scholarly journals Improving Signal to Noise Ratios in Ion Mobility Spectrometry and Structures for Lossless Ion Manipulations (SLIM) using a High Dynamic Range Analog-to-Digital Converter

Author(s):  
Adam L. Hollerbach ◽  
Cameron M. Giberson ◽  
Joon-Yong Lee ◽  
Adam P. Huntley ◽  
Richard D. Smith ◽  
...  
2014 ◽  
Vol 23 (06) ◽  
pp. 1450090 ◽  
Author(s):  
ARASH ESMAILI ◽  
HADISEH BABAZADEH ◽  
KHAYROLLAH HADIDI ◽  
ABDOLLAH KHOEI

A 13-bit analog-to-digital converter (ADC) is designed in 0.35 μm CMOS technology that reduces the power consumption through sharing the resources between pipeline stages. Using a dummy sample-and-hold (S/H) and recirculating concept the requirements for the first stage are relaxed and the design restrictions are resolved. This ADC does not use a dedicated S/H and reaches a speed of 50 MS/s. The design is tested with TSMC mixed-signal 0.35 μm technology and post layout simulations shows over 75 dB Signal-to-Noise and Distortion-Ratio (SNDR) and over 85 dB Spurious Free Dynamic Range (SFDR) at the Nyquist frequency. The designed chip occupies an area of 1.3 mm–0.7 mm and consumes 164 mW power at Nyquist from a 3.3 V supply.


1999 ◽  
Vol 9 (2) ◽  
pp. 3157-3160 ◽  
Author(s):  
A. Hodge Worsham ◽  
D.L. Miller ◽  
P.D. Dresselhaus ◽  
A.H. Miklich ◽  
J.X. Przybysz

Energies ◽  
2019 ◽  
Vol 12 (23) ◽  
pp. 4567
Author(s):  
Mfana ◽  
Hasan ◽  
Ali

Digitization is at the center of fourth industrial revolution (4IR) with previously analog systems being digitized through an analog-to-digital converter. In addition, 4IR applications such as fifth generation (5G) Cellular Networks Technology and Cognitive Electronic Warfare (EW) at some point interface digitally through an analog-to-digital converter. Efficient use of digital resources such as memory, largely depends on the signal sampling design of analog-to-digital converters. Existing even order sampling has been found to perform better than traditional sampling techniques. Research on the efficiency of a digital interface with a 4IR platform is still in its infancy. This paper presents a performance study of three sampling techniques: the proposed new and novel odd/even order sampling architecture, existing Mod-∆, and traditional 1st order delta-sigma, to address this. Step-size signal-to-noise (SNR), dynamic range, and sampling frequency are also studied. It was found that the proposed new and novel odd/even order sampling achieved an SNR performance of 6 dB in comparison to 18 dB for Mod-∆. Sampling frequency findings indicated that the proposed new and novel odd/even order sampling achieved a sampling frequency of 2 kHz in comparison to 8 kHz from a traditional 1st order sigma-delta. Dynamic range findings indicated that the proposed odd/even order sampling has achieved a dynamic range of 1.088 volts/ms in comparison to 1.185 volts/ms from a traditional 1st order sigma-delta. Findings have indicated that the proposed odd/even order sampling has superior SNR and sampling frequency performances, while the dynamic range is reduced by 8%.


2003 ◽  
Vol 211 ◽  
pp. 487-496 ◽  
Author(s):  
A. T. Tokunaga ◽  
C. Ftaclas ◽  
J. R. Kuhn ◽  
P. Baudoz

General arguments for optimized coronagraphy in the search for planets are presented. First, off-axis telescopes provide the best telescopic platforms for use with coronagraphy, and telescope fabrication technology now allows the fabrication of such telescopes with diameters of up to 6.5 m. We show that in certain circumstances a smaller telescope with an off-axis primary has a signal-to-noise advantage compared with larger Cassegrain telescopes. Second, to fully exploit the advantages of the coronagraph for suppressing stray light, it is necessary to use a high Strehl ratio adaptive optics system. This can be best achieved initially with modest aperture telescopes of 3–4 m in diameter. Third, application of simultaneous differential imaging and simultaneous polarimetric techniques are required to reach the photon-limit of coronagraphic imaging. These three developments, if pursued together, will yield significant improvements in the search for planets.


2009 ◽  
Vol 19 (3) ◽  
pp. 670-675 ◽  
Author(s):  
A. Inamdar ◽  
S. Rylov ◽  
A. Talalaevskii ◽  
A. Sahu ◽  
S. Sarwana ◽  
...  

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