Bibcode
Vernin, J.; Munoz-Tunon, C.
Referencia bibliográfica
Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 1, p. 311-318
Fecha de publicación:
4
1994
Número de citas
84
Número de citas referidas
72
Descripción
The results of an intensive site testing assessment campaign, held at
the Observatorio del Roque de los Muchachos (ORM) (La Palma) during four
nights on July 1990 are presented and discussed. To evaluate the optical
quality of an astronomical site for high angular resolution astronomy
our philosophy leads us to make use of as many instruments as possible.
The Scidar instrument was adapted to the Nordic Optical Telescope (NOT)
focus, whilst free-flying balloons and an instrumented mast were used to
evaluate the 'open air' seeing. The results are described following a
classical approach in terms of seeing. During three nights out of four,
image size was better than 0.7 sec. The mean value, however, goes up to
0.96 sec due to strong turbulent layers appearing during part of one of
the observing nights. The geophysics relevant to understanding the
genesis of these turbulent layers in terms of the atmosphere stability
is discussed. The contribution to image size degradation from the
surface layer is almost negligible. From a comparison between seeing
measured at at the NOT focus and the seeing for the whole atmosphere, it
is concluded that NOT dome and mirror seeing do not significantly
contribute to image degradation; it is an example of a well designed
system in terms of thermal turbulence. The mean value of seeing attained
at NOT focus with Scidar working as a seeing monitor was 0.76 sec. From
balloon soundings, quantities related to high angular resolution
astronomy like the speckle lifetime and the isoplanatic angle, as well
as the integrated content of water vapor relevant to IR astronomy are
obtained. The isoplanatic angle is less than two arcsec and, in most
cases, the number of well defined turbulent layers is very small, so
that multiconjugate adaptive optics is applicable. The mean value of
precipitable water vapor content is 3.4 mm with a minimum attained value
of 1.99 mm. This points towards the ORM to be a potentially good site
for IR astronomy although, clearly, a longer sample would have to be
taken for this to be established.