We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

Characterization of the mesospheric sodium layer at La Palma.

Michaille, L. and Clifford, J. B. and Dainty, J. C. and Gregory, T. and Quartel, J. C. and Reavell, F. C. and Wilson, R. W. and Wooder, N. J. (2001) 'Characterization of the mesospheric sodium layer at La Palma.', Monthly notices of the Royal Astronomical Society., 328 (4). pp. 993-1000.


We present the results of a mesospheric sodium monitoring programme at La Palma carried out through five campaigns of one week each, from 1999 September to 2000 August. The yearly averaged parameters of the layer (the sodium column density and the width) are given. We show that the short time-scale dynamics of the layer are governed by the sporadic layers with an average frequency of one event per night. The influence of the short time-scale dynamics of the layer on an adaptive optics system working on the William Herschel Telescope is quantified. It appears that it is a small effect in terms of defocus error. Finally, we present data obtained during the Perseid meteor shower and show that the dynamics of the sodium layer undergoes a transition with the meteoric activity.

Item Type:Article
Additional Information:
Keywords:Atomic processes, Scattering, Atmospheric effects, Site testing, telescopes.
Full text:Full text not available from this repository.
Publisher Web site:
Record Created:22 Nov 2006
Last Modified:08 Apr 2009 16:24

Social bookmarking: del.icio.usConnoteaBibSonomyCiteULikeFacebookTwitterExport: EndNote, Zotero | BibTex
Look up in GoogleScholar | Find in a UK Library