scholarly journals Inter-channel uniformity of a microwave sounder in space

2018 ◽  
Vol 11 (7) ◽  
pp. 4005-4014 ◽  
Author(s):  
Martin Burgdorf ◽  
Imke Hans ◽  
Marc Prange ◽  
Theresa Lang ◽  
Stefan A. Buehler

Abstract. We analyzed intrusions of the Moon in the deep space view of the Advanced Microwave Sounding Unit-B on the NOAA-16 satellite and found no significant discrepancies in the signals from the different sounding channels between 2001 and 2008. However, earlier investigations had detected biases of up to 10 K, by using simultaneous nadir overpasses of NOAA-16 with other satellites. These discrepancies in the observations of Earth scenes cannot be due to non-linearity of the receiver or contamination of the deep space view without affecting the signal from the Moon as well. As neither major anomalies of the on-board calibration target nor the local oscillator were present, we consider radio frequency interference in combination with a strongly decreasing gain the most obvious reason for the degrading photometric stability. By means of the chosen example we demonstrate the usefulness of the Moon for investigations of the performance of microwave sounders in flight.

2017 ◽  
Author(s):  
Martin Burgdorf ◽  
Imke Hans ◽  
Marc Prange ◽  
Theresa Lang ◽  
Stefan A. Buehler

Abstract. We analyzed intrusions of the Moon in the deep space view of the Advanced Microwave Sounding Unit-B on the NOAA-16 satellite and found no significant discrepancies in the signals from the different sounding channels between 2001 and 2008. Earlier investigations, however, had detected biases of up to 10 K by using simultaneous nadir overpasses of NOAA-16 with other satellites. These discrepancies in the observations of Earth scenes cannot be due to non-linearity of the receiver or contamination of the deep space view without affecting the signal from the Moon as well. As major anomalies of the on-board calibration target and frequency shifts of the local oscillator were not present, either, the most obvious reason for the degrading photometric stability is radio frequency interference in combination with a strongly decreasing gain. By means of the chosen example we demonstrate the usefulness of the Moon for investigations of the performance of microwave sounders in flight.


Author(s):  
Kristian Zarb Adami ◽  
I. O. Farhat

This work sketches a possible design architecture of a low-frequency radio interferometer located on the lunar surface. The design has evolved from single antenna experiments aimed at the global signal detection of the epoch of reionization (EoR) to the square kilometre array (SKA) which, when complete, will be capable of imaging the highly red-shifted H 1 -signal from the cosmic dawn through to the EoR. However, due to the opacity of the ionosphere below 10 MHz and the anthropogenic radio-frequency interference, these terrestrial facilities are incapable of detecting pre-ionization signals and the moon becomes an attractive location to build a low-frequency radio interferometer capable of detecting such cosmological signals. Even though there are enormous engineering challenges to overcome, having this scientific facility on the lunar surface also opens up several new exciting possibilities for low-frequency radio astronomy. This article is part of a discussion meeting issue ‘Astronomy from the Moon: the next decades’.


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