Author/Authors :
Ishii، نويسنده , , S. and Seta، نويسنده , , M. and Nakai، نويسنده , , N. and Nagai، نويسنده , , S. and Miyagawa، نويسنده , , N. and Yamauchi، نويسنده , , A. and Motoyama، نويسنده , , H. and Taguchi، نويسنده , , M.، نويسنده ,
Abstract :
We measured the 220 GHz atmospheric-transparency at the Dome Fuji station in Antarctica from 18 December 2006 to 14 January 2007 using a tipping radiometer. The mean optical depth at zenith was 0.045 ± 0.007, and during 98% of this period we measured an optical depth of less than 0.06. These data indicate that the atmospheric-transparency in summer at Dome Fuji is comparable to that of well-known submillimeter astronomical sites such as the Atacama desert in Chile in their best seasons.