turbulence;
atmospheric effects;
methods: data analysis;
site testing;
TIBETAN PLATEAU;
DOME-C;
SIMULATIONS;
PARAMETERS;
PROFILES;
SCINTILLATION;
RESOLUTION;
TELESCOPE;
ROGUE;
SITES;
D O I:
10.1093/mnras/stad2795
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
A worldwide search is currently being conducted to determine the most appropriate sites for the next generation of large optical and infrared telescopes. Here, we report a global map of atmospheric optical turbulence-associated parameter (atmospheric coherence length) based on the fifth generation of European Centre for Medium Range Weather Forecasts re-analysis data set and results for atmospheric coherence lengths at European Southern Observatory and Tibetan Plateau locations (all at mid latitudes). These confirm the accuracy of the global atmospheric optical turbulence model, but also the simulation result reveals that an excellent atmospheric calm site exist at the Ethiopian Plateau (at a latitude of similar to 10 N-degrees) outside of the rainy season. The Ethiopian Plateau is the highest plateau in Africa, known as the 'Roof of Africa', with an average ele v ation of o v er 2500 m, and thus potentially provides good opportunities for astronomy and astrophysics. The median atmospheric coherence length at the Ethiopian Plateau was 17.7 cm and approximately 75 per cent of the time abo v e 15.6 cm for dry conditions, indicating a very calm atmosphere. Although fa v ourable atmospheric turb ulence conditions at the Ethiopian Plateau were found from the global turbulence model, due to the complete lack of infrastructure it has never been visited, meaning that additional validation experiments are required.