PPT
... • If displacement is occurred at the boundary, the lighter plasma which pushed up by the displacement is lighter than surrounding plasma so that it has a buoyancy then continue to move up. • Denser plasma which pushed down is heavier than surrounding plasma so that it has stronger gravity force then ...
... • If displacement is occurred at the boundary, the lighter plasma which pushed up by the displacement is lighter than surrounding plasma so that it has a buoyancy then continue to move up. • Denser plasma which pushed down is heavier than surrounding plasma so that it has stronger gravity force then ...
Current Systems in Planetary Magnetospheres and Ionospheres
... where E is the ambient electric field, and the so-called “pick-up conductivity” σpickup is proportional to the time rate of addition of new-born ions to the flow, ṅ. 2.1 Planetary Ionospheres and Associated Plasma Domains The solar ultraviolet and X-ray light impinging on a planet’s or moon’s atmos ...
... where E is the ambient electric field, and the so-called “pick-up conductivity” σpickup is proportional to the time rate of addition of new-born ions to the flow, ṅ. 2.1 Planetary Ionospheres and Associated Plasma Domains The solar ultraviolet and X-ray light impinging on a planet’s or moon’s atmos ...
The on quilibrium ISIS
... Characteristics of our spectral code (Ji PhD thesis 2006) based on the updated atomic data (CHIANTI , APED) the atomic data and the code are separate ...
... Characteristics of our spectral code (Ji PhD thesis 2006) based on the updated atomic data (CHIANTI , APED) the atomic data and the code are separate ...
Response of equatorial-low latitude ionosphere
... the ionospheric current system associated with the second pulse of si-it has the same pattern but opposite sense to that of the first pulse. The current system has been interpreted as the effect of reduced magnteospheric convection due to reduced dynamic pressure of solar wind. One can therefore exp ...
... the ionospheric current system associated with the second pulse of si-it has the same pattern but opposite sense to that of the first pulse. The current system has been interpreted as the effect of reduced magnteospheric convection due to reduced dynamic pressure of solar wind. One can therefore exp ...
Laboratory Astrophysics: Spectral Analysis of Photoionized Neon J ames MacArthur
... depends on the product of the ion and electron densities) and a larger electron velocity increases the energy and collisional frequency. Collisionally ionized plasmas are common in the earth and throughout the universe. Planetary cores, stars, stellar coronae, and black hole accretion disks are just ...
... depends on the product of the ion and electron densities) and a larger electron velocity increases the energy and collisional frequency. Collisionally ionized plasmas are common in the earth and throughout the universe. Planetary cores, stars, stellar coronae, and black hole accretion disks are just ...
Determination of the levitation limits of dust particles within the
... and the extent of the unstable region near the lower electrode, locating the lower levitation limit for dust particles, in radio frequency (RF) discharges. These results are then compared to current sheath theories. With this, a new, in situ experimental method is provided that can be employed in an ...
... and the extent of the unstable region near the lower electrode, locating the lower levitation limit for dust particles, in radio frequency (RF) discharges. These results are then compared to current sheath theories. With this, a new, in situ experimental method is provided that can be employed in an ...
On the dimensionally correct kinetic theory of turbulence
... the underlying equations can be readily solved by computational means. This cannot be accomplished unless the foundational nonlinear response functions—which are expressed in terms of formal momentum integrals over the derivatives of the particle distribution functions, and also involve multiple inf ...
... the underlying equations can be readily solved by computational means. This cannot be accomplished unless the foundational nonlinear response functions—which are expressed in terms of formal momentum integrals over the derivatives of the particle distribution functions, and also involve multiple inf ...
The Properties of Reconnection Current Sheets in GRMHD
... et al. 2015a, b) where we coupled HARM to the radiative transfer algorithm GRay (Chan et al. 2013) and varied the black hole spin, density normalization, observer inclination, initial magnetic field configuration, as well as the electron thermodynamic prescription. From these investigations, we iden ...
... et al. 2015a, b) where we coupled HARM to the radiative transfer algorithm GRay (Chan et al. 2013) and varied the black hole spin, density normalization, observer inclination, initial magnetic field configuration, as well as the electron thermodynamic prescription. From these investigations, we iden ...
The energetics of relativistic magnetic reconnection: ion
... In all these cases, it is crucial to know the amount of magnetic energy transferred to the particles during a reconnection event, the relative fraction distributed to ions and electrons, as ...
... In all these cases, it is crucial to know the amount of magnetic energy transferred to the particles during a reconnection event, the relative fraction distributed to ions and electrons, as ...
Low-energy charged particle measurement by MAP-PACE onboard SELENE
... limb of the Moon and the degree of the plasma compression has a regional dependence (Criswell, 1973). It is therefore thought that there is a weak but significant magnetic field anomaly on the surface of the Moon and that this deflects the solar wind particles and varies the degree of compression (L ...
... limb of the Moon and the degree of the plasma compression has a regional dependence (Criswell, 1973). It is therefore thought that there is a weak but significant magnetic field anomaly on the surface of the Moon and that this deflects the solar wind particles and varies the degree of compression (L ...
Understanding of the role of magnetic fields: Galactic perspective
... be slow, there is a possibility (which has not yet been convincingly refuted) that all simulation related to the interstellar medium, including those of turbulence have significnant errors due to a dramatic disparity between the rates of astrophysical and numerical reconnection. If the reconnection ...
... be slow, there is a possibility (which has not yet been convincingly refuted) that all simulation related to the interstellar medium, including those of turbulence have significnant errors due to a dramatic disparity between the rates of astrophysical and numerical reconnection. If the reconnection ...
Pickup ions near Mars associated with escaping oxygen atoms
... suggested in this paper that ‘‘the pickup ions detected by SLED should have their origin 5 – 6 104 km upstream of Mars’’ (this is due to the very large gyroradius of a pickup oxygen ion). [4] Pickup ions are created by the ionization of neutrals and are initially almost at rest in comparison with ...
... suggested in this paper that ‘‘the pickup ions detected by SLED should have their origin 5 – 6 104 km upstream of Mars’’ (this is due to the very large gyroradius of a pickup oxygen ion). [4] Pickup ions are created by the ionization of neutrals and are initially almost at rest in comparison with ...
Simultaneous observation of the electron acceleration and ion deceleration
... Y. SAITO et al.: ELECTRON ACCELERATION AND ION DECELERATION OVER LUNAR MAGNETIC ANOMALIES ...
... Y. SAITO et al.: ELECTRON ACCELERATION AND ION DECELERATION OVER LUNAR MAGNETIC ANOMALIES ...
Potential for Life on the Terrestrial Planets
... fluxes result in higher exospheric temperatures and more expanded thermosphereexosphere environments and, hence, suffer stronger atmospheric erosion, which may result in the total loss of several hundred bars even if an exoplanet is protected by a “magnetic shield” with its boundary located at one E ...
... fluxes result in higher exospheric temperatures and more expanded thermosphereexosphere environments and, hence, suffer stronger atmospheric erosion, which may result in the total loss of several hundred bars even if an exoplanet is protected by a “magnetic shield” with its boundary located at one E ...
