Spectral and Hydrodynamic Modeling of X-Ray Michael Rosenberg
... field will experience a force inward toward the z-axis (Figure 1.5). This pinching motion toward the z-axis is what gives the Z-pinch its name. This fairly uniform cylindrical shell of plasma implodes onto its axis at a velocity of nearly 100 km/s or 10 cm/ /-LS. As a piece of plasma approaches the ...
... field will experience a force inward toward the z-axis (Figure 1.5). This pinching motion toward the z-axis is what gives the Z-pinch its name. This fairly uniform cylindrical shell of plasma implodes onto its axis at a velocity of nearly 100 km/s or 10 cm/ /-LS. As a piece of plasma approaches the ...
Simulations of Collisionless Perpendicular Shocks in Partially
... and downstream regions, the plasma flow is gradually decelerated by the pressure of pickup ions produced in upstream and downstream regions. In this Letter, charge exchange and collisional ionization are enhanced by a factor of 103 and vsh ≈ 10 vA , so that the actual ionization length scale becomes ...
... and downstream regions, the plasma flow is gradually decelerated by the pressure of pickup ions produced in upstream and downstream regions. In this Letter, charge exchange and collisional ionization are enhanced by a factor of 103 and vsh ≈ 10 vA , so that the actual ionization length scale becomes ...
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... field structures was investigated in Kramar et al. (2014). There we applied the tomography method that employs STEREO data to reconstruct 3D density of global solar corona and related it to the coronal magnetic field structure. This method was applied to characterize the solar corona over the Carrin ...
... field structures was investigated in Kramar et al. (2014). There we applied the tomography method that employs STEREO data to reconstruct 3D density of global solar corona and related it to the coronal magnetic field structure. This method was applied to characterize the solar corona over the Carrin ...
Magnetic fluctuations and formation of large-scale inhomogeneous magnetic structures
... mean horizontal magnetic field to the bottom of a cell, but impeding its upward return 关4,13,23兴. Turbulence may form inhomogeneous large-scale magnetic fields due to turbulent diamagnetic and paramagnetic effects 共see, e.g., 关3,24–28兴兲. Inhomogeneous velocity fluctuations lead to a transport of mea ...
... mean horizontal magnetic field to the bottom of a cell, but impeding its upward return 关4,13,23兴. Turbulence may form inhomogeneous large-scale magnetic fields due to turbulent diamagnetic and paramagnetic effects 共see, e.g., 关3,24–28兴兲. Inhomogeneous velocity fluctuations lead to a transport of mea ...
More detailed notes
... deuterium-fusing stage is very short and generates little energy. It is usually neglected in considering stellar evolution, but is used as a convenient yardstick to separate brown dwarfs (which never fuse 1H, but do fuse 2H) from gas giant planets (which never fuse anything). The corresponding mass ...
... deuterium-fusing stage is very short and generates little energy. It is usually neglected in considering stellar evolution, but is used as a convenient yardstick to separate brown dwarfs (which never fuse 1H, but do fuse 2H) from gas giant planets (which never fuse anything). The corresponding mass ...
PoS(AASKA14)174 - Proceeding of science
... was followed by the comforting conjecture that the Universe was essentially in a “steady state” with a constant rate of stars ageing and being replaced. What instead became apparent in the late 1990’s is that the rate at which stars are formed has varied dramatically with time. That rate has increas ...
... was followed by the comforting conjecture that the Universe was essentially in a “steady state” with a constant rate of stars ageing and being replaced. What instead became apparent in the late 1990’s is that the rate at which stars are formed has varied dramatically with time. That rate has increas ...
2014 HSC Physics - Board of Studies
... Which of the following best describes the motion of the particles? (A) Both particles move with the same acceleration. (B) ...
... Which of the following best describes the motion of the particles? (A) Both particles move with the same acceleration. (B) ...
Precipitation Behavior and Magnetic Properties of Cu-Fe
... formed after annealing at 973 K for 2000 min. Figures 4(a)– 4(d) correspond to the atomic structure inside the precipitate, while Figures 4(e)–4(h) correspond to the copper matrix. The spots appearing in Figure 4(b) are due to the lattice fringes of the B2 structure of the ordered FeCo intermediate ...
... formed after annealing at 973 K for 2000 min. Figures 4(a)– 4(d) correspond to the atomic structure inside the precipitate, while Figures 4(e)–4(h) correspond to the copper matrix. The spots appearing in Figure 4(b) are due to the lattice fringes of the B2 structure of the ordered FeCo intermediate ...