Chlorophyll Fluorescence in vivo : A Theory (Part II). ... The model of carbon assimilation V c ( m M C m -3 s -1 ) by phytoplankton is based on light dependence of photosynthesis , which can be described by a coefficient of underwater radiation absorption by photosynthetic pigments of photosystem II in suspension of microalga a PSP (m -1 ) averaged over the spectral range of underwater radiation, where ... According this assumption the photosynthesis rate is equal to: . ...
... MSU Chamber Orchestra . Concerts of . ... 1999/2000 season: . MOSCOW . ... German Music of XVII c. Johann ROSENMULLER (1620 - 1684) . ... Leontyevsky pereulok, 6 (metro station "Arbatskaya" or "Pushkinskaya") . ... MSU Chamber orchestra . ... Ulitsa Fadeeva, 4 (metro station "Mayakovskaya") . ... Big Hall of Moscow State University (the building at Vorobievy Gory) . ... MSU CHAMBER ORCHESTRA . ... The tickets are in the Moscow State Philarmony office . ... Big Hall of Moscow State University . ...
... Here is a brief outline of the current theory of the events in the early history of the solar system: . A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own gravity. ... The gas cools off enough for the metal, rock and (far enough from the forming star) ice to condense out into tiny particles. (i.e. some of the gas turns back into dust). ... Once the larger of these particles get big enough to have a nontrivial gravity, their growth accelerates. ...
... Sternberg State Astronomical Institute, Moscow, Russia . ... The Sc galaxy NGC 6181 was observed at the 6m telescope of SAO RAS with the scanning Perot-Fabry interferometer in the H-alpha emission line and at the 1m telescope of SAO RAS in BVRI broadband filters with CCD. ... Sil'chenko, O. K. Sternberg State Astronomical Institute, Moscow, Russia . ... COMPLEX FORMATION HISTORY OF LENTICULAR GALAXIES WITH STELLAR COUNTERROTATION: NGC 4138 AND NGC 4550 . ... YOUNG NUCLEI IN DWARF ELLIPTICAL GALAXIES...
ChangeLog for / # # Generated by Trac 0.12.5 # 04/11/16 21:51:15 Sun , 19 Dec 2010 19:34:04 GMT Daniil Alexeyevsky me.dendik@тАж [38:db4d49b346d3] * snake.py ( modified ) implemented snake.Rule.applies; untested yet Sun , 19 Dec 2010 19:29:43 GMT Daniil Alexeyevsky me.dendik@тАж [37:67e6785396e1] * snake.py ( modified ) snake.Rule.load: added check that center of rule is own head Sun , 19 Dec 2010 19:25:27 ...
... Продолжены теоретические и экспериментальные исследования динамики поляризации излучения иттербиевого волоконного лазера с двойной оболочкой. ... International Conference Laser and Laser-information technologies: fundamental problems and Applications, ILLA 2006, p.83. ... Dynamical characteristics of generation of two-frequencies lasers with orthogonal polarizations //Proceedings of 8th International Conference on Laser and Fiber-Optical Networks Modeling, LFNM-2006, Kharkiv, Ukraine, July, 2006, pp...
Заседание семинара по социофизике . ... Goubko M. (2014) Minimizing Degree-Based Topological Indices for Trees with Given Number of Pendent Vertices // MATCH Commun. ... Goubko M., Gutman I. (2014) Degree-based topological indices: Optimal trees with given number of pendents // Applied Mathematics and Computation. ... Goubko M., Reti T. (2014) Note on Minimizing Degree-Based Topological Indices of Trees with Given Number of Pendent Vertices // MATCH Commun. ...
Gamma-rays above 10 TeV Dieter Horns University Hamburg RXJ1713-3946 [HESS Coll. ... The indirect path to the accelerator sky Dieter Horns University Hamburg Is it a good deal? [astro-ph/0607109] Unveiling Cosmic Ray accelerators: Interstellar medium ( B-field + gas + photons) Accelerated Nuclei Meson production via inelastic scattering Gamma-rays , Neutrinos Cosmic rays Neutral particles (photons neutrinos) retain directional information: Accelerator sky Charged particles ( ...
... C olumn S et C olumn V alues , . ... C olumn Add N ew C olumns C (Y ). ln(col(B )) C olumn S et C olumn V alues. , sq rt() Add F unction, col(B ) Add C olumn. , 1/, 1/sq rt(col(B )), OK . ... ln() Add F unction. col(B ) Add C olumn. ... Shift 3 C 6,0 5,5 Y Axis Title 5,0 4,5 4,0 350 400 450 500 550 600 650 X Axis Title . ... Layer . ... 0,8 B 20000 15000 Y Axis Title 10000 5000 0 0 200 400 600 800 1000 X Axis Title . ... 14 B 1400 1200 1000 Y Axis Title 800 600 400 200 0 200 400 X Axis Title 600 800...
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