Innovative telescopes and instrumentation for solar astrophysics
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Innovative telescopes and instrumentation for solar astrophysics 24-28 August 2002, Waikoloa, Hawaii, USA by James Tyler Kent

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Published by SPIE in Bellingham, WA .
Written in English

Book details:

Edition Notes

StatementStephen L. Keil, Sergey V. Avakyan, chairs/editors.
LC ClassificationsQB
The Physical Object
Paginationxiv, 690 p. :
Number of Pages690
ID Numbers
Open LibraryOL22525809M
ISBN 100819446327

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Telescopes and Instrumentation for Solar Astrophysics Silvano Fineschi Mark A. Gummin SUB Gottingen Chi/EditChairs/Editors August SanD,»,o,n,aUSA Sponsored and Published by SPIE—The International Society for Optical Engineering Volume SPIE is an international technical society dedicated to advancing engineering. The 4-m aperture Advanced Technology Solar Telescope (ATST) is the next generation ground based solar telescope. In this paper we provide an overview of the ATST post-focus instrumentation. The new m high resolution telescope will be build up on the reused solar tower of the German 45 cm Gregory Coude Telescope at the Teide Observatory, Izana, Tenerife. The new telescope is a Gregory type with open telescope structure, alt-azimuth mount, complete retractable dome, and a pool of well established and new developed post focus instruments. The New Vacuum Solar Telescope (NVST) is a one meter vacuum solar telescope that aims to observe fine structures on the Sun. The main goals of NVST are high resolution imaging and spectral observations, including measurements of the solar magnetic by:

Abstract. For high resolution spectral observations of the Sun – particularly its chromosphere, we have developed a dual-band echelle spectrograph named Fast Imaging Solar Spectrograph (FISS), and installed it in a vertical optical table in the Coudé Lab of the meter New Solar Telescope at Big Bear Solar by:   David N Burrows is Professor of Astronomy and Astrophysics at the Pennsylvania State University, and lead scientist for the X-ray Telescope on NASA's Swift satellite. His research interests include X-ray instrumentation, gamma-ray burst afterglows and supernova remnants. In this paper, we describe its mechanical and optical design, the polishing and testing of the optics and the instrumentation in use or planned for this telescope. Paper Details Date Published: 11 February PDF: 10 pages Proc. SPIE , Innovative Telescopes and Instrumentation for Solar Astrophysics, (11 February ); doi: / Phase diverse speckle inversion applied to data from the Swedish 1-meter solar telescope: Authors: Lofdahl, Mats G.; Scharmer, Goran B. Affiliation: AA(Institute for Solar Physics, USA), AB(Institute for Solar Physics, USA) Publication: Innovative Telescopes and Instrumentation for Solar Astrophysics. Edited by Stephen L. Keil, Sergey V. Avakyan.

Get this from a library! Innovative telescopes and instrumentation for solar astrophysics: August , Waikoloa, Hawaii, USA. [Stephen L Keil; S V Avaki︠a︡n; Society of Photo-optical Instrumentation Engineers.; International Commission for Optics.; SPIE Digital Library.;]. Astro-Physics. 16" Easy-Balance Dovetail Saddle Plate with 3 clamps - , , , , Mach1 and Mach2 (DOVELM) This 16" Dovetail Saddle Plate, designed and manufactured by Astro-Physics, is the ultimate in versa. Solar. Baader Planetarium Solar ; Kendrick Solar ; Spacers & Extensions Astro-Physics telescopes are world-renowned for sharp, high-contrast image quality and mechanical construction. Astro-Physics. mm f StarFire GTX "Gran Turismo" with " Focuser (GTX) Astro-Physics introduced the re-imagined "Gran Turismo" at the Northeast. The design characteristics of a large open telescope (LOT) are: (i) an open tower with only pure translations of the platform under wind load; (ii) an open telescope construction with extremely stiff geometry and drives; (iii) simple optics with easy aligning and testing, but nevertheless suitable for large auxiliary equipment like by: 8.