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Дата публикацииНазваниеАвторы
2022The burst mode of accretion in massive star formation with stellar inertiaMeyer, D. M. -A.; Vorobyov, E. I.; Elbakyan, V. G.; Kraus, S.; Liu, S. -Y.; Nayakshin, S.; Sobolev, A. M.
2019Calculation of linear induction motor features by detailed equivalent circuit method taking into account non-linear electromagnetic and thermal propertiesSmolyanov, I.; Sarapulov, F.; Tarasov, F.
2015Calculations of wind mass transfer of pollution: Simulation and analytical modelsBerg, D. B.; Gubarev, S. V.; Medvedev, A. N.; Taubayev, A. A.
2020Collective magnetic fluctuations in Hubbard plaquettes captured by fluctuating local field methodRubtsov, A. N.; Stepanov, E. A.; Lichtenstein, A. I.
2016Controlled time integration for the numerical simulation of meteor radar reflectionsRäbinä, J.; Mönkölä, S.; Rossi, T.; Markkanen, J.; Gritsevich, M.; Muinonen, K.
2020Convergence and stability estimates in difference setting for time-fractional parabolic equations with functional delayHendy, A. S.; Pimenov, V. G.; Macías-Díaz, J. E.
2018Design of reinforced concrete structures in the early stages of construction taking into account heat dissipation of concreteRedikultsev, E. A.; Belyaeva, Z. V.
2020Detection of the Lowest-Lying Odd-Parity Atomic Levels in ActiniumZhang, K.; Studer, D.; Weber, F.; Gadelshin, V. M.; Kneip, N.; Raeder, S.; Budker, D.; Wendt, K.; Kieck, T.; Porsev, S. G.; Cheung, C.; Safronova, M. S.; Kozlov, M. G.
2013A difference scheme for the numerical solution of an advection equation with aftereffectSolodushkin, S. I.
2021Direct estimation of SIR model parameters through second-order finite differencesMedvedeva, M.; Simos, T. E.; Tsitouras, C.; Katsikis, V.
2019Effect of particle diameter and packing density on heating of metallic iron particles in alternating magnetic fieldKrekhno, R. V.; Safronov, A. P.; Beketov, I. V.
2021Efficient HIE-FDTD method for designing a dual-band anisotropic terahertz absorption structureZhou, Y.; Li, H.; Li, L.; Cai, Y.; Zeyde, K.; Han, X.
2022Evolution of the dust trail of comet 17P/HolmesGritsevich, M.; Nissinen, M.; Oksanen, A.; Suomela, J.; Silber, E. A.
2022FEM-based time-reversal technique for an ultrasonic cleaning applicationTommiska, O.; Mustonen, J.; Moilanen, P.; Rauhala, T.; Gritsevich, M.; Salmi, A.; Hæggström, E.
2018First scattered light detection of a nearly edge-on transition disk around the T Tauri star RY LupiLanglois, M.; Pohl, A.; Lagrange, A. -M.; Maire, A. -L.; Mesa, D.; Boccaletti, A.; Gratton, R.; Denneulin, L.; Klahr, H.; Vigan, A.; Benisty, M.; Dominik, C.; Bonnefoy, M.; Menard, F.; Avenhaus, H.; Cheetham, A.; Van, Boekel, R.; De, Boer, J.; Chauvin, G.; Desidera, S.; Feldt, M.; Galicher, R.; Ginski, C.; Girard, J. H.; Henning, T.; Janson, M.; Kopytova, T.; Kral, Q.; Ligi, R.; Messina, S.; Peretti, S.; Pinte, C.; Sissa, E.; Stolker, T.; Zurlo, A.; Magnard, Y.; Blanchard, P.; Buey, T.; Suarez, M.; Cascone, E.; Moller-Nilsson, O.; Weber, L.; Petit, C.; Pragt, J.
2013Heat transfer under high-power heating of liquids. 1. Experiment and inverse algorithmRutin, S. B.; Smotritskiy, A. A.; Starostin, A. A.; Okulovsky, Y. S.; Skripov, P. V.
2019Hydrodynamical Simulation of Astrophysical Flows: High-Performance GPU ImplementationAkimova, E.; Misilov, V.; Kulikov, I.; Chernykh, I.
2023Improving agricultural efficiency with solar-powered tractors and magnetohydrodynamic entropy generation in copper–silver nanofluid flowObalalu, A. M.; Alqarni, M. M.; Odetunde, C.; Memon, M. A.; Olayemi, O. A.; Shobo, A. B.; Mahmoud, E. E.; Ali, M. R.; Sadat, R.; Hendy, A. S.
2019Increase of Transient Stability Level of Gas Turbine Power Plant Using FACTSSolodyankin, S.; Pazderin, A.
2021Influence of gas flow turbulence scale on heat exchange intensity in a long smooth pipeNevolin, A. M.; Osipov, L. E.; Plotnikov, L. V.