A High‐Altitude Site Survey for SOFIA
A High‐Altitude Site Survey for SOFIA
复制标题
索菲亚高海拔现场勘察
DOI:
10.1086/316132
复制
发表时间:
1998
期刊:
影响因子:
--
通讯作者:
L. Pfister
中科院分区:
文献类型:
--
作者:
M. Haas;L. Pfister
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a modified Boeing 747‐SP equipped with a 2.5 m telescope dedicated to astronomical research. Currently under joint development by the US (NASA) and Germany (DLR), it is scheduled to begin operations in late 2001. The ability of SOFIA to carry out its mission will depend strongly on the meteorological conditions at and above flight altitudes in the vicinity of its home base. The most important meteorological factors are the frequency of high‐altitude clouds and the magnitude of the water vapor overburdens. This paper performs a high‐altitude site survey by gathering together the best available meteorological data, defining metrics, and evaluating them for a variety of sites. These metrics are found to corroborate past airborne experience and to be consistent with well‐known global circulation patterns, convection, and upper tropospheric dynamics. They indicate that there are significant variations in the weather at SOFIA flight altitudes. Particularly in summer, some continental US sites are shown to be worse than Hawaii, where high‐altitude cirrus clouds and the associated moisture have historically caused significant losses in the amount and quality of the astronomical data collected by NASA's Kuiper Airborne Observatory. SOFIA's planned home base, Moffett Field, CA, is found to have excellent high‐altitude weather and to be one of the best continental US sites.