Kinetic aspects of the vortex-induced
... where is the Lorentz factor, c is the speed of light and the suffix j is the particle number. The charge density and the current density J is calculated by the PIC method. Using initial density N0 and in-plane magnetic field B0, normalizations are made as follows: the velocity, time, and length ...
... where is the Lorentz factor, c is the speed of light and the suffix j is the particle number. The charge density and the current density J is calculated by the PIC method. Using initial density N0 and in-plane magnetic field B0, normalizations are made as follows: the velocity, time, and length ...
X-Ray Scattering from Warm Dense Matter at Vulcan
... Counter propagating long pulse beams simultaneously irradiate a plastic coated aluminium target (targets are produced on site, allowing user flexibility on their design). As the plastic ablates, the rocket like expansion drives shock waves through the target. Careful selection of the pulse duration, ...
... Counter propagating long pulse beams simultaneously irradiate a plastic coated aluminium target (targets are produced on site, allowing user flexibility on their design). As the plastic ablates, the rocket like expansion drives shock waves through the target. Careful selection of the pulse duration, ...
Isolated Attosecond Pulses from Laser
... (FWHM) is 3TL , where TL is the light wave period. The time and space steps aret 1:3 105 TL , z 2:6 105 0 . Initially, 100 particles are in each mesh cell; both electrons and ions are mobile. The characteristic times t1 , t2 , and t3 of the subcycle release of plasma electrons, thei ...
... (FWHM) is 3TL , where TL is the light wave period. The time and space steps aret 1:3 105 TL , z 2:6 105 0 . Initially, 100 particles are in each mesh cell; both electrons and ions are mobile. The characteristic times t1 , t2 , and t3 of the subcycle release of plasma electrons, thei ...
On the Electrodynamics of the Big Bang Universe - SLAC
... in the expression for current j = nev. Actually, due to the three dimensional wrinkling of sheet-void boundaries, current amplification in certain local volumes (in corners) will be very much larger. However, simultaneously, the number of current carriers, n , will also increase dramatically due to ...
... in the expression for current j = nev. Actually, due to the three dimensional wrinkling of sheet-void boundaries, current amplification in certain local volumes (in corners) will be very much larger. However, simultaneously, the number of current carriers, n , will also increase dramatically due to ...
Presentación de PowerPoint - High
... • Understanding the role of dust particles into the Faraday Effect, we found that the electron contribution is predominant for the dusty torus of AGN, and the dust does not affect the rotation of electron vector of polarization (EVPA). • For the outer parts of the jet, kilo-parsec regions, the elect ...
... • Understanding the role of dust particles into the Faraday Effect, we found that the electron contribution is predominant for the dusty torus of AGN, and the dust does not affect the rotation of electron vector of polarization (EVPA). • For the outer parts of the jet, kilo-parsec regions, the elect ...
Prediction of the Plasma Environment in the Geostationary Orbit
... are presumably influenced by increased pressure due to the fluid adiabatic process from the magnetotail in the plasma injection process. However, no quantitative consistency was found in electron density and temperature; the density resulting from calculation is much larger than that observed in mos ...
... are presumably influenced by increased pressure due to the fluid adiabatic process from the magnetotail in the plasma injection process. However, no quantitative consistency was found in electron density and temperature; the density resulting from calculation is much larger than that observed in mos ...
A novel mechanism for electron-cyclotron maser
... Another important instability driven by a fast electron beam is the Langmuir wave (LW) instability, which usually has a much faster growth rate than that of the AW instability. However, this does not imply that the LW instability is more important than the AW instability. The propagation of the LW c ...
... Another important instability driven by a fast electron beam is the Langmuir wave (LW) instability, which usually has a much faster growth rate than that of the AW instability. However, this does not imply that the LW instability is more important than the AW instability. The propagation of the LW c ...
Title Three-dimensional diagnostics of dynamic behaviors of excited
... The structure of our present ac-type panel for the 3-D measurement is shown schematically in Fig. 1, with components labeled (a)–(i). It has a design similar to a realistic ac-type cell in the structure and size. The essential point to realize the 3-D observation was the idea of using transparent gl ...
