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URL - StealthSkater
URL - StealthSkater

... Beltrami fields. The condition implies that vacuum currents can be non-vanishing only provided the dimension DCP2 of the CP2 projection of the space-time surface is less than four(4) so that in the regions with D CP2=4, Maxwell's vacuum equations are satisfied. The hypothesis that Kähler current is ...
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Molecular Clouds and the Onset of Star Formation

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Introducing the fission–fusion reaction process: using a

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Interpretation of the Helix Planetary Nebula using Hydro

... luminous mass of stars and  the more diffusive NBDM-ISM (CDM) mass. The million trillion-planet-PGCs per galaxy each have fossil-density ρ0 ≈ ρP GC ≈ ×104 greater than the hρg i ≈ 10−21 kg m−3 galaxy average and ≈ ×109 hρU i, where hρU i ≈ 10−26 kg m−3 is the flat universe average density at the pr ...
NASA/TM—2005–213688 National Aeronautics and Space Administration AD33
NASA/TM—2005–213688 National Aeronautics and Space Administration AD33

... revolutionary ideas for shielding that would mitigate these costs were examined. None of the revolutionary new ideas examined for the first time in this workshop showed clear promise. The workshop participants felt that some previously examined concepts were definitely useful and should be pursued. ...
Radiato-Magneto-Thermal Winds from an Accretion Disk
Radiato-Magneto-Thermal Winds from an Accretion Disk

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RADIO RELICS AND MAGNETIC FIELDS IN GALAXY CLUSTERS

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Magnetized Quark and Strange Quark Matter in the Spherical Symmetric Space-Time Admitting Conformal Motion

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Section IV High-Energy Astrophysics and Cosmology

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EUV and X-ray Spectroscopy of the Active Sun

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- Repository of the Academy`s Library

... The solar corona and the Earth’s magnetosphere are undoubtedly the most studied natural plasma systems. Both consist of highly ionised plasmas penetrated by a magnetic field, that plays the decisive role in the structure, short-term dynamics and long-term evolution of these plasmas. The solar corona ...
2016 HSC Physics Marking Guidelines
2016 HSC Physics Marking Guidelines

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Evolution of Oxygen Deficiency Center on Fused Silica Surface

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Solar Flares: Magnetohydrodynamic Processes | SpringerLink

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... to mix. These calculations enabled Angel et al. (1974) to identify the peculiar features in the spectrum of GD 90 as Balmer lines with resolvable Zeeman structure at a mean surface Ðeld of 5 MG. This represented the Ðrst unequivocal determination of the magnetic Ðeld of a white dwarf and heralded th ...
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Jeans instability criterion modified by external

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Influence of Hydrogen Atoms on the Growth of carbon based

... expands in form of a ball for power values above 300 W. In the region of expansion the plasma is not bounded by the wall of the quartz tube so wall recombination and wall loss processes do not exist in this region. The photo of the so-called plasma ball is presented in the Fig. 2.1 in the left upper ...
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Low-temperature surface formation of NH3 and HNCO

Low-temperature surface formation of NH3 and HNCO
Low-temperature surface formation of NH3 and HNCO

A. Point Charge Model for Ion Wakefields
A. Point Charge Model for Ion Wakefields

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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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