2003
DOI: 10.1117/12.457982
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MASS: a monitor of the vertical turbulence distribution

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 S… Show more

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Cited by 115 publications
(75 citation statements)
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“…Simultaneous MASS [12] results are also shown for comparison (bottom right panel in Fig. 10; no simultaneous MASS data are available for the other datasets).…”
Section: B Slodar Resultsmentioning
confidence: 99%
“…Simultaneous MASS [12] results are also shown for comparison (bottom right panel in Fig. 10; no simultaneous MASS data are available for the other datasets).…”
Section: B Slodar Resultsmentioning
confidence: 99%
“…The beam splitting between annular apertures is done by internal optics (Kornilov et al 2003). Scintillation, which depends on the altitude of the turbulence, is detected in each aperture using photomultipliers with 1 ms exposure time.…”
Section: The Mass (Multi Aperture Scintillation Sensor)mentioning
confidence: 99%
“…Unlike most previously existing instruments, however, the division of the pupil into subapertures and the separation of the two star images of these subapertures are achieved not by a mask in the entrance pupil, but in a reimaged pupil plane behind the telescope optics using tilted mirrors. There, a second set of mirrors also separates the light of another part of the pupil and sends it to the photomultipliers of a multiaperture scintillation sensor (MASS) turbulence profiler [3]. Thus, MASS and DIMM are combined in a single instrument.…”
Section: Introductionmentioning
confidence: 99%