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Proceedings Paper

MASS: a monitor of the vertical turbulence distribution
Author(s): Victor Kornilov; Andrei A. Tokovinin; Olga Vozyakova; Andrei Zaitsev; Nicolai Shatsky; Serguei F. Potanin; Marc S. Sarazin
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Paper Abstract

The MASS (Multi-Aperture Scintillation Sensor) instrument consists of a 14-cm off-axis reflecting telescope and a detector unit which measures the scintillations of single stars in four concentric zones of the telescope pupil using photo-multipliers. Statistical analysis of these signals yields information of the vertical turbulence profile with a resolution of dh/h=0.5. We describe the instrument and present the results of its first field tests, including comparisons with DIMM seeing monitor and generalized SCIDAR. MASS will be used to obtain the extensive statistics of turbulence profiles at potential sites of future giant telescopes, as needed to predict the quality of adaptive seeing compensation.

Paper Details

Date Published: 7 February 2003
PDF: 9 pages
Proc. SPIE 4839, Adaptive Optical System Technologies II, (7 February 2003); doi: 10.1117/12.457982
Show Author Affiliations
Victor Kornilov, Sternberg Astronomical Institute (Russia)
Andrei A. Tokovinin, Cerro Tololo Inter-American Observatory (Chile)
Olga Vozyakova, Sternberg Astronomical Institute (Russia)
Andrei Zaitsev, Sternberg Astronomical Institute (Russia)
Nicolai Shatsky, Sternberg Astronomical Institute (Russia)
Serguei F. Potanin, Sternberg Astronomical Institute (Russia)
Marc S. Sarazin, European Southern Observatory (Germany)


Published in SPIE Proceedings Vol. 4839:
Adaptive Optical System Technologies II
Peter L. Wizinowich; Domenico Bonaccini, Editor(s)

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