Titlebook: Laser Optoelectronic Oscillators; Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smols Book 2020 The Editor(s) (if applicable) and The Autho

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0342-4111 nd oscillators with electromagnetic wave cavities. Special attention is paid to Q-factors and phase noises of RF carriers at small offsets. The authors discuss the technical characteristics of modern optoelectr978-3-030-45702-0978-3-030-45700-6Series ISSN 0342-4111 Series E-ISSN 1556-1534

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h’s interior. Elastic waves may be generated by earthquakes or artificial sources (explosives). Analysing the recorded wavefields yields information about the medium through which the waves have propagated. Information about the velocity structure within the Earth, provides important constraints on

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Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smolskiy. In this way, it is possible to describe the thermal evolution of the Earth more realistically than by parameterized convection models. The model is heated mainly from within by a temporally declining heat generation rate per volume and, to a minor degree, from below. The volumetrically averaged te

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Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smolskiy. In this way, it is possible to describe the thermal evolution of the Earth more realistically than by parameterized convection models. The model is heated mainly from within by a temporally declining heat generation rate per volume and, to a minor degree, from below. The volumetrically averaged te

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Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smolskiy. In this way, it is possible to describe the thermal evolution of the Earth more realistically than by parameterized convection models. The model is heated mainly from within by a temporally declining heat generation rate per volume and, to a minor degree, from below. The volumetrically averaged te

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Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smolskiyential equations for infinite Prandtl-number convection are solved using a three-dimensional finite-element spherical-shell method on a computational mesh derived from a regular icosahedron with 1.351.746 or, alternatively, 10.649.730 nodes. We formulate a radial viscosity profile from solid-state p

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Alexander A. Bortsov,Yuri B. Il’in,Sergey M. Smolskiyblack holes in microquasar or black hole X-ray binaries (BHXBs), around young stellar objects, but also around stellar compact sources as white dwarfs in symbiotic stars and neutron stars in low mass X-ray binaries (LMXBs). In interacting binaries containing compact objects, the secondary — a main-s