The following graphic information of our weather stations, are used to determine when you can make astronomical observations with telescopes and if the weather is too adverse for this activity it is shown. We also use the data for the quality control of the images obtained from the observatory and study its relationship with certain astronomical parameters such as the magnitude of sky background, extinction in certain wavelengths or so-called "astronomical seeing."

We put at the disposal of the general public one of our cameras for follow-up and vigilance, with vision of the peak of the Sagra installed in the same observatory.


Weather Station DAVIS VANTAGE VUE (Universal Time format UT).


Meteo parameters WebCam
Temperature Humidity
Wind speed Preasure
Precipitation Cloud sensor