... The experimental study of magnetic ordering, magnetoelastic, magnetocaloric and galvanomagnetic effects, exchange and magnetocrystalline interactions in rare earth metals, alloys and compounds. ... the Divisions of chemistry and physics of high pressures of the chemical faculty MSU; . ... Tver' State University . ... The effect of rare earth sublattice on magnetic anisotropy in these compounds has been determined. The magnetic order in R(Fe,Co)(Si,Ge) compounds has been investigated. ...

Еще в разделе: (Показать все результаты (>14) - ferro.phys.msu.ru/ )

• Laboratory of Ferroelectricity
• Department of General Physics and magneto-ordered matter. Physics Department of

Problems for Ultrahyperbolic Equations in Half-Space Prof. Dmitry P. Kostomarov Faculty of Computational Mathematics and Cybernetics Lomonosov Moscow State University Pontryagin Anniversary Conference June 17ґ22, 2008 , Moscow, Russia Section Differential Equations Subsection Partial Differential Equations Prof. D.P. Kostomarov (CMC MSU) Problems for Ultrahyperbolic Equations June 22, ... June 22, 2008 (2.13) Problems for Ultrahyperbolic Equations 16 / 23 2.2. ...

Еще в разделе: (Показать все результаты (>10) - ani.cmc.msu.ru/ )

... Инновационная . структура МГУ . ... деятельности . ... Process of Forming a Company . ... Finance for Start-Up . ... In the commercial world, the business manager (entrepreneur, Chief Executive Officer (CEO), Chief Operating Officer (COO):) must create the infrastructure and face many issues specific to the establishment and development of a new company. ... 2005 Управление инновационной политики . и организации инновационной деятельности . МГУ им. М.В. Ломоносова . ...

Еще в разделе: (Показать все результаты (>19) - innovation.msu.ru/ )

... Earlier still lies the remaining frontier, where the first stars, galaxies and massive black holes formed. ... Building on this general framework, and relying on the development of efficient new computational tools, the fragmentation properties of primordial gas inside such minihaloes were investigated with numerical simulations, leading to the result that the first stars, so-called population III, were predominantly very massive4,8 (see Box 1 for the terminology used here). ... Astrophys. ... III. ...

Еще в разделе: (Показать все результаты (>12) - ocean.phys.msu.ru/ )

• http://ocean.phys.msu.ru/courses/stathyd/2001%20Ferrari%20et%20al.%2C%20The%20temperature-salinity%20relationship%20of%20the%20mixed%20layer.pdf
• http://ocean.phys.msu.ru/courses/geo/lectures-addons/04/1896%20Arrhenius.pdf
• http://ocean.phys.msu.ru/courses/stathyd/2005%20Smyth%20et%20al.%2C%20Differential%20diffusion%20in%20breaking%20Kelvin-Helmholtz%20billows.pdf

... These spectral characteristics compare with introduction (ВВЕДЕНИЕ) At last time many workers have studied thermal Rayleigh-Benard convection using numerical At last time many workers have studied thermal Rayleigh- Benard convection using numerical time many At last time many workers have studied thermal Rayleigh-Benard convection using numerical used spectral methods with periodic boundary conditions. ... In numerical simulations were derived secondary stationary, [pic] where ? ...

Еще в разделе: (Показать все результаты (>25) - hit-conf.imec.msu.ru/ )

• http://hit-conf.imec.msu.ru/2006/CD/Palymskiy2.doc
• http://hit-conf.imec.msu.ru/books/NeZaTeGiUs_2010.pdf
• http://hit-conf.imec.msu.ru/2006/CD/Palymskiy2.pdf

... An extended set of observables of the nuclear quasi-free (p, d + ) reaction including the triple differential cross-section for coincidence measurements, its analyzing power in case of polarized proton beams and, also, the parameters of the polarization of the excited recoil nucleus and the produced deuteron are considered in the framework of the distorted-wave impulse approximation using the reaction 16 O(p, d + )15 N at a proton energy of 650 MeV as an example. ...

227. http://sun.sai.msu.ru/texts/somov-1-10Lect.pdf

228. Курс АиАЯ | Страница поддержки курса "Алгоритмы и алгоритмические языки" для 1

---

Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда