[PDF] Top 20 Descuentos por Servicios No Regulados en el Diseño de la Empresa Modelo
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Magnetic turbulence in and around the Earth's magnetosphere
... Magnetic turbulence in the high altitude cusp, observed from Cluster spacecraft (Nykyri et ...pens around the proton ...bient magnetic field that range from parallel to perpendicular (Nykyri ... See full document
24
Substorm time magnetic field perturbations in the polar magnetosphere: POLAR observations
... the magnetic field in the inner magnetosphere undergoes dipolarization after the expansion onset (see, ...inner magnetosphere exerts the pressure gradient force directed away from it; in the ... See full document
6
Trapped positron flux formation in the innermost magnetosphere of the Earth
... Nuclear interactions of cosmic ray protons with the Earth’s atmosphere are a well-known source of charged and neutral energetic particles in the magnetosphere. These in- teractions take place in the innermost ... See full document
6
Scale similarity of MHD turbulence in the Earth’s core
... = 7.29 × 10 −5 rad/s). No one knows what arises from the obvious difference. To understand the realistic Earth’s dynamo, much smaller Ekman numbers and much larger Rayleigh numbers must be adopted in numerical ... See full document
26
The anisotropy of local turbulence in the Earth’s core
... buoyancy-driven turbulence in the core by direct numerical simulation ...local turbulence considered here is so small, of the or- der of kilometer (see below), that it is impossible to resolve it by global ... See full document
106
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling
... non-stationary magnetic fluctuations within sliding overlapping ...of turbulence in the solar wind is typi- cally less than a ...magnetohydrodynamic turbulence is of the order of some ...of ... See full document
13
On the validity of Akasofu’s ε parameter and of the Vasyliunas et al general formula for the rate of solar wind magnetosphere energy input
... interplanetary magnetic field (IMF) is assumed to be expressed by the combination of B, the magnitude of the IMF, and sin(θ/2), where θ is the clock angle, or by the combination of B T = ( By 2 + Bz 2 ) 1 / 2 , the ... See full document
11
Concentration of electrostatic solitary waves around magnetic nulls within magnetic reconnection diffusion region: single event based statistics
... single magnetic reconnection ...ESWs around the magnetic null-pairs within the magnetic reconnection ion diffusion region of Earth's magnetosphere on 10 September ...observed ... See full document
191
Electrodynamics in the duskside inner magnetosphere and plasmasphere during a super magnetic storm on March 13–15, 1989
... the magnetic activ- ity in the inner ...the earth during the early recovery ...the magnetic field in the plasmasphere region, in addition to the sweeping out of plasma due to the mag- netospheric ... See full document
10
Characterization of high-intensity, long-duration continuous auroral activity (HILDCAA) events using recurrence quantification analysis
... the Earth and beyond (Kivelson and Russell, ...tary magnetic field (IMF) presenting a predominantly south- ward orientation, in the geocentric solar magnetosphere ref- erence system, merges into the ... See full document
12
Turbulent processes in the Earth's magnetotail: spectral and statistical research
... Besides, magnetic reconnection can involve tur- bulence, but one should not forget about the work of Speiser (1970) describing the magnetic reconnection without noise ...for magnetic reconnection and ... See full document
38
Turbulence in a global magnetohydrodynamic simulation of the Earth’s magnetosphere during northward and southward interplanetary magnetic field
... Theoretical analyses indicate that a turbulent state features three ranges in the power spectral density (PSD), a driv- ing (or energy-containing) scale at the longest wavelengths (timescales) at which energy is supplied ... See full document
31
Electron hybrid code simulation of whistler mode chorus generation with real parameters in the Earth’s inner magnetosphere
... the magnetic field inho- mogeneity along a field line is an important factor con- trolling the spectral properties of ...real magnetosphere, and therefore larger magnetic field inhomogeneities have ... See full document
285
The dynamical behavior of the earth’s magnetosphere based on laboratory simulation
... The continuous flow of the tail current near the earth after the solarwind disappearance is related to the effective current confinement of the ring current particles. The confinement time is consistent with the ... See full document
14
Magnetodisc modelling in Jupiter's magnetosphere using Juno magnetic field data and the paraboloid magnetic field model
... the magnetic field is domi- nated by the magnetodisc and the planetary ...outer magnetosphere the field becomes strongly influenced by ex- ternal conditions in the solar wind, and although in some cir- ... See full document
20
Electric, Magnetic and Gravitation Field of the Earth
... Ferromagnetic Hypothesis of the Magnetic Field of the Earth. It is known from physics that under certain thermodynamic conditions some substances can change to the ferromagnetic state, their magnetic ... See full document
65
Earth’s Magnetic Field for Spacecraft Attitude Control Applications (TECHNICAL NOTE)
... earth’s magnetic field, and the results are verified with one of the standard ...earth’s magnetic field is transformed into the body coordinates of the spacecraft in order to be used in attitude control ... See full document
102
On the maximum energy of protons in the hotspots of AGN jets
... as usually assumed. By equating the acceleration and syn- chrotron cooling timescales, the mean free path of E e,max - electrons is greater than the maximum value imposed by plasma physics for reasonable values of the ... See full document
6
Time scales of close in exoplanet radio emission variability
... The longer time-scale is most apparent in systems where the or- bital and stellar rotation periods are similar in length. This results in a very long synodic period. In the most extreme case, when the stel- lar rotation ... See full document
25
Magnetic reconnection and intermittent turbulence in the solar wind
... 3 s resolution magnetic field measure- ments from the Magnetic Field Investigation (MFI) [46] and proton moments from the 3D Plasma Analyzer (3DP) [47] onboard the Wind ...the magnetic field ... See full document
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