Seeing and coherence time

Description

Astronomical seeing (units arcesec) refers to the blurring or instantaneous image broadening of astronomical objects caused by turbulent mixing in the Earth's atmosphere due to the variations of the optical refractive index.

Importance

Atmospheric optical conditions are crucial for selecting the best astronomical sites of the world, among them, the seeing because is directly related with the spatial resolution of images. Typical median seeing at the Canarian Observatories is of 0.7".

Seeing and coherence time
Techniques of measurement

The differential image motion monitor (Stock & Keller 1960; Sarazin & Roddier 1990; Vernin & Muñoz-Tuñón 1995) oper- ates by measuring the wavefront slope differences over two small pupils some distance apart.

Results

The seeing values at the ORM ranges from 0.63" to 0.72" (25th perc.=0.53"). Thes values, well below 1", assure the optimal conditions for High Resolution and AO in particular. The results obtained with different techniques and periods, are all in very good agreement with differences below one tenth.

Related documents
Control quality of seeing measurements provided by the DIMMA at the ORM

Control quality of seeing measurements provided by the DIMMA at the ORM Antonia M. Varela, Casiana Muñoz-Tuñón & Julio Castro-Almazán Feb-2013- Technical report ------------------------------------- An automatic DIMM is installed near the GTC site. Data have been validated and the results presented in this document. Real time values are accessible at http://www.iac.es/site-testing/DIMMA_ORM. The comparison baseline spans from April to October 2012. Mean and median values in this period are 0.95” and 0.86” respectively.

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