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Hvězdný make up Proč jsou hvězdy skvrnité?
Hvězdný make up Proč jsou hvězdy skvrnité?

... necessity of a rigid rotation and to admit that the outer layers controlled by magnetic field and denser inner parts can rotate differently.” Stępień (1998). ...
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The theme “Research of fundamental interactions in nucleus at low

... comprise non-luminous, nonbaryonic matter. Cosmological data indicate that only 5% of the mass in the Universe are accounted for by ordinary substance and another <2% by neutrinos. The unknown rest composition is dark energy (65–70%) and dark matter (about 25%). A direct observation of the interacti ...
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... order of 10−6 G; see Refs. [1–3] and references therein. Understanding the origin of these fields is one of the challenging questions of modern astrophysics. Generally speaking, there are two popular scenarios. The first one envisages the generation of magnetic fields through different astrophysical ...
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... bremsstrahlung, cyclotron and synchrotron radiation. In these cases the acceleration of the electron is just produced either by the collision or by the Lorentz force due to the magnetic field. ...
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Proposed isotropic negative index in three-dimensional optical metamaterials Boubacar Kante, Kevin O’Brien,

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Project list - Institute for Nuclear Theory

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the magnetic field properties of radio galaxies in different

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... these particles (gravitational microclusters of lunar dust) inside the lunar exosphere. Under these circumstances, it density becomes equal to the density of the lunar exosphere (~ 10 −18 kg.m −3 ) [14]. The amount of Rayleigh scattering that occurs for a beam of light depends upon the size of the p ...
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< 1 ... 15 16 17 18 19 20 21 22 23 ... 39 >

Spheromak

Not to be confused with the spherical tokamak, another topic in fusion research.A spheromak is an arrangement of plasma formed into a toroidal shape similar to a smoke ring. The spheromak contains large internal electric currents and their associated magnetic fields arranged so the magnetohydrodynamic forces within the spheromak are nearly balanced, resulting in long-lived (microsecond) confinement times without external fields. Spheromaks belong to a type of plasma configuration referred to as the compact toroids.The physics of the spheromak and their collisions is similar to a variety of astrophysical events, like coronal loops and filaments, relativistic jets and plasmoids. They are particularly useful for studying magnetic reconnection events, when two or more spheromaks collide. Spheromaks are easy to generate using a ""gun"" that ejects spheromaks off the end of an electrode into a holding area, called the flux conserver. This has made them useful in the laboratory setting, and spheromak guns are relatively common in astrophysics labs. These devices are often, confusingly, referred to simply as ""spheromaks"" as well; the term has two meanings.Spheromaks have been proposed as a magnetic fusion energy concept due to their long confinement times, which was on the same order as the best tokamaks when they were first studied. Although they had some successes during the 1970s and 80s, these small and lower-energy devices had limited performance and most spheromak research ended when fusion funding was dramatically curtailed in the late 1980s. However, in the late 1990s research demonstrated that hotter spheromaks have better confinement times, and this led to a second wave of spheromak machines. Spheromaks have also been used to inject plasma into a bigger magnetic confinement experiment like a tokamak.
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