共查询到20条相似文献，搜索用时 93 毫秒
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B.J. Kellett R. Bingham R.A. Cairns V. Tsikoudi 《Monthly notices of the Royal Astronomical Society》2002,329(1):102-108
In this paper we review four different types of X-ray and/or radio observations of active late-type stars. We then consider if a single magnetic source configuration – a toroidal dipole magnetic trap – can possibly explain these various different observations. We conclude that, indeed, dipole magnetic confinement (similar to the magnetic configurations of the Earth's radiation belts and the case of Jupiter and the Io torus) can explain all the diverse observational data. We take this to be very strong observational support for this type of magnetic confinement scheme. We also consider that this magnetic configuration is only likely to be established and maintained in the most active stars. 相似文献
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Contaminated electrode effects of a retarding potential trap on the temperature measurement are investigated in laboratory plasma. It is shown that poorly conductive layers on the electrode surface modify the v-i curves. This contamination effect of RPT electrode can be overcome either by increasing the sweep-rate of the grid potential or by the use of a large effective sheath resistance. 相似文献
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We consider the kinetic problem of charged-particle acceleration in a magnetic trap with converging magnetic mirrors. We show that for a positive electrostatic potential of the trap plasma relative to the mirrors, the efficiency of confinement and acceleration increases for electrons and decreases for ions. 相似文献
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Gui-Yun Liang Hui-Gang Wei Da-Wei Yuan Fei-Lu Wang Ji-Min Peng Jia-Yong Zhong Xiao-Long Zhu Mike Schmidt Günter Zschornack Xin-Wen Ma Gang Zhao 《天文和天体物理学研究(英文版)》2018,(1)
Spectra are fundamental observation data used for astronomical research,but understanding them strongly depends on theoretical models with many fundamental parameters from theoretical calculations.Different models give different insights for understanding a specific object.Hence,laboratory benchmarks for these theoretical models become necessary.An electron beam ion trap is an ideal facility for spectroscopic benchmarks due to its similar conditions of electron density and temperature compared to astrophysical plasmas in stellar coronae,supernova remnants and so on.In this paper,we will describe the performance of a small electron beam ion trap/source facility installed at National Astronomical Observatories,Chinese Academy of Sciences.We present some preliminary experimental results on X-ray emission,ion production,the ionization process of trapped ions as well as the effects of charge exchange on the ionization. 相似文献
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The possibility of H3+ playing a role as a sink for noble gases has been investigated in the case of Argon. Elaborate quantum methods (ab initio Coupled Cluster and density functional BH&HLYP levels of theory) have been shown to reproduce the rotational constants within 0.3% together with the only known IR frequency on the test case of Ar…D3+. Dissociation energies of (Ar)n…H3+ as a function of cluster size, i.e. 7.2 (n=1), 3.7 (n=2), 3.6 (n=3), 1.6 (n=4), 1.7 (n=5) kcal/mol, follow the pattern established experimentally for (Ar)n…H3+ and (H2)n…H3+ series. Rotational constants and harmonic frequencies of (Ar)n…H3+ (n=1-3) are presented. 相似文献
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B. S. Sandhu 《Earth, Moon, and Planets》1992,56(2):165-171
Whipple's icy conglomerate model of cometary nucleus enjoyed wide acceptance and a long successful life. Considerable changes were brought to it based on the guidance of observational evidences and theoretical considerations. After the fractal model and the rubble pile model, icy glue model brought major alterations. But the concept of porous refractory boulders of the icy glue model seems to be quite unrealistic and unexplicable. Viewing minutely the process of the formation of comets a new model is proposed in which in the outskirts of the solar accretion disc ice and dust mixture formed small particles, which agglomerated to give large particles. These large particles further agglomerated to form tens of meters sized boulders. In this model it is assumed that up to the formation of boulders, ice and dust mix glue was consumed almost completely. The boulders collide with one another and get glued with the help of the glue formed due to the breakage of small particles at the interface, and form a boulder complex of the size of hundreds of meters. These complexes of boulders along with small boulders come together to form the cometary nucleus. 相似文献
