1.8V Power Suppy 16MBIT-MRAM with 40% Array Efficiency

Author(s):  
H. Yoda ◽  
T. Kai ◽  
Y. Iwata ◽  
S. Ikegawa ◽  
K. Tsuchida ◽  
...  
Keyword(s):  
2020 ◽  
Vol 1618 ◽  
pp. 062044
Author(s):  
Javier Sanz Rodrigo ◽  
Fernando Borbón Guillén ◽  
Pedro M. Fernandes Correia ◽  
Bibiana García Hevia ◽  
Wolfgang Schlez ◽  
...  

2006 ◽  
Vol 42 (10) ◽  
pp. 2724-2726 ◽  
Author(s):  
H. Yoda ◽  
T. Kai ◽  
T. Inaba ◽  
Y. Iwata ◽  
N. Shimomura ◽  
...  

2005 ◽  
Vol 23 (9) ◽  
pp. 3111-3113 ◽  
Author(s):  
P. Tříska ◽  
A. Czapek ◽  
J. Chum ◽  
F. Hruška ◽  
J. Šimůnek ◽  
...  

Abstract. Data on solar array efficiency measured on board two Czech MAGION micro-satellites between August 1995 and June 2002, during the period of increasing and high solar activity, were used to study the space weather effects on photo-voltaic solar cells. A stronger degradation of the solar array was observed on MAGION-5 in comparison with MAGION-4. This fact can be explained by the essential difference between the two orbits. The MAGION-5 s/c was in the radiation belts more than 40% of the time, whereas the MAGION-4 was only present about 4% of the time. The experimental data refer to periods of low as well as high solar activity, with an enhanced occurrence of strong solar events. The evaluation of the data set covering a period of more than 6 years has shown that solar proton flares can have an almost immediate effect on the solar array efficiency. However, in the case of MAGION-5, an important role in solar cell degradation is played by the long-term effect of energetic particles in the radiation belts. Periods with a distinctly steeper decrease in the solar array output power were observed and can be explained by an increase of particle flux density in the radiation belts. Periods in slower decline of the solar array output power correspond to periods in low radiation belt indices based on the NOAA POES s/c data.


2020 ◽  
Vol 2020 (3) ◽  
Author(s):  
A.V. Blank ◽  
◽  
S.D. Bogdanov ◽  
N.A. Suhareva ◽  
◽  
...  

2017 ◽  
Vol 37 (11) ◽  
pp. 4053-4064 ◽  
Author(s):  
Kim C. Nguyen ◽  
Jack J. Katzfey ◽  
John Riedl ◽  
Alberto Troccoli

Energies ◽  
2021 ◽  
Vol 14 (4) ◽  
pp. 892
Author(s):  
Jérôme Thiébot ◽  
Nasteho Djama Dirieh ◽  
Sylvain Guillou ◽  
Nicolas Guillou

Assessing the efficiency of a tidal turbine array is necessary for adequate device positioning and the reliable evaluation of annual energy production. Array efficiency depends on hydrodynamic characteristics, operating conditions, and blockage effects, and is commonly evaluated by relying on analytical models or more complex numerical simulations. By applying the conservations of mass, momentum, and energy in an idealized flow field, analytical models derive formulations of turbines’ thrust and power as a function of the induction factor (change in the current velocity induced by turbines). This simplified approach also gives a preliminary characterization of the influence of blockage on array efficiency. Numerical models with turbines represented as actuator disks also enable the assessment of the efficiency of a tidal array. We compare here these two approaches, considering the numerical model as a reference as it includes more physics than the analytical models. The actuator disk approach is applied to the three-dimensional model Telemac3D in realistic flow conditions and for different operating scenarios. Reference results are compared to those obtained from three analytical models that permit the investigation of the flow within tidal farm integrating or excluding processes such as the deformation of the free surface or the effects of global blockage. The comparison is applied to the deployment of a fence of turbines in the Alderney Race (macro-tidal conditions of the English Channel, northwest European shelf). Efficiency estimates are found to vary significantly from one model to another. The main result is that analytical models predict lower efficiency as they fail to approach realistically the flow structure in the vicinity of turbines, especially because they neglect the three-dimensional effects and turbulent mixing. This finding implies that the tidal energy yield potential could be larger than previously estimated (with analytical models).


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