共查询到20条相似文献，搜索用时 31 毫秒
1.
S. S. Davydenko 《Geomagnetism and Aeronomy》2012,52(2):211-221
Exact distributions of the electric field and current density in the vicinity of the rotating magnetized planet are determined
within the planetary electric generator model. The model planetary plasma envelope is assumed to be inhomogeneous and consists
of an atmosphere, an ionospheric layer rotating with respect to the atmosphere, and a magnetosphere located beyond the ionosphere.
The model parameters, under which the influence of a large-scale flow of the ionospheric plasma on the electric field and
current in the lower atmosphere is significant are determined. It is shown that the ionospheric superrotation reduces the
electric field arising in the Earth’s lower atmosphere due to the planetary generator effect. 相似文献
2.
《Journal of Atmospheric and Solar》2007,69(3):288-302
This tutorial review deals with large-scale convection electric fields in Earth's inner magnetosphere and the particle populations that interact strongly with those fields, specifically the inner plasma sheet, ring current, and plasmasphere. We summarize the state of knowledge in the early 1970s, by which time most of the major observational features had been discovered and much of the basic theory had been developed. The review then focuses on how observational knowledge and theoretical understanding have increased since the early 1970s in several areas, specifically prompt-penetration electric fields; polarization jets (PJs), subauroral ionization drifts (SAIDs), and subauroral polarization streams (SAPS); ring current dynamics; and large-scale plasmasphere dynamics. 相似文献
3.
《Journal of Atmospheric and Solar》2007,69(14):1723-1738
Ion-cyclotron waves play important roles in planetary magnetospheres and are diagnostic of the processes operating in the magnetosphere and of the composition of the plasma producing the waves. At Jupiter, Io's exosphere interacts with the corotating magnetospheric plasma. At Saturn, the neutral torus around the E ring interacts with the corotating plasma. At the unmagnetized planets, Mars and Venus, the interaction is between the solar-wind flow and the planetary exosphere. A possible analog of these processes exists in the vicinity of the Earth's polar cusp where the shocked solar-wind plasma penetrates the Earth's exosphere. 相似文献
4.
美国利用IMAGE卫星的极紫外辐射（EUV）探测器对地球等离子体层进行了连续5年的遥感成像观测。由于IMAGE卫星数据是沿观测路径上的积分投影数据,并且存在地球“遮挡”、“阴影”、“数据缺失”等问题,无法直接利用传统的CT方法对等离子体层进行三维重建。本文利用地球磁场模型,基于地球等离子体层的物理性质,建立一个联系地球磁赤道面密度与投影数据的EUV成像模型,实现了从单个角度的EUV观测图像进行地球等离子层三维重构的方法。 相似文献
5.
Paul Melchior 《Surveys in Geophysics》1974,1(3):275-303
The main geometrical characteristics and mechanical properties of bodily tides are described, using the convenient elastic parameters of Love. The problem of the Earth's deformation is a problem of spherical elasticity of the sixth order. The importance of Earth tides in astronomy and geophysics is emphasized by their relation to the precession-nutation and tesseral tidal problems, the secular retardation of the Earth's speed of rotation due to the dissipation of energy in sectorial tides, the periodic variations of the speed of rotation due to zonal tides, the satellite orbit perturbations due to the Earth's potential variation, and the radial deformations in laser distance measurements. The possibility that dynamical effects would be produced in the Earth's liquid core was pointed out by Poincaré and developed by Jeffreys, Vicente, and Molodensky. An experimental confirmation is presented here. The role of the Earth tide phenomenon in gravimetry and oceanography is also described, as are the perturbing effects due to regional tectonic features. Instrumental developments are critical in the acquisition of precise data; the calibration problem is fundamental for a correct comparison with Earth models. 相似文献
6.
《Journal of Geodynamics》2010,49(3-5):219-225
Tidal forces due to the tide-raising potential deform the solid and fluid regions of the Earth, causing the Earth's inertia tensor to change, and hence causing the Earth's rate of rotation and length-of-day to change. Because both the tide-raising potential and the solid Earth's elastic response to the tidal forces caused by this potential are well-known, accurate models for the effects of the elastic solid body tides on the Earth's rotation are available. However, models for the effect of the ocean tides on the Earth's rotation are more problematic because of the need to model the dynamic response of the oceans to the tidal forces. Hydrodynamic ocean tide models that have recently become available are evaluated here for their ability to account for long-period ocean tidal signals in length-of-day observations. Of the models tested here, the older altimetric data-constrained model of Kantha et al. (1998) is shown to still do the best job of accounting for ocean tidal effects in length-of-day, particularly at the fortnightly tidal frequency. The model currently recommended by the IERS is shown to do the worst job. 相似文献
7.
The effects of the dayside and dusk plumes of the plasmasphere during the ring current recovery phase on the disturbance level
of the ground geomagnetic field horizontal component have been considered. It has been indicated that the geomagnetic field
horizontal component changes specifically and synchronously in the region corresponding to the plasmaspheric dayside plume.
