
Talk - Frontiers in Computational Astrophysics
... a structure with leading and trailing shocks. Shock is similar to the shock in simulations with the constant contact discontinuity. The spectrum from jet electrons in a weak magnetic field in a small system shows a Bremsstrahlung like spectrum with higher frequency enhancement with turbulent mag ...
... a structure with leading and trailing shocks. Shock is similar to the shock in simulations with the constant contact discontinuity. The spectrum from jet electrons in a weak magnetic field in a small system shows a Bremsstrahlung like spectrum with higher frequency enhancement with turbulent mag ...
Document
... randomly from a uniform distribution between 0° and 90°, and the initial energies chosen randomly from a power law distribution between 28.469keV and 128.109keV. In this situation, increasing the initial energies results in much less change in the evolution of the distribution function over time com ...
... randomly from a uniform distribution between 0° and 90°, and the initial energies chosen randomly from a power law distribution between 28.469keV and 128.109keV. In this situation, increasing the initial energies results in much less change in the evolution of the distribution function over time com ...
Dynamic Martian magnetosphere: Transient - HAL
... (with Bz > 0), a parallel Bow Shock (BS) region (region of the BS where the shock normal is parallel to the IMF direction) can be identified in the -Z half plane. Figure 1 represents an isovalue surface of the total magnetic field at 5 nT highlighting the BS surface at t = 0 s corresponding to the o ...
... (with Bz > 0), a parallel Bow Shock (BS) region (region of the BS where the shock normal is parallel to the IMF direction) can be identified in the -Z half plane. Figure 1 represents an isovalue surface of the total magnetic field at 5 nT highlighting the BS surface at t = 0 s corresponding to the o ...
- EPJ Web of Conferences
... Deduction of Lorentz forces analytical formula for cuboid container was performed in this article. This formula was obtained by transformation of analytical formula from cylindrical container. Contours of Lorentz forces obtained from CFD code NS-FEM3D and analytical formula were displayed. A simplif ...
... Deduction of Lorentz forces analytical formula for cuboid container was performed in this article. This formula was obtained by transformation of analytical formula from cylindrical container. Contours of Lorentz forces obtained from CFD code NS-FEM3D and analytical formula were displayed. A simplif ...
BRFFI
... A new approach to the q-deformation procedure of the simplest classical symmetry groups and their Lee algebra's, based on the use of the special composition rule for group vector-parameters and corresponding linearity relations, is developed. In the framework of the earlier constructed axiomatic t ...
... A new approach to the q-deformation procedure of the simplest classical symmetry groups and their Lee algebra's, based on the use of the special composition rule for group vector-parameters and corresponding linearity relations, is developed. In the framework of the earlier constructed axiomatic t ...
zaneposter
... and the Soft Gamma-ray Repeaters (SGRs), two classes of sources observationally very similar in many respects (see Mereghetti et al. 2008 for a review).They are all slow X-ray pulsars with spin periods clustered in a narrow range (P ~ 2-12 s), relatively large period derivatives (dP/dt ~ 10-13 -10-1 ...
... and the Soft Gamma-ray Repeaters (SGRs), two classes of sources observationally very similar in many respects (see Mereghetti et al. 2008 for a review).They are all slow X-ray pulsars with spin periods clustered in a narrow range (P ~ 2-12 s), relatively large period derivatives (dP/dt ~ 10-13 -10-1 ...
Angular momentum evolution
... Observational constraints • Several thousands of rotational periods now available for solar-type and low-mass stars from ~1 Myr to a ~10 Gyr (0.2-1.2 Msun) • Kepler still expected to yield many more rotational periods for field stars • Several tens of vsini measurements available for VLM stars and ...
... Observational constraints • Several thousands of rotational periods now available for solar-type and low-mass stars from ~1 Myr to a ~10 Gyr (0.2-1.2 Msun) • Kepler still expected to yield many more rotational periods for field stars • Several tens of vsini measurements available for VLM stars and ...