In this paper we present an analysis of wind speed, wind direction, relative humidity and air pressure taken at TNG, CAMC and NOT at Observatorio del Roque de Los Muchachos, in the Canary Islands. Data are compared in order to check local variations and both long term and short term trends of the microclimate. Furthermore, influence of wind speed on the astronomical seeing is estimated to the aim to better understand the influence of wide scale parameters on local meteorological data. The three telescopes show different prevailing wind direction, wind speed, relative humidity and air pressure confirming differences in local microclimate. We found that seeing deteriorates when wind speed is lower than 3.3 m/s. Comparison in terms of wind spe...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
ABSTRACT The requirements for current large and future extremely large telescopes as well as the qui...
In this paper we present an analysis of temperature taken at two telescopes located at the Observato...
The new extremely large telescope projects need accurate evaluation of the candidate sites. In this ...
The early 1970's saw the start of a new era in astronomy with the rst approach to building large tel...
The early 1970's saw the start of a new era in astronomy with the rst approach to building large tel...
In this paper, we present meteorological and photometric studies of the Oukaimeden astronomical site...
In this paper, we present meteorological and photometric studies of the Oukaimeden astronomical site...
We present comprehensive and reliable statistics of high altitude wind speeds and the tropospheric f...
Context: It is known that the Canary Islands are normally affected by dominant winds flowing from no...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
Extrapolations from 10m above the ground up to the wind turbine hub height are frequently made to th...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
ABSTRACT The requirements for current large and future extremely large telescopes as well as the qui...
In this paper we present an analysis of temperature taken at two telescopes located at the Observato...
The new extremely large telescope projects need accurate evaluation of the candidate sites. In this ...
The early 1970's saw the start of a new era in astronomy with the rst approach to building large tel...
The early 1970's saw the start of a new era in astronomy with the rst approach to building large tel...
In this paper, we present meteorological and photometric studies of the Oukaimeden astronomical site...
In this paper, we present meteorological and photometric studies of the Oukaimeden astronomical site...
We present comprehensive and reliable statistics of high altitude wind speeds and the tropospheric f...
Context: It is known that the Canary Islands are normally affected by dominant winds flowing from no...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
Extrapolations from 10m above the ground up to the wind turbine hub height are frequently made to th...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
This study analyses quality controlled and homogenized near-surface wind speed series (SWS) at 87 me...
ABSTRACT The requirements for current large and future extremely large telescopes as well as the qui...