... The structure of our present ac-type panel for the 3-D measurement is shown schematically in Fig. 1, with components labeled (a)–(i). It has a design similar to a realistic ac-type cell in the structure and size. The essential point to realize the 3-D observation was the idea of using transparent gl ...
Northward IMF
... • Because is it easy for particles to move along the magnetic field the radiation belts are mainly field aligned features. • The ring current is an azimuthal current circling the Earth at equatorial distances of 3RE to 6RE. • There is no clear distinction between the ring current particles and the r ...
... • Because is it easy for particles to move along the magnetic field the radiation belts are mainly field aligned features. • The ring current is an azimuthal current circling the Earth at equatorial distances of 3RE to 6RE. • There is no clear distinction between the ring current particles and the r ...
Northward IMF - University of Massachusetts Lowell
... • Because is it easy for particles to move along the magnetic field the radiation belts are mainly field aligned features. • The ring current is an azimuthal current circling the Earth at equatorial distances of 3RE to 6RE. • There is no clear distinction between the ring current particles and the r ...
... • Because is it easy for particles to move along the magnetic field the radiation belts are mainly field aligned features. • The ring current is an azimuthal current circling the Earth at equatorial distances of 3RE to 6RE. • There is no clear distinction between the ring current particles and the r ...
Spontaneous radiative alignment of dipole moments of atoms
... having a dielectric constant ~ ( w = is the plasma frequency and vo is the collision frequency). This model of the medium is quite general, since it describes a collisionless plasma and a weakly ionized collisional gas (W 4vo). Also discussed is spontaneous self-polarization in a gas of unperturbed ...
... having a dielectric constant ~ ( w = is the plasma frequency and vo is the collision frequency). This model of the medium is quite general, since it describes a collisionless plasma and a weakly ionized collisional gas (W 4vo). Also discussed is spontaneous self-polarization in a gas of unperturbed ...
Nanocrystalline silicon prepared at high growth rate using helium
... High H2 dilution and high level of electrical excitation to the SiH4 plasma are the two critical parameters facilitating the growth of nanocrystalline network in plasma enhanced chemical vapour deposition (PECVD). However, high H2 dilution retards the film growth rate and high electrical power cause ...
... High H2 dilution and high level of electrical excitation to the SiH4 plasma are the two critical parameters facilitating the growth of nanocrystalline network in plasma enhanced chemical vapour deposition (PECVD). However, high H2 dilution retards the film growth rate and high electrical power cause ...
Spectroscopic study of the decomposition process of
... formula [24]: N e = C(Te,N e) (k S)3/2, where k s is the Stark broadening of line in Å and C(Te,N e) = 3.58 1014 Å 3/2 cm 3—constant. The profile of hydrogen line was recorded in the second order by means of high resolution spectrograph with the dispersion of 130 pixels/nm. The experimental ...
... formula [24]: N e = C(Te,N e) (k S)3/2, where k s is the Stark broadening of line in Å and C(Te,N e) = 3.58 1014 Å 3/2 cm 3—constant. The profile of hydrogen line was recorded in the second order by means of high resolution spectrograph with the dispersion of 130 pixels/nm. The experimental ...
m - viXra
... mechanical, electromagnetic, etc. For example, we can look on the momentum variation Δp as due to absorption or emission of electromagnetic energy. In this case, it was shown previously that the expression of χ , in the particular case of incident radiation on a heterogeneous matter(powder, dust, cl ...
... mechanical, electromagnetic, etc. For example, we can look on the momentum variation Δp as due to absorption or emission of electromagnetic energy. In this case, it was shown previously that the expression of χ , in the particular case of incident radiation on a heterogeneous matter(powder, dust, cl ...
and mutual-impedance probes
... Due to the S304 sensor size, the Ne and Te might be determined so long as λD was in the 0.5-6 m range. The sphere size, 8-10 cm in diameter, was much < λD. ...
... Due to the S304 sensor size, the Ne and Te might be determined so long as λD was in the 0.5-6 m range. The sphere size, 8-10 cm in diameter, was much < λD. ...
