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Effective Area of the Antenna of the RT-22 CrAO RI Radio Telescope

机译:RT-22 CrAO RI射电望远镜天线的有效面积

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摘要

Based on the results of calibrator observations at 13.5-mm and 8.2-mm wavelengths in 1985 and 2005, the dependence of the effective area of the RT-22 CrAO RI antenna on ambient temperature and elevation was determined. The obtained results confirm a high quality of the RT-22 antenna at millimeter wavelengths. A high accuracy of the reflector surface makes it possible to observe at millimeter wavelengths right to 2 mm. At 8.2-mm wavelength, the effective area changes by no more than 5% when the antenna is reinstalled from the zenith to 15° elevation angle. Large antennas, intended to operate at maximum frequencies, should be built either taking into account the climatic conditions of the antenna sites or taking measures to provide thermal stability of the antenna.
机译:根据1985年和2005年在13.5mm和8.2mm波长处的校准器观测结果,确定了RT-22 CrAO RI天线的有效面积与环境温度和海拔的相关性。所得结果证实了RT-22天线在毫米波长下的高质量。反射器表面的高精度使得可以在毫米波长至2 mm的范围内观察。在8.2毫米波长处,将天线从天顶重新安装到15°仰角时,有效面积变化不超过5%。应考虑天线位置的气候条件或采取措施以提供天线的热稳定性,建造旨在以最大频率工作的大型天线。

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