Titlebook: Neural Networks and Learning Algorithms in MATLAB; Ardashir Mohammadazadeh,Mohammad Hosein Sabzalian, Book 2022 The Editor(s) (if applicab

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Ardashir Mohammadzadeh,Mohammad Hosein Sabzalian,Oscar Castillo,Rathinasamy Sakthivel,Fayez F. M. El-sponsored events. Summer Schools at Belgerati, Italy in 1972 and Ajaccio, Corsica in 1975 on the topic of "Solid­ -State IOllics" dealt with fundamental aspects of solid-state electro­ chemistry and materials science. The application of specific solid ionic conductors played a significant role in t

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Ardashir Mohammadzadeh,Mohammad Hosein Sabzalian,Oscar Castillo,Rathinasamy Sakthivel,Fayez F. M. Eland development of materials, techniques, and theoretical approaches. This science is one of the great triumphs of the second part of the 20th century. For nearly a century, development of materials for solid-state ionic technology has been restricted. During the last two decades there have been rem

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on instrumentation and per­ sonell is also low. These properties are examined and the necessary conditions are discussed (Chapter 1) as are the analytical tasks (Chapter 6) for which use of this method is advantageous. Other features that are often overlooked are just as important: The simplicity o

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Ardashir Mohammadzadeh,Mohammad Hosein Sabzalian,Oscar Castillo,Rathinasamy Sakthivel,Fayez F. M. Elture pattern may be characteristic for a given species and thus a match of laboratory and observational profile may be a sufficient argument to identify a known molecule as a DIB carrier. It is emphasized that a criterion of identification must meet the requirements of both: experimentalists and obs

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Ardashir Mohammadzadeh,Mohammad Hosein Sabzalian,Oscar Castillo,Rathinasamy Sakthivel,Fayez F. M. Eles whose major components are very well constrained. Lastly, the signature of carbon-rich polycyclic aromatic hydrocarbons (PAHs), shockingly large molecules by earlier interstellar chemistry standards, is widespread throughout the Universe. This paper presents a detailed summary of these disparate

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Ardashir Mohammadzadeh,Mohammad Hosein Sabzalian,Oscar Castillo,Rathinasamy Sakthivel,Fayez F. M. Elar the centre of the nebula by the pressure of the Lα light surrounding the globule, but in the early evolution of the nebula particles can escape into the ionized medium when fronts are R-type. Ice grains escaping at this time will be destroyed for distances to the exciting stars less than 1 pc. Th