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 ...
... 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 ...
Photospheric processes and magnetic flux tubes
... region far enough above the merging height the radial component of the magnetic field vanishes and the gas pressure becomes negligible so that Ampères law reduces to ...
... region far enough above the merging height the radial component of the magnetic field vanishes and the gas pressure becomes negligible so that Ampères law reduces to ...
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 ...
... 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
... 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. ...
... 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. ...
RADIO RELICS AND MAGNETIC FIELDS IN GALAXY CLUSTERS
... Radio relics are diffuse synchrotron sources generally located in the peripheries of galaxy clusters in merging state. According to the current leading scenario, relics trace gigantic cosmological shock waves that cross the intra-cluster medium where particle acceleration occurs. The relic/shock con ...
... Radio relics are diffuse synchrotron sources generally located in the peripheries of galaxy clusters in merging state. According to the current leading scenario, relics trace gigantic cosmological shock waves that cross the intra-cluster medium where particle acceleration occurs. The relic/shock con ...
Charging and interaction of two-particle system within a glass box
... the top particle in a vertical, two-particle chain is pushed from its equilibrium position using a high-power Verdi laser, and as it returns to equilibrium will interact with the second particle. In order to isolate the particle interaction force, the electrostatic force and neutral drag force are s ...
... the top particle in a vertical, two-particle chain is pushed from its equilibrium position using a high-power Verdi laser, and as it returns to equilibrium will interact with the second particle. In order to isolate the particle interaction force, the electrostatic force and neutral drag force are s ...
(2004) - H. Peter
... come from in active stars? higher “filling-factor” than Sun? not enough space on the surface and: also stellar X-rays are structured stellar corona are not only brighter, they have also high densities high temperatures ...
... come from in active stars? higher “filling-factor” than Sun? not enough space on the surface and: also stellar X-rays are structured stellar corona are not only brighter, they have also high densities high temperatures ...
- 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 ...
... 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
... • Relates features on the seismogram to the behaviour of different types of earthquake waves and Earth’s internal structure • Relates features on the seismogram to the behaviour of different types of earthquake waves and/or Earth’s internal structure • Links features of the seismogram to waves and/o ...
... • Relates features on the seismogram to the behaviour of different types of earthquake waves and Earth’s internal structure • Relates features on the seismogram to the behaviour of different types of earthquake waves and/or Earth’s internal structure • Links features of the seismogram to waves and/o ...
Chapter 15--Our Sun - Geological Sciences
... demands for roughly the next 500,000 years! Of course, only a tiny fraction of the Sun’s total energy output reaches Earth, with the rest dispersing in all directions into space. Most of this energy is radiated in the form of visible light, but once you leave the protective blanket of Earth’s atmosp ...
... demands for roughly the next 500,000 years! Of course, only a tiny fraction of the Sun’s total energy output reaches Earth, with the rest dispersing in all directions into space. Most of this energy is radiated in the form of visible light, but once you leave the protective blanket of Earth’s atmosp ...
Magnetism in Isolated and Binary White Dwarfs
... 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 ...
... 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 ...
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 ...
... 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 ...