CNRS
Subject Terms:
Astronomy earth cosmic environment, Astronomie et environnement cosmique terrestre, Sciences exactes et technologie, Exact sciences and technology, Terre, ocean, espace, Earth, ocean, space, Astronomie, Astronomy, Astronomie fondamentale et astrophysique. Instrumentation, techniques, et observations astronomiques, Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations, Techniques d'observation et de réduction des données. Simulation et modélisation par ordinateur, Observation and data reduction techniques. Computer modeling and simulation, Traitement des images (incluant l'extraction des sources), Image processing (including source extraction), Système solaire, Solar system, Physique solaire, Solar physics, Chromosphère solaire et transition chromosphère-couronne. Spicules, Chromosphere and chromosphere-corona transition. Spicules, Atmosphère solaire, Solar atmosphere, Chromosphère solaire, Solar chromosphere, Cromosfera solar, Observation multifréquence, Multifrequency observation, Observación multifrecuencia, Photosphère solaire, Solar photosphere, Fotosfera solar, Soleil, Sun, Speckle, Speckles, Technique mesure, Measurement technique, Técnica medida, Tomographie, Tomography, Traitement image, Image processing, Sun: chromosphere, Sun: photosphere, techniques: image processing, telescopes
Document Type:
Academic journal
Article
File Description:
text
Language:
English
Author Affiliations:
Sterrekundig Instituut, Utrecht University, Postbus 80 000, 3508 TA Utrecht, Netherlands
Institute of Theoretical Astrophysics, Oslo University, PO Box 1029 Blindern, 0315 Oslo, Norway
ASTRON/NFRA, Postbus 2, 7990 AA Dwingeloo, Netherlands
Institute of Theoretical Astrophysics, Oslo University, PO Box 1029 Blindern, 0315 Oslo, Norway
ASTRON/NFRA, Postbus 2, 7990 AA Dwingeloo, Netherlands
ISSN:
0004-6361
Rights:
Copyright 2004 INIST-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Notes:
Astronomy
Accession Number:
edscal.15401575
Database:
PASCAL Archive
Further Information
The Dutch Open Telescope (DOT) on La Palma is an innovative optical solar telescope capable of reaching 0.2 arcsec angular resolution over extended durations. The DOT presently progresses from technology testbed to a stable science configuration providing multi-wavelength imaging and multi-camera speckle data acquisition for tomographic mapping of the solar atmosphere. Large-volume speckle processing will soon enable frequent usage and community-wide time allocation, in particular for tandem operation with other solar telescopes pursuing spectropolarimetry and EUV imaging. We summarize the DOT hardware and software in the context of this increasing availability and outline the corresponding open-DOT program.