Radiometer system to map the cosmic background radiation.
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.
Gorenstein
M V
MV
University of California, Lawrence Berkeley Laboratory and Space Sciences Laboratory, Berkeley, CA 94720, USA.
Muller
R A
RA
Smoot
G F
GF
Tyson
J A
JA
D000401:Aircraft / Q000295:instrumentation*; D003359:Cosmic Radiation; D004867:Equipment Design; D019544:Equipment Failure Analysis; D008872:Microwaves; D011834:Radiation Monitoring / Q000295:instrumentation* / Q000379:methods; D015203:Reproducibility of Results; D012680:Sensitivity and Specificity