Add to ORKGMany instruments are able to provide local (in space and time) estimations of all the astroclimatic parameters that depend on the optical turbulence. The numerical technique is, at the present time, the only approach that can provide 3D characterization of the optical turbulence. Since a few years, many efforts have been dedicated to increase the reliability of the atmospherical meso-scale model called Meso-Nh in simulating C[N]2 profiles above astronomical sites. The most recent and promising results have been obtained above the San Pedro Mártir site. In this paper these results are summarized
Abstract. In order to eciently use the recent astronomy high angular resolution techniques (Adaptive...
We present the results of monitoring optical-turbulence profiles at San Pedro Maacute;rtir, M...
In order to efficiently use the recent astronomy high angular resolution techniques (Adaptive Optic...
In preceding papers we have presented comparisons between simulated and measured $C_N^2$profiles abo...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
The first statistical results of simulations of optical turbulence over Cerro Paranal by an atmosphe...
Results of monitoring optical-turbulence profiles and velocity of the turbulence layers at San P...
We present the first complete seasonal variation study extended over 1 year, of all the principal as...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
The numerical technique is, at the present time, the only approach that can provide 3D C[N]2 ma...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
The optical turbulence, which creates perturbations of the wavefronts coming from the stars, is caus...
Abstract. In order to eciently use the recent astronomy high angular resolution techniques (Adaptive...
We present the results of monitoring optical-turbulence profiles at San Pedro Maacute;rtir, M...
In order to efficiently use the recent astronomy high angular resolution techniques (Adaptive Optic...
In preceding papers we have presented comparisons between simulated and measured $C_N^2$profiles abo...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
We show results obtained from simulations of the optical turbulence (OT), provided by the atmospheri...
The first statistical results of simulations of optical turbulence over Cerro Paranal by an atmosphe...
Results of monitoring optical-turbulence profiles and velocity of the turbulence layers at San P...
We present the first complete seasonal variation study extended over 1 year, of all the principal as...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
The numerical technique is, at the present time, the only approach that can provide 3D C[N]2 ma...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
These last years have seen the development of many devices to measure and monitor some atmospheric ...
The optical turbulence, which creates perturbations of the wavefronts coming from the stars, is caus...
Abstract. In order to eciently use the recent astronomy high angular resolution techniques (Adaptive...
We present the results of monitoring optical-turbulence profiles at San Pedro Maacute;rtir, M...
In order to efficiently use the recent astronomy high angular resolution techniques (Adaptive Optic...