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用于绘制宇宙背景辐射的辐射计系统。

Radiometer system to map the cosmic background radiation.

作者信息

Gorenstein M V, Muller R A, Smoot G F, Tyson J A

机构信息

University of California, Lawrence Berkeley Laboratory and Space Sciences Laboratory, Berkeley, CA 94720, USA.

出版信息

Rev Sci Instrum. 1978 Apr;49(4):440. doi: 10.1063/1.1135445.

Abstract

We have developed a 33-GHz airborne radiometer system to map large angular scale variations in the temperature of the 3 K cosmic background radiation. A ferrite circulator switches a room-temperature mixer between two antennas pointing 60 degrees apart in the sky. In 40 min of observing, the radiometer can measure the anisotropy of the microwave background with an accuracy of +/-1 mK rms, or about 1 part in 3000 of 3 K. The apparatus is flown in a U-2 jet to 20 km altitude where 33-GHz thermal microwave emission from the atmosphere is at a low level. A second radiometer, tuned to 54 GHz near oxygen emission lines, monitors spurious signals from residual atmospheric radiation. The antennas, which have an extremely low side-lobe response of less than -65 dB past 60 degrees , reject anisotropic radiation from the earth's surface. Periodic interchange of the antenna positions and reversal of the aircraft's flight direction cancel equipment-based imbalances. The system has been operated successfully in U-2 aircraft flown from NASA-Ames at Moffett Field, CA.

摘要

我们研制了一种33吉赫兹机载辐射计系统,用于绘制3K宇宙背景辐射温度的大角度尺度变化图。一个铁氧体环行器在指向天空中相距60度的两个天线之间切换一个室温混频器。在40分钟的观测中,该辐射计能够以均方根误差±1毫开尔文的精度测量微波背景的各向异性,约为3K的三千分之一。该仪器搭载在U-2喷气式飞机上飞行至20千米的高空,在那里来自大气的33吉赫兹热微波辐射处于低水平。另一个调谐到靠近氧发射线的54吉赫兹的辐射计,监测来自残余大气辐射的杂散信号。天线在60度以外具有低于-65分贝的极低旁瓣响应,可抑制来自地球表面的各向异性辐射。天线位置的定期互换和飞机飞行方向的反转消除了基于设备的不平衡。该系统已在从加利福尼亚州莫菲特场的美国国家航空航天局艾姆斯研究中心起飞的U-2飞机上成功运行。

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