radiative-gas dynamics

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• Radiative forcing — In climate science, radiative forcing is generally defined as the change in net irradiance between different layers of the atmosphere. Typically, radiative forcing is quantified at the tropopause in units of watts per square meter. A positive… …   Wikipedia

• Greenhouse gas — Simple diagram of greenhouse effect. A greenhouse gas (sometimes abbreviated GHG) is a gas in an atmosphere that absorbs and emits radiation within the thermal infrared range. This process is the fundamental cause of the greenhouse effect.[1] …   Wikipedia

• Coronal radiative losses — In astronomy and in astrophysics, for radiative losses of the solar corona, it is meant the energy flux irradiated from the external atmosphere of the Sun (traditionally divided into chromosphere, transition region and corona), and, in particular …   Wikipedia

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• GADGET — is a freely available code for cosmological N body/SPH simulations written by Volker Springel at the Max Planck Institute for Astrophysics. This article describes version 2 of GADGET (known as GADGET 2).DescriptionGADGET computes gravitational… …   Wikipedia

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• Smoothed particle hydrodynamics — (SPH) is a computational method used for simulating fluid flows. It has been used in many fields of research, including astrophysics, ballistics, vulcanology and oceanology. It is a mesh free Lagrangian method (where the co ordinates move with… …   Wikipedia

• Sergei Kurdumov — is a Russian scientist. He s a specialist in synergetics.Research activities* Inertial laser fusion, localization of thermonuclear burning, cumulative and self organization phenomena in nonlinear media * Two and three dimensional equilibrium and… …   Wikipedia

• analysis — /euh nal euh sis/, n., pl. analyses / seez /. 1. the separating of any material or abstract entity into its constituent elements (opposed to synthesis). 2. this process as a method of studying the nature of something or of determining its… …   Universalium