Observational rates under terahertz (THz) opacities less than 3.0 and 2.0 at the Atacama Large Millimeter/submillimeter Array (ALMA) site have been calculated using the 225 GHz tipping radiometer monitoring data and the opacity correlation between 225 GHz and THz opacities. The observational rate with THz opacity condition less than 3.0 is 12.4% in a year, and in winter (November - April) it is about twice higher than in summer (May - October). This observational rate shows a large sinusoidal annual variation, and it seems to have relation with the El Ni\~no and La Ni\~na phenomena; the La Ni\~na years tend to have high observational rates, but the El Ni\~no years show low rates. On the other hand, the observational rate with the THz opacity condition less than 2.0 is only 1.9%, and no obvious annual and seasonal variations are observed. This indicates that THz observations under low opacity condition of less than 2.0 at the ALMA site are very difficult to be performed.
@article{arxiv.1108.2279,
title = {Possibility of Terahertz Observations at the ALMA site},
author = {Satoki Matsushita},
journal= {arXiv preprint arXiv:1108.2279},
year = {2015}
}
Comments
4 pages, 3 figures. Conference proceeding of "Atmospheric Data from Astronomical Site Testing in Chile." To be appeared on the Revista Mexicana de Astronom\'ia y Astrof\'isica Conference Series