Quantum mechanical model for the study of pressure
... electronic structure of a SC is similar to the traditional average-atom calculation, except that each SC has an integer number of bound electrons. The equations required for the calculation of SCs are obtained from the stationarity of the ion-cell free energy with imposed integer populations for the ...
... electronic structure of a SC is similar to the traditional average-atom calculation, except that each SC has an integer number of bound electrons. The equations required for the calculation of SCs are obtained from the stationarity of the ion-cell free energy with imposed integer populations for the ...
Real Properties of Electromagnetic Fields and
... such that electrostatic forces between bodies that are each surrounded by such DL-bounded plasma cells are negligibly weak. Homogeneous models often are found to be misleading and should be replaced by inhomogeneous models, with the inhomogeneities being produced by filamentary currents and DLs that ...
... such that electrostatic forces between bodies that are each surrounded by such DL-bounded plasma cells are negligibly weak. Homogeneous models often are found to be misleading and should be replaced by inhomogeneous models, with the inhomogeneities being produced by filamentary currents and DLs that ...
Dynamical Petschek Reconnection
... thought to play a core role in explosive energy conversion of solar flares. According to the SweetParker theory, it is, however, difficult to conduct magnetic reconnection efficiently in highly conductive plasma of the solar corona. Petschek proposed another reconnection theory, in which small magne ...
... thought to play a core role in explosive energy conversion of solar flares. According to the SweetParker theory, it is, however, difficult to conduct magnetic reconnection efficiently in highly conductive plasma of the solar corona. Petschek proposed another reconnection theory, in which small magne ...
Argon is a chemical element represented by the symbol Ar.
... Argon is a chemical element represented by the symbol Ar. Argon has atomic number 18 and is the third element in group 18 of the periodic table. Argon is the third most common gas in the Earth's atmosphere, at 0.93%, making it more common than carbon dioxide. Nearly all of this argon is radiogenic a ...
... Argon is a chemical element represented by the symbol Ar. Argon has atomic number 18 and is the third element in group 18 of the periodic table. Argon is the third most common gas in the Earth's atmosphere, at 0.93%, making it more common than carbon dioxide. Nearly all of this argon is radiogenic a ...
Longitudinal Asymmetry of the Jovian Magnetosphere
... interplanetary space.Thus although the particlesescapeprinWe propose that the observed 10-hour variations in ener- cipally on the night side of Jupiter, they may be observedon geticparticle fluxesobservedboth in the magnetosphereand in the day side on interplanetary field lines that connect to the i ...
... interplanetary space.Thus although the particlesescapeprinWe propose that the observed 10-hour variations in ener- cipally on the night side of Jupiter, they may be observedon geticparticle fluxesobservedboth in the magnetosphereand in the day side on interplanetary field lines that connect to the i ...
Nanocrystalline silicon prepared at high growth rate using helium
... By extrapolating the straight portion of the Tauc’s plot to α = 0 at the onset of optical absorption (as shown by the inset of figure 1), the optical gap (Eg) of the samples was estimated and that shows its gradual widening, as presented in table 1. Systematic reduction in α and simultaneous widenin ...
... By extrapolating the straight portion of the Tauc’s plot to α = 0 at the onset of optical absorption (as shown by the inset of figure 1), the optical gap (Eg) of the samples was estimated and that shows its gradual widening, as presented in table 1. Systematic reduction in α and simultaneous widenin ...
Beyond Ideal MHD - Harvard-Smithsonian Center for Astrophysics
... Higher frequency waves go faster (unlike sound, Alfvén waves) ...
... Higher frequency waves go faster (unlike sound, Alfvén waves) ...
AMPTE: NOTES ON THE INITIAL ... WORK IN PROGRESS _ _ _ _ _... _
... was more filamentary than one might have anticipated. It consisted essentially of plasma blobs that were breaking off from the main body of the comet. The comet created a magnetic cavity in the solar wind that collapsed suddenly about 270 seconds after release, much sooner than expected. We had expe ...
... was more filamentary than one might have anticipated. It consisted essentially of plasma blobs that were breaking off from the main body of the comet. The comet created a magnetic cavity in the solar wind that collapsed suddenly about 270 seconds after release, much sooner than expected. We had expe ...
On the origin of the fast solar wind in polar coronal funnels
... replenishing of the spectrum. The kinetic physics of the wavedamping process in the dissipation domain is certainly much more complicated and still not understood well. For a further discussion see Marsch (1999) and references therein. The spatial evolution of the wave energy-density spectrum P is d ...
... replenishing of the spectrum. The kinetic physics of the wavedamping process in the dissipation domain is certainly much more complicated and still not understood well. For a further discussion see Marsch (1999) and references therein. The spatial evolution of the wave energy-density spectrum P is d ...
Slide 1
... Likewise in the absence of bounce-resonant field variations, the second (bounce) adiabatic invariant is expected to be conserved. In a dipole field this is ...
... Likewise in the absence of bounce-resonant field variations, the second (bounce) adiabatic invariant is expected to be conserved. In a dipole field this is ...
Relativistic electron-positron plasmas
... Despite the diversity, collisionless shocks share common characteristics: they are inferred to efficiently accelerate nonthermal particles and to generate and amplify magnetic fields, in addition to effectively decelerating supersonic flows. As a result of nonlinear plasma processes involved in the ...
... Despite the diversity, collisionless shocks share common characteristics: they are inferred to efficiently accelerate nonthermal particles and to generate and amplify magnetic fields, in addition to effectively decelerating supersonic flows. As a result of nonlinear plasma processes involved in the ...
Driven reconnection and bursty bulk flows
... δi ∼ 104 km during a BBF, one can show (Lakhina, 1996) that the Earthward flow with a bulk velocity vx > 400 km s−1 lasting for a few seconds and bulk flows with speeds of ∼ 100 km s−1 lasting for about one minute or so can be produced by the bursty driven reconnections. Initially, the energy is sto ...
... δi ∼ 104 km during a BBF, one can show (Lakhina, 1996) that the Earthward flow with a bulk velocity vx > 400 km s−1 lasting for a few seconds and bulk flows with speeds of ∼ 100 km s−1 lasting for about one minute or so can be produced by the bursty driven reconnections. Initially, the energy is sto ...
Other Solar System Bodies
... that the moon spends part of its orbit inside the terrestrial magnetosphere, such that its interaction at these times is with the various magnetospheric fields and plasma populations discussed above, rather than the solar wind. Comets A comet nucleus is a relatively small body (~ a few 10’s of kilom ...
... that the moon spends part of its orbit inside the terrestrial magnetosphere, such that its interaction at these times is with the various magnetospheric fields and plasma populations discussed above, rather than the solar wind. Comets A comet nucleus is a relatively small body (~ a few 10’s of kilom ...