Compact low-noise pulse generating lasers with repetition rates of 10 to 50 GHz

2006 ◽  
pp. 21-36
Author(s):  
G. J. Spühler ◽  
L. Krainer ◽  
S. C. Zeller ◽  
Ch. Erny ◽  
R. Paschotta ◽  
...  
Keyword(s):  
Low Noise ◽  
Noise Pulse

Compact low-noise pulse generating lasers with repetition rates of 10 to 50 GHz

2005 ◽  
Vol 15 (03) ◽  
pp. 497-512 ◽  
Author(s):  
G. J. Spühler ◽  
L. Krainer ◽  
S. C. Zeller ◽  
Ch. Erny ◽  
R. Paschotta ◽  
...  
Keyword(s):  
Wavelength Division Multiplexing ◽  
Time Domain ◽  
Fundamental Mode ◽  
Low Noise ◽  
Noise Pulse ◽  
Wavelength Division ◽  
Optical Time Division Multiplexing ◽  
Optical Time ◽  
The Time Domain ◽  
Time Division

We review the main results obtained with our recently introduced passively fundamental mode-locked Er : Yb :glass lasers mainly in the context of telecom applications, and we discuss their key enablers. Specifically, we focus on the aspects of the lasers for application in the time-domain for optical time-division multiplexing and in the wavelength domain for dense wavelength-division-multiplexing.

Low Noise Pulse Polarograph Suitable for Automation

1974 ◽  
Vol 5 (4) ◽  
pp. 257-270 ◽  
Author(s):  
B. H. Vassos ◽  
R. A. Osteryoung
Keyword(s):  
Low Noise ◽  
Noise Pulse

scholarly journals A low-power CMOS ASIC for X-ray Silicon Drift Detectors low-noise pulse processing

2014 ◽  
Vol 9 (03) ◽  
pp. C03036-C03036 ◽  
Author(s):  
M Ahangarianabhari ◽  
G Bertuccio ◽  
D Macera ◽  
P Malcovati ◽  
M Grassi ◽  
...  
Keyword(s):  
Low Power ◽  
Low Noise ◽  
Noise Pulse ◽  
X Ray ◽  
Pulse Processing ◽  
Low Power Cmos ◽  
Silicon Drift Detectors

scholarly journals Ultrasound detection via low-noise pulse interferometry using a free-space Fabry-Pérot

2018 ◽  
Vol 26 (17) ◽  
pp. 22405 ◽  
Author(s):  
Oleg Volodarsky ◽  
Yoav Hazan ◽  
Amir Rosenthal
Keyword(s):  
Free Space ◽  
Low Noise ◽  
Noise Pulse ◽  
Fabry Perot

Development of a Low Noise Pulse Combustor

1987 ◽  
Vol 52 (1-3) ◽  
pp. 107-119 ◽  
Author(s):  
ISAO INUI ◽  
KENJI OKAMOTO ◽  
MITSUYOSHI NAKAMOTO ◽  
MASATO HOSAKA
Keyword(s):  
Low Noise ◽  
Noise Pulse ◽  
Pulse Combustor

Distribution of R- and S-Process Elements in the Galactic Halo

1988 ◽  
Vol 132 ◽  
pp. 501-506
Author(s):  
C. Sneden ◽  
C. A. Pilachowski ◽  
K. K. Gilroy ◽  
J. J. Cowan
Keyword(s):  
Heavy Element ◽  
Galactic Halo ◽  
Low Noise ◽  
Heavy Elements ◽  
Process Synthesis ◽  
Element Abundances ◽  
Halo Stars ◽  
Abundance Patterns ◽  
R Process ◽  
Process Elements

Current observational results for the abundances of the very heavy elements (Z>30) in Population II halo stars are reviewed. New high resolution, low noise spectra of many of these extremely metal-poor stars reveal general consistency in their overall abundance patterns. Below Galactic metallicities of [Fe/H] Ã −2, all of the very heavy elements were manufactured almost exclusively in r-process synthesis events. However, there is considerable star-to-star scatter in the overall level of very heavy element abundances, indicating the influence of local supernovas on element production in the very early, unmixed Galactic halo. The s-process appears to contribute substantially to stellar abundances only in stars more metal-rich than [Fe/H] Ã −2.

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