Outside the plume the time variations in the geomagnetic field horizontal component pronouncedly differs. A spectral analysis
of disturbances in the geomagnetic field horizontal components in the range of geomagnetic pulsations indicated that the intensity
in the range of Pc4 pulsations increases at magnetic stations located on field lines corresponding to the dayside and dusk
plumes of the plasmasphere. These pulsations detected in the dynamic spectrum of the geomagnetic field horizontal components
in the dayside plume region of the plasmasphere, probably reflect the resonance oscillations of magnetic field lines in the
region of field-aligned currents at comparatively low altitudes. We assume that this is caused by the instability of field-aligned
currents originating as a result of the interaction between the ring current energetic ions and electromagnetic waves in the
region with a relatively dense background plasma of the dayside plume. 相似文献
8.
Alv Egeland 《Journal of Atmospheric and Solar》2009,71(17-18):1749-1755
More than one hundred years ago Kristian Birkeland (1867–1917) first addressed the question as to why auroras appear overhead when the Earth's magnetic field is disturbed. He laid foundations for our current understanding of geomagnetism and polar auroras. For the first time cosmic phenomena were scaled and simulated in a laboratory. Birkeland's terrella experiments were ingenious. Even though the famous Lord Kelvin, in 1892, wrote that no matter passes between the Sun and the Earth, Birkeland's first auroral theory from 1896 is based on charged particle of solar origin, illustrated by the following quotation: “the auroras are formed by corpuscular rays drawn in from space, and coming from the sun”. Thus, the year 1896 marks the founding of space plasma physics. His most enduring contribution to auroral physics was his recognition that field-aligned currents are needed to couple auroral phenomena in the upper atmosphere to interplanetary space. The existence of field-aligned currents was controversial and disputed vigorously among scientists for more than 50 years. During The Birkeland Symposium in 1967 it was unanimously proposed that field-aligned currents in space should be called “Birkeland currents”, which was accepted by the International Union for Geomagnetism and Aeronomy. Today, plasma physicists strongly believe that many significant cosmic phenomena result from streams of Birkeland currents. 相似文献
9.
10.
Robert R. Newton 《Surveys in Geophysics》1973,1(2):123-145
In this paper, we review the current state of knowledge about the acceleration of the Earth's spin, and about the closely related acceleration of the Moon. It is now established at a high confidence level that the acceleration of the Moon, when taken respect to Universal time, has changed by a large amount, and that it has even changed sign, within historic times. This almost certainly means that the acceleration of the Earth's spin has also changed by a large amount. At present we do not have enough information to say whether the changes have been in the contributions from tidal friction, in the contributions that do not arise from tidal friction, or both. Further, we do not know yet whether or not the variations in the Earth's rotation can account for the observed fluctuations in the longitudes of the Sun, the Moon, and the planets. 相似文献
11.
《Journal of Atmospheric and Solar》2002,64(7):795-804
We report on the recent studies on the long-term influence of cosmic rays on the Earth's environment. While on short time-scales solar activity is the driver for atmospheric changes suspected to be due to cosmic rays, for long time-scales the heliosphere, i.e. the circumsolar region occupied by the expanding part of the Sun's atmosphere, has to be considered. The heliosphere is identified as an important shield against interstellar influences and hazards. It has been demonstrated by quantitative modelling that a change of the interstellar medium surrounding the heliosphere as a result of the Sun's quasi-Keplerian motion around the galactic center triggers significant changes of planetary environments caused by enhanced fluxes of neutral atoms as well as by the increased cosmic ray fluxes. We give a compilation of recent space science results of interest to the atmospheric science community. 相似文献
12.
Masaki Matsushima 《地球物理与天体物理流体动力学》2013,107(6):630-642
A thermal diffusive process in the Earth's core is principally enhanced by small-scale flows that are highly anisotropic because of the Earth's rapid rotation and a strong magnetic field. This means that a thermal eddy diffusivity should not be a scalar but a tensor. The effect of such anisotropic tensor diffusivity, which is to be prescribed, on dynamics in the Earth's core is investigated through numerical simulations of magnetoconvection in a rapidly rotating system. A certain degree of anisotropy has an insignificant effect on the character, like kinetic and magnetic energies, of magnetoconvection in a small region with periodic boundaries in the three directions. However, in a region with top and bottom rigid boundary surfaces, kinetic and magnetic energies of magnetoconvection can be altered by the same degree of anisotropy. This implies that anisotropic tensor diffusivity affects on dynamics in the core, in particular near the boundary surfaces. 相似文献
13.
Ana G. Elias 《Journal of Atmospheric and Solar》2009,71(14-15):1602-1609
The Earth's magnetic field presents long-term variations with changes in strength and orientation. Particularly, changes in the dip angle (I) and, consequently, in the sin(I)cos(I) factor, affect the thermospheric neutral winds that move the conducting plasma of the ionosphere. In this way, a lowering or lifting of the F2-peak (hmF2) is induced together with changes in foF2, depending on season, time and location. A simple theoretical approximation, developed in a previous work, is extended to a worldwide latitude–longitude grid to assess hmF2 and foF2 trends due to Earth's magnetic field secular variations. Compared to the greenhouse gases effects over the ionosphere, the Earth's magnetic field may be able to produce stronger trends which vary with season, time and location. However, to elucidate the origin of F2-region trends, long-term variations in the three possible known mechanisms should be considered altogether—greenhouse gases, geomagnetic activity and Earth's magnetic field. 相似文献
14.
