Zobrazeno 1 - 10
of 95
pro vyhledávání: '"G Ares de Parga"'
Autor:
M. Ortiz-Domínguez, O. A. Gómez-Vargas, G. Ares de Parga, G. Torres-Santiago, R. Velázquez-Mancilla, V. A. Castellanos-Escamilla, J. Mendoza-Camargo, R. Trujillo-Sánchez
Publikováno v:
Advances in Materials Science and Engineering, Vol 2019 (2019)
An indispensable tool to choose the suitable process parameters for obtaining boride layer of an adequate thickness is the modeling of the boriding kinetics. In this work, two mathematical approaches were used in order to determine the value of activ
Externí odkaz:
https://doaj.org/article/1e27d6051e3b4a278c0f937c5965a077
Autor:
E. Salinas-Hernandez, G. Ares de Parga
Publikováno v:
International Journal of Algebra. 15:265-276
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8264cab97c19412d670abeea2cd98b48
https://doi.org/10.12988/ija.2021.91577
https://doi.org/10.12988/ija.2021.91577
Autor:
Alejandro Esquivel, G. Ares de Parga, Pablo F. Velázquez, Estela Marta Reynoso, Ernesto Matías Schneiter, A. Moranchel-Basurto
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 494:1531-1538
We have performed 3D magnetohydrodynamics (MHD) numerical simulations with the aim of exploring the scenario in which the initial mass distribution of a supernova (SN) explosion is anisotropic. The purpose is to analyse if this scenario can also expl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8ee2fae0172689143fad97ebc0182b3e
https://doi.org/10.1093/mnras/staa627
https://doi.org/10.1093/mnras/staa627
Publikováno v:
SSRN Electronic Journal.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::08378f9dd44c3b46cf14e81c1f30a0f7
https://doi.org/10.2139/ssrn.4264504
https://doi.org/10.2139/ssrn.4264504
Publikováno v:
Physica A: Statistical Mechanics and its Applications. 516:472-479
A deduction of the radiation intensity at see level is deduced by using a semiclassical approach by means of the quantum energy spectrum deduced from the driven damped harmonic oscillator, the ergodic theorem and the mean energy obtained by using the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::907cd6a36e212879c6de9626cf4515ba
https://doi.org/10.1016/j.physa.2018.10.043
https://doi.org/10.1016/j.physa.2018.10.043
Publikováno v:
Journal of Physics: Conference Series. 2307:012063
In this paper, we study the propagation of jets with some characteristics of Type II spicules into the solar corona using a thermomechanical (TM) approximation. Embedding two plasmas with different densities (one representing the chromospheric plasma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c430c66c3ccd8fdb50ed6c7b46ae5ed
https://doi.org/10.1088/1742-6596/2307/1/012063
https://doi.org/10.1088/1742-6596/2307/1/012063
Publikováno v:
Journal of Physics: Conference Series. 2307:012065
We study the possible influence of a magnetic narrow region on the propagation of jets with some characteristics of Type II spicules into the solar corona using MHD approximation numerical simulations. We found that an increase of temperature occurs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01ecb1624d97e0f84e811132e5f4854c
https://doi.org/10.1088/1742-6596/2307/1/012065
https://doi.org/10.1088/1742-6596/2307/1/012065
Publikováno v:
Journal of Physics: Conference Series. 2307:012064
This paper studies Phases 2 and 3 of jets’ propagation with some Type II spicules characteristics into the solar corona using a thermomechanical (TM) approximation. Embedding two plasmas with different densities (one representing the chromospheric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a07f30fbb99879178a97e8da30d8da32
https://doi.org/10.1088/1742-6596/2307/1/012064
https://doi.org/10.1088/1742-6596/2307/1/012064
Publikováno v:
Physica A: Statistical Mechanics and its Applications. 600:127556
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f59014ee63cdf1430cd5335c148b5b4b
https://doi.org/10.1016/j.physa.2022.127556
https://doi.org/10.1016/j.physa.2022.127556
Publikováno v:
Revista Mexicana de Física. 64:187-196
The classical central field is analyzed within the Hammond theory of radiation reaction force. For the attractive Coulomb field, the trajectories deduced from Ford and Hammond equations are numerically obtained. Ford and Hammond equations are rewritt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6bb2afc9879a5a6724e9e578a4b1020d
https://doi.org/10.31349/revmexfis.64.187
https://doi.org/10.31349/revmexfis.64.187