17 September 2012 The new TNG-DIMM: calibrations and first data analysis
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Abstract
Since 2011 a new differential image motion monitor (DIMM) works at Roque de los Muchachos Observatory close to Telescopio Nazionale Galileo (TNG). The purpose of this instrument is to provide useful information about the optical turbulence for the astronomical observations at TNG. We present the instrument and the first statistical results including a relationship between the principal components analysis of local-ground atmospheric parameters and seeing.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Emilio Molinari, Emilio Molinari, A. G. de Gurtubai, A. G. de Gurtubai, A. della Valle, A. della Valle, S. Ortolani, S. Ortolani, J. San Juan, J. San Juan, A. F. Martinez Fiorenzano, A. F. Martinez Fiorenzano, V. Zitelli, V. Zitelli, "The new TNG-DIMM: calibrations and first data analysis", Proc. SPIE 8444, Ground-based and Airborne Telescopes IV, 844462 (17 September 2012); doi: 10.1117/12.925900; https://doi.org/10.1117/12.925900
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