scholarly journals A Glimpse of the Initial Conditions for the Development of Science and Technology and Soviet Specialists in the PRC: 1949–1955

2021 ◽  
Vol 5 (2) ◽  
pp. 141-160
Author(s):  
Yuri M. BATURIN 尤里·M. 巴图林
Keyword(s):  
Initial Conditions ◽  
Science And Technology

scholarly journals An Efficient Numerical Technique for the Nonlinear Fractional Kolmogorov–Petrovskii–Piskunov Equation

Mathematics ◽  
2019 ◽  
Vol 7 (3) ◽  
pp. 265 ◽  
Author(s):  
Pundikala Veeresha ◽  
Doddabhadrappla Prakasha ◽  
Dumitru Baleanu
Keyword(s):  
Numerical Simulations ◽  
Convergence Analysis ◽  
Initial Conditions ◽  
Numerical Technique ◽  
Science And Technology ◽  
Elliptic Functions ◽  
Jacobi Elliptic Functions ◽  
Transform Method ◽  
Homotopy Analysis ◽  
Frame Work

The q -homotopy analysis transform method ( q -HATM) is employed to find the solution for the fractional Kolmogorov–Petrovskii–Piskunov (FKPP) equation in the present frame work. To ensure the applicability and efficiency of the proposed algorithm, we consider three distinct initial conditions with two of them having Jacobi elliptic functions. The numerical simulations have been conducted to verify that the proposed scheme is reliable and accurate. Moreover, the uniqueness and convergence analysis for the projected problem is also presented. The obtained results elucidate that the proposed technique is easy to implement and very effective to analyze the complex problems arising in science and technology.

Laboratory Simulation of Lunar Luminescence

1962 ◽  
Vol 14 ◽  
pp. 441-444 ◽  
Author(s):  
J. E. Geake ◽  
H. Lipson ◽  
M. D. Lumb
Keyword(s):  
Science And Technology ◽  
Laboratory Simulation ◽  
The Moon ◽  
Physics Department ◽  
Luminescent Spectrum

Work has recently begun in the Physics Department of the Manchester College of Science and Technology on an attempt to simulate lunar luminescence in the laboratory. This programme is running parallel with that of our colleagues in the Manchester University Astronomy Department, who are making observations of the luminescent spectrum of the Moon itself. Our instruments are as yet only partly completed, but we will describe briefly what they are to consist of, in the hope that we may benefit from the comments of others in the same field, and arrange to co-ordinate our work with theirs.

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