Simulations of Si and SiO2 Etching in SF6+O2 Plasma
... k3 = 1.00 × 104 s−1 , ω = 3500 s−1 . It is observed that the desorption frequency of SiF4 molecules has different values for Si and SiO2 etching. During PCE of SiO2 the desorption frequency of SiF4 molecules is markedly lower than that during PCE of Si in SF6 +O2 plasma. As the frequency of oscillat ...
... k3 = 1.00 × 104 s−1 , ω = 3500 s−1 . It is observed that the desorption frequency of SiF4 molecules has different values for Si and SiO2 etching. During PCE of SiO2 the desorption frequency of SiF4 molecules is markedly lower than that during PCE of Si in SF6 +O2 plasma. As the frequency of oscillat ...
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 ...
Full Text Report
... Atomic cross section data are generated using the ATBASE suite of codes [16]. Energy levels, photoionization cross sections, oscillator strengths, autoionization rates, and energy levels are calculated using a configuration interaction model with Hartree-Fock wavefunctions. Collisional coupling betw ...
... Atomic cross section data are generated using the ATBASE suite of codes [16]. Energy levels, photoionization cross sections, oscillator strengths, autoionization rates, and energy levels are calculated using a configuration interaction model with Hartree-Fock wavefunctions. Collisional coupling betw ...
Driven reconnection and bursty bulk flows
... NENL model has been quite successful in explaining many diverse observed features of substorm related changes in the magnetotail. Even though BBFs are positively correlated with the geomagnetic activity, there is no one-to-one correspondence between a substorm and BBF. Therefore, the NENL paradigm c ...
... NENL model has been quite successful in explaining many diverse observed features of substorm related changes in the magnetotail. Even though BBFs are positively correlated with the geomagnetic activity, there is no one-to-one correspondence between a substorm and BBF. Therefore, the NENL paradigm c ...
EUROPEAN ACADEMIC RESEARCH, VOL
... Pakistan air space (PAS) in term of complete parameters. Also it is essential to make result about atmosphere F2-layer ionosphere plasma. We present some probabilistic approaches that establish claim in atmosphere science the plasma turbulence for ionospheric Es-layer at Pakistan air space. To infer ...
... Pakistan air space (PAS) in term of complete parameters. Also it is essential to make result about atmosphere F2-layer ionosphere plasma. We present some probabilistic approaches that establish claim in atmosphere science the plasma turbulence for ionospheric Es-layer at Pakistan air space. To infer ...
Spectral-Type Trends: Absorption
... stellar luminosity or surface temperature. So, an X-ray emission trend would be very surprising. But stellar winds are stronger and denser for hotter and more luminous stars, so an X-ray hardness trend governed by wind attenuation is expected.) To explore the effect of wind absorption, we have devel ...
... stellar luminosity or surface temperature. So, an X-ray emission trend would be very surprising. But stellar winds are stronger and denser for hotter and more luminous stars, so an X-ray hardness trend governed by wind attenuation is expected.) To explore the effect of wind absorption, we have devel ...
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 ...
Longitudinal Asymmetry of the Jovian Magnetosphere
... the spin axis and the magnetic axis of Jupiter (Figure 1). degree of field distortion observed at a given point in the However, the same 10-hour modulation was subsequentlyre- nonrotating referenceframe. In particular, the distanceto the ported to be a feature of relativisticelectron fluxesobservedi ...
... the spin axis and the magnetic axis of Jupiter (Figure 1). degree of field distortion observed at a given point in the However, the same 10-hour modulation was subsequentlyre- nonrotating referenceframe. In particular, the distanceto the ported to be a feature of relativisticelectron fluxesobservedi ...
Gravitational lensing in presence of plasma O.Yu. Tsupko G.S. Bisnovatyi-Kogan
... Another law of angle deflection (significant for radio waves) -> another formula for magnification -> ratios of magnifications can be different for optical band and for radio band -> ratios of fluxes can be different for optical and for radio bands if light rays forming images travel through plasma ...
... Another law of angle deflection (significant for radio waves) -> another formula for magnification -> ratios of magnifications can be different for optical band and for radio band -> ratios of fluxes can be different for optical and for radio bands if light rays forming images travel through plasma ...