WASABI: Framework for Real-Time Speech Analysis Applications (Demo)

2002 ◽  
pp. 105-108
Author(s):  
Eric W. Brown ◽  
Anni R. Coden
Keyword(s):  
Real Time ◽  
Speech Analysis

A Single Chip Digital Signal Processor and Its Application to Real-Time Speech Analysis

1983 ◽  
Vol 18 (1) ◽  
pp. 91-99 ◽  
Author(s):  
Y. Hagiwara ◽  
Y. Kita ◽  
T. Miyamoto ◽  
Y. Toba ◽  
H. Hara ◽  
...  
Keyword(s):  
Real Time ◽  
Digital Signal Processor ◽  
Digital Signal ◽  
Speech Analysis ◽  
Single Chip ◽  
Signal Processor

Comparison of Real-Time Speech Magnetic Resonance Imagings With Perceptual Speech Analysis in Evaluation Velopharyngeal Sphincter Function

2021 ◽  
Vol Publish Ahead of Print ◽  
Author(s):  
Tugba Feryal Yildiz-Deger ◽  
Fatih Cinar ◽  
Semih Baghaki ◽  
Anil Demiroz ◽  
Zahra Polat ◽  
...  
Keyword(s):  
Magnetic Resonance ◽  
Real Time ◽  
Speech Analysis ◽  
Sphincter Function

A single chip digital signal processor and its application to real-time speech analysis

1983 ◽  
Vol 31 (1) ◽  
pp. 339-346 ◽  
Author(s):  
Y. Hagiwara ◽  
Y. Kita ◽  
T. Miyamoto ◽  
Y. Toba ◽  
H. Hara ◽  
...  
Keyword(s):  
Real Time ◽  
Digital Signal Processor ◽  
Digital Signal ◽  
Speech Analysis ◽  
Single Chip ◽  
Signal Processor

Some Recent Results in Quiescent Prominence Spectrometry

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman
Keyword(s):  
Real Time ◽  
Computer System ◽  
Spectral Response ◽  
Absolute Intensity ◽  
Solar Observatory ◽  
Target Size ◽  
Small Target ◽  
Signal Averaging ◽  
Quiescent Prominence

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.

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