From Differential Image Motion to Seeing

By A. Tokovinin. 2002

269 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Atomic and Molecular Physics, and Optics, Electrical and Electronic Engineering

View Paper: https://www.semanticscholar.org/paper/5d73ceb7cb2dbe8b7878b35a3fc6a5e51fe012fc

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Aerospace Engineering

1. Joop Schaye
2. O. Siegmund
3. Thierry Contini
4. M. Carollo
5. R. Bouwens

In Atomic and Molecular Physics, and Optics

1. Marc Sarazin
2. T. Butterley
3. Joop Schaye
4. J. Richard
5. R. Wilson
6. O. Siegmund
7. R. Bouwens

In Electrical and Electronic Engineering

1. Marc Sarazin
2. T. Butterley
3. Joop Schaye
4. J. Brinchmann
5. J. Richard
6. R. Wilson
7. O. Siegmund
8. R. Bouwens

Citations in the corpus

• UV, X-ray, and gamma-ray space instrumentation for astronomy XV : 26-27 August 2007, San Diego, California, USA (2007, methodology): “We can nevertheless use the FWHM of the seeing-limited PSF and, assuming a given outer scale value, estimate the seeing as in Tokovinin(2002)[11].”
• Determination of the profile of atmospheric optical turbulence strength from SLODAR data (2006, background): “This differs slightly from the mean or gradient tilt (‘G-tilt’) of the wavefront (see e.g. Tokovinin 2002).”
• The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection (2017, methodology): “For the VLT’s large aperture, a good representation of the atmospheric turbulence is given by Tokovinin (2002) in the form of a finite outer scale von Karman turbulence model.”