Investigations to extend the lower frequency limit of reverberation chambers

Author(s):  
M.O. Hatfield ◽  
M.B. Slocum ◽  
E.A. Godfrey ◽  
G.J. Freyer
1965 ◽  
Vol 23 ◽  
pp. 357-362
Author(s):  
T. R. Hartz

Solar radio noise in the frequency range 1.5 to 10 MHz appears sporadically in the Alouette sweep-frequency recordings above the galactic noise level. The type III bursts can be readily identified, but other spectral types are much more difficult to identify from only the satellite records. Using a plausible model for the coronal electron densities, the Type III frequency drift curves have been interpreted as corresponding to a source velocity in the range 0.1 to 0.15 times the velocity of light. Preliminary estimates have also been made of the coronal temperatures from some of the burst durations.Other solar noise events of longer duration have not been classified other than as enhanced solar noise at this stage. These enhancements frequently show an intensity structure, extending down to the 1.5 MHz lower frequency limit of the equipment. These events are discussed briefly.


1982 ◽  
Vol 36 (4) ◽  
pp. 390-393 ◽  
Author(s):  
L. A. Carreira ◽  
R. Nelson ◽  
M. L. Horovitz ◽  
L. Azarraga

A scanning algorithm for condensed-phase CARS and folded BOXCARS along with the necessary optical alignment hardware for folded BOXCARS have been developed. Due to the unique geometry of the folded BOXCARS beams, the CARS signal is sufficiently isolated from the pump and Stokes beams such that extended spectra with a lower frequency limit of 70 cm−1 have been obtained.


1987 ◽  
Vol 41 (7) ◽  
pp. 1142-1144 ◽  
Author(s):  
F. Devlin ◽  
P. J. Stephens

The development of dispersive instrumentation for the measurement of vibrational circular dichroism (VCD) with a lower frequency limit of ∼650 cm−1 is reported. VCD spectra of 3-methylcyclohexanone, α-pinene, and 3-bromocamphor in the frequency range of 800 to 650 cm−1 are presented to illustrate instrumental performance. The spectra obtained are superior to earlier spectra obtained with the use of a Fourier transform spectrometer.


1971 ◽  
Vol 36 (4) ◽  
pp. 527-537 ◽  
Author(s):  
Norman P. Erber

Two types of special hearing aid have been developed recently to improve the reception of speech by profoundly deaf children. In a different way, each special system provides greater low-frequency acoustic stimulation to deaf ears than does a conventional hearing aid. One of the devices extends the low-frequency limit of amplification; the other shifts high-frequency energy to a lower frequency range. In general, previous evaluations of these special hearing aids have obtained inconsistent or inconclusive results. This paper reviews most of the published research on the use of special hearing aids by deaf children, summarizes several unpublished studies, and suggests a set of guidelines for future evaluations of special and conventional amplification systems.


2021 ◽  
Author(s):  
Wei Huang ◽  
Lifei Zhang ◽  
Xiaogang Wu ◽  
Chengxiang Li ◽  
Jie Zhang ◽  
...  

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