Claudio Vita-Finzi 《Journal of Atmospheric and Solar》2010,72(2-3):139-142
Measurements of solar EUV irradiance show, besides the ～11-year Schwabe cycle, a series of oscillations with a ～27-day period. They are generally explained by the passage of active regions across the solar surface resulting from the Sun's rotation, but the calculated amplitude underestimates the observed long-term variation in irradiance (Lean 1991). The variant of this model proposed here is modulation of EUV emission from the corona by rotation of the Sun's radiative zone. The response would be immediate, raising the prospect of short-term forecasting of EUV effects on space weather and on the Earth's atmospheric circulation. 相似文献
15.
From the data on the cold plasma measurements onboard the INTERBALL-1 spacecraft (1995–2000), the plasmapause positions determined from the most frequently used formal criterion—a fivefold or higher decrease in plasma density with an increase in the L-shell by 0.5—and visually from the measured energy spectra of thermal protons have been analyzed and compared. The difference in the results of the both empiric techniques makes it possible to estimate the thickness of the boundary layer of the plasmasphere. The model of the Earth’s plasmasphere developed earlier by the authors (Verigin et al., 2012; Kotova et al., 2015) based on the theoretical expressions makes it possible to reconstruct the plasma distribution throughout the plasmasphere from the measurements along a single pass of the orbiter and to find the plasmapause position defined as the last closed stream line. Comparison of the plasmapause position obtained with empirical techniques to the position of this boundary calculated with physically based models of the plasma distribution in the plasmasphere has shown that the modeled position of the plasmapause approximately coincides with that determined from the formal criterion described above. 相似文献
16.
Chao-Ho Sung 《地球物理与天体物理流体动力学》2013,107(1):179-182
Abstract Sufficient conditions for stability are established for the magnetic field problem of the Earth's core considered by Braginsky. 相似文献
17.
P. A. Sedykh 《Geomagnetism and Aeronomy》2011,51(7):912-922
The magnetosphere and ionosphere are coupled into a power circuit by field-aligned currents. If there were only Hall current
in the ionosphere, the problem of magnetosphere-ionosphere interaction would not have arisen. Field-aligned currents could
be seen as emerging as a result of the break in the magnetospheric current across the tail, since the Hall current is divergence-free
and does not perform any work. In fact, the current in the ionosphere is complex. It always has a Pedersen component, and
the ionosphere is a real energy consumer. Together with energy, an extrinsic electrical current should flow into the ionosphere.
The current coming from the generator in front of the bow shock is a part of the extrinsic current. The aim of this paper
is to generalize the previously obtained partial solution to the problem of magnetosphere-ionosphere interactions in the region
of auroral electrojets, also taking into account the generation of the extrinsic current in front of the bow shock. 相似文献
18.
19.
Abstract It is shown that in the Earth's core, where the geodynamo is at work (and is supplied with energy by the prevailing unstable density stratification), a buoyancy instability of a local character exists which is highly supercritical. This instability results in fully developed turbulence dominated by small scale vortices. The influence of the Earth's rotation and of the magnetic field produced by the geodynamo makes this small scale turbulence highly anisotropic. A qualitative picture of this local anisotropic turbulence is devised and the main parameters characterizing it are estimated. Expressions for the turbulent diffusivity are developed and discussed. 相似文献
20.
Estimation of the size of earthquake preparation zones 总被引：8，自引：0，他引：8
During the earthquake preparation a zone of cracked rocks is formed in the region of a future earthquake focal zone under the influence of tectonic stresses. In the study of the surrounding medium this region may be considered as a solid inclusion with altered moduli. The inclusion appearance causes a redistribution of the stresses accompanied by corresponding deformations. This paper deals with the study of deformations at the Earth's surface, resulting from the appearance of a soft inclusion. The Appendix contains an approximate solution of the problem for a soft elastic inclusion in an elastic half-space. It is assumed that the moduli of the inclusion differ slightly from those of the surrounding medium (by no more than 30%). The solution permits us to calculate the deformations at the Earth's surface for the inclusion with an arbitrary heterogeneity and anisotropy. The problem is solved by the small perturbation method. The calculation is made for a special case of a homogeneous isotropic inclusion where only the shear modulus decreases. The shear stresses act at infinity. The equations are deduced for the estimation of deformations and tilts at the Earth's surface as a function of the magnitude of the preparing earthquake and the distance from the epicentre. Comparison has shown a satisfactory agreement between the theoretical and field results. Let us assume that the zone of effective manifestation of the precursor deformations is a circle with the centre in the epicentre of the preparing earthquake. The radius of this circle called ‘strain radius’ may be calculated from the equation $$\rho = 10^{0.43M} km,$$ where M is the magnitude. It was shown that the precursors of other physical nature fall into this circle. 相似文献