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281.
Mitchell Donald G. C:son Brandt Pontus Roelof Edmond C. Hamilton Douglas C. Retterer Kyle C. Mende Steven 《Space Science Reviews》2003,109(1-4):63-75
The magnetospheric O+ population in the 52–180 keV range during storms is investigated through the analysis of energetic neutral atom (ENA) images. The images are obtained from the high energy neutral atom (HENA) imager onboard the IMAGE satellite. At each substorm onset following the commencement of a geomagnetic storm the oxygen ENA display ~30 min intense bursts. Only very weak corresponding features in the 60–119 keV hydrogen ENA can be occasionally seen. The dominating fraction of the oxygen ENA emissions are produced when O+ ions mirror/precipitate at low altitudes, where the number density of the neutral atmosphere is high. During the storm we observed several bursts of oxygen ENA, but it is still not clear how much the O+ content of the ring current increases during the storm main phase. Our observations suggest that the responsible injection mechanism is mass-dependent and scatters the pitch angles. This leads us to favor a non-adiabatic mechanism proposed by (Delcourt, 2002). 相似文献
282.
We find the forms of the orbits in a self-consistent galactic model generated by a N-body simulation of the collapse of a protogalaxy. The model represents a stationary elliptical galaxy of type E5, which is approximately axisymmetric around its longest axis. The orbits are of three main types, box orbits (including box-like orbits), tube orbits and chaotic orbits. The box or box-like and tube orbits are represented by closed invariant curves on a Poincaré surface of section. The forms of the orbits and of the invariant curves can be explained by a third integral of motion I, that is given by the Giorgilli (1979) computer program. The nonresonant form of the third integral explains the box orbits, while a resonant form of this integral explains both the box orbits and the 1:1 tube orbits. The N-body model gives the distribution of velocities F, which is an exponential of the third integral. 相似文献
283.
Quintessence – the energy density of a slowly evolving scalar field – may constitute a dynamical form of the homogeneous dark energy in the universe. We review the basic idea and indicate observational tests which may distinguish quintessence from a cosmological constant. 相似文献
284.
285.
Peter C. Thomas Joseph Veverka Michael F. A’Hearn Lucy Mcfadden Michael J. S. Belton Jessica M. Sunshine 《Space Science Reviews》2005,117(1-2):193-205
The Deep Impact mission will provide the highest resolution images yet of a comet nucleus. Our knowledge of the makeup and
structure of cometary nuclei, and the processes shaping their surfaces, is extremely limited, thus use of the Deep Impact
data to show the geological context of the cratering experiment is crucial. This article briefly discusses some of the geological
issues of cometary nuclei. 相似文献
286.
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288.
铝-锂合金的真空熔炼 总被引:2,自引:0,他引:2
在ZG-25型中频感应真空炉中进行了铝-锂合金的熔炼与铸锭。真空度为66Pa。考察了普通石墨坩埚、氧化铝坩埚,以及氧化锌涂料、氮化硼涂料与铝-锂熔体的反应。抄到了在真空下控制铝-锂熔体中锂含量的方法。在不使用钛-硼细化剂的条件下,铸锭呈细小等轴晶组织,其成分均匀,夹杂物极少。真空熔炼可使合金中的氢、钾,钠等杂质含量显著地降低。 相似文献
289.
在用氢泡法观测凹半球降落伞模型的流场时,我们还用单分力应变天平对其进行了阻力测量。通过测量及理论分析,得出加速起动期间最大阻力F_(max)和附加质量引起的力F_a之比与无量纲参数U_(max)~2/ad之间的关系。此外,还研究了与最大阻力有联系的一些流动现象。该试验有助于深入了解降落伞的动稳定性与开伞动载方面的内在联系。 相似文献
290.
Acceleration of the solar wind 总被引:2,自引:0,他引:2
In this review, we discuss critically recent research on the acceleration of the solar wind, giving emphasis to high-speed solar wind streams emanating from solar coronal holes. We first explain why thermally driven wind models constrained by solar and interplanetary observations encounter substantial difficulties in explaining high speed streams. Then, through a general discussion of energy addition to the solar wind above the coronal base, we indicate a possible resolution of these difficulties. Finally, we consider the question of what role MHD waves might play in transporting energy through the solar atmosphere and depositing it in the solar wind, and we conclude by examining, in a simple way, the specific mechanism of solar wind acceleration by Alfvén waves and the related problem of accelerating massive stellar winds with Alfvén waves.Paper presented at the IX-th Lindau Workshop The Source Region of the Solar Wind.On leave from the Auroral Observatory, Institute of Mathematical and Physical Sciences, University of Tromsø, N-9001 Tromsø, Norway.The National Center for Atmospheric Research is sponsored by the National Science Foundation. 相似文献