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The Dutch Open Telescope on La Palma

Published online by Cambridge University Press:  14 March 2005

R.J. Rutten ,
F.C.M. Bettonvil ,
R.H. Hammerschlag ,
A. P. L. Jägers ,
J. Leenaarts ,
F. Snik ,
P. Sütterlin ,
K. Tziotziou  and
A.G. de Wijn
R.J. Rutten
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
F.C.M. Bettonvil
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
R.H. Hammerschlag
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
A. P. L. Jägers
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
J. Leenaarts
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
F. Snik
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
P. Sütterlin
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
K. Tziotziou
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
A.G. de Wijn
Affiliation:
Sterrekundig Instituut, Faculteit Natuur- en Sterrenkunde, Utrecht University Postbus 80000, NL–3508 TA Utrecht, The Netherlands email: [email protected]
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Abstract

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The Dutch Open Telescope (DOT) on La Palma is an innovative solar telescope combining open telescope structure and an open support tower with a multi-wavelength imaging assembly and with synchronous speckle cameras to generate high-resolution movies which sample different layers of the solar atmosphere simultaneously and co-spatially at high resolution over long durations. The DOT test and development phase is nearly concluded. The installation of an advanced speckle processor enables full science utilization including “Open-DOT” time allocation to the international community. Co-pointing with spectropolarimeters at other Canary Island telescopes and with TRACE furnishes valuable Solar-B precursor capabilities.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 597 - 604
Copyright
© 2004 International Astronomical Union