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Robertson-Walker cosmological model with bulk viscosity is investigated with equation of statep=(–1). The cosmological solution of the model is obtained with the help of the special law of variation for Hubble's deceleration parameter. Some physical consequences of the solution is studied pertaining to two extreme cases of the equation of state. 相似文献
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M. Yu. Reshetnyak 《Solar System Research》2014,48(3):182-193
Using the Lagrangian approach, the author considered the temporal evolution of an ensemble of interacting magnetohydrodynamic cyclones, obeying equations of the Langevin type, in a rotating medium. The problem is topical for fast-rotating convective objects: cores of planets and a number of stars, where the Rossby numbers are much less than unity and the geostrophic balance of forces is observed. In this work, results of simulation are given both for the two-dimensional case, when axes of cyclones can rotate only in the vertical plane, and for the three-dimensional case when the axes are rotating by two angles. It is shown that a change in the heat flux on the shell boundary impacts the frequency of reversals of the mean dipole magnetic field, which agrees with results of simulation in three-dimensional models of a planetary dynamo. Applications of the model for the giant planets are considered, and an explanation of certain episodes of the geomagnetic field in the past is offered. 相似文献
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We present exact solutions of a Bianchi type VI0 viscous fluid cosmological model. It is a generalization of the model proposed by Banerjee and Santos (1983) for Bianchi type I. 相似文献
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Terry W. Edwards 《Astrophysics and Space Science》1970,7(1):151-159
A Population II, 1.3M
, pre-helium flash, red-giant model is investigated with respect to the influence of inclusion of relativistic gas characteristics, i.e., the equations of state, entropy, specific heats, and the adiabatic gradient. Little change is found in the observable properties of the model, but slightly large changes are found in the interior properties, the most important of which is the narrowing of the already thin radiative zone between the hydrogen burning shell and the extensive outer convective envelope from 9.6 to 8.0 density scale heights. 相似文献
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M. I. Wanas 《Astrophysics and Space Science》1989,154(2):165-177
The field equations of the generalized field theory constructed by Mikhail and Wanas have been applied to a well-established geometrical structure given earlier by H. P. Robertson in connection with the cosmological problem. A unique solution, representing a specified expanding Universe (withq
0=0, 0=0.75,k=–1) has been obtained. The model obtained has been compared with cosmological observations and with FRW-models of relativistic cosmology. It has been shown that the suggested model is free of particle horizons. The existence of singularities has been discussed.The two cases, when the associated Riemannian-space has a definite or indefinite metric are considered. The case of indefinite metric with signature (+ – – –) is found to be characterized byk=–1, while the case of +ve definite metric is characterized byk=+1. Apart from that difference, the two cases give rise to the same cosmological parameters. It has been shown that energy conditions are satisfied by the material contents in both cases. 相似文献
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M. K. Das 《Astrophysics and Space Science》1985,116(1):131-139
Slowly-rotating partially-degenerate standard models have been computed for different values of central degeneracy parameter
c
. For increased central degeneracy the models get more distorted, since the central condensation increases and this results in more severe rotational effects in the outer layers of the configuration. 相似文献
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Robertson—Walker cosmological models with bulkviscosity are investigated explicitly with equation of statep=(-1). In particular, the physical nature of the extreme cases, i.e., degenerate vacuum bulkviscous fluid model and bulkviscous stiff fluid model are studied in detail. 相似文献
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George Driver Nelson 《Solar physics》1978,60(1):5-18
We present a two-dimensional, nearly flux constant solar atmosphere which includes a physical model of granulation. If the inhomogeneous character of the solar photosphere is neglected in the construction of empirical models, the result is an underestimate of the temperature gradient in the layers below 0.5 and an overestimate of the convective flux penetration into the observable layers. The two-dimensional model adequately reproduces the mean limb darkening, the magnitude and center-to-limb variation of the intensity fluctuations, and the rms vertical and horizontal convective velocities. 相似文献