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321.
为了降低超音速飞行时产生的波阻,通过斜激波基本公式建立了设计马赫数为2的布泽曼双翼翼型,借助CFD软件计算其升阻特性,并与菱形单翼翼型作对比,同时分析了在非设计条件下布泽曼双翼翼型的壅塞问题.结果表明,布泽曼双翼在设计马赫数下,其波阻较传统菱形单翼降低90%,壅塞问题也得到很好地解决. 相似文献
322.
J. Büchner 《Space Science Reviews》2006,124(1-4):345-360
Reconnection is a major commonality of solar and magnetospheric physics. It was conjectured by Giovanelli in 1946 to explain
particle acceleration in solar flares near magnetic neutral points. Since than it has been broadly applied in space physics
including magnetospheric physics. In a special way this is due to Harry Petschek, who in 1994 published his ground breaking
solution for a 2D magnetized plasma flow in regions containing singularities of vanishing magnetic field. Petschek’s reconnection
theory was questioned in endless disputes and arguments, but his work stimulated the further investigation of this phenomenon
like no other. However, there are questions left open. We consider two of them – “anomalous” resistivity in collisionless
space plasma and the nature of reconnection in three dimensions. The CLUSTER and SOHO missions address these two aspects of
reconnection in a complementary way -- the resistivity problem in situ in the magnetosphere and the 3D aspect by remote sensing of the Sun. We demonstrate that the search for answers to both questions
leads beyond the applicability of analytical theories and that appropriate numerical approaches are necessary to investigate
the essentially nonlinear and nonlocal processes involved. Necessary are both micro-physical, kinetic Vlasov-equation based
methods of investigation as well as large scale (MHD) simulations to obtain the geometry and topology of the acting fields
and flows. 相似文献
323.
The possibility of remote diagnostics of coronal structures with impulsively-generated short-period fast magnetoacoustic wave
trains is demonstrated. An initially broad-band, aperiodic fast magnetoacoustic perturbation guided by a 1D plasma inhomogeneity
develops into a quasi-periodic wave train with a well-pronounced frequency and amplitude modulation. The quasi-periodicity
results from the geometrical dispersion of the modes, determined by the transverse profile of the loop, and hence contains
information about the profile. Wavelet images of the wave train demonstrate that their typical spectral signature is of a
“crazy tadpole’’ shape: a narrow spectrum tail precedes a broad-band head. The instantaneous period of the oscillations in
the wave train decreases gradually with time, with a mean value of several seconds for typical coronal values. The period
and the spectral amplitude evolution are determined by the steepness of the transverse density profile and the density contrast
ratio in the loop, which offers a tool for estimation of the sub-resolution structuring of the corona. 相似文献
324.
S. Lepidi L. CafarellaM. Pietrolungo L. Santarelli 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
A statistical analysis of low frequency geomagnetic fluctuations at the two Antarctic stations Mario Zucchelli Station (geographic coordinates: 74.7°S, 164.1°E; corrected geomagnetic coordinates: 80.0°S, 306.8°E) and Dumont D’Urville (geographic coordinates: 66.7°S, 140.0°E; corrected geomagnetic coordinates: 80.4°S, 236.0°E) is shown. The analysis focuses on power spectra, coherence and phase difference between the stations, which are both located in the polar cap, with a 5-h magnetic local time displacement along a geomagnetic parallel; in this situation, the phase difference between geomagnetic fluctuations indicates the direction of their azimuthal propagation. Coherent fluctuations have been found to occur preferably when both stations are on the same side (dawnward or duskward) with respect to the polar cusp; moreover, around local magnetic midnight, they occur essentially during open magnetospheric conditions. The phase difference for coherent fluctuations indicates a propagation direction away from local geomagnetic noon and midnight. Also the analysis of three individual pulsation events, occurring at different times during the day, is shown; they are characterized at the two stations by simultaneous, coherent fluctuations, whose phase difference finds correspondence with the statistical behaviour. 相似文献
325.
Y. Le Coq J.A. Retter S. Richard A. Aspect P. Bouyer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We analyze the advantages of using ultra-cold coherent sources of atoms for matter-wave interferometry in space. We present a proof-of-principle experiment that is based on an analysis of the results previously published in Richard et al. (2003) from which we extract the ratio h/m for 87Rb. This measurement shows that a limitation in accuracy arises due to atomic interactions within the Bose–Einstein condensate. Finally we discuss the promising role of coherent-matter-wave sensors, in particular inertial sensors, in future fundamental physics missions in space. 相似文献
326.
E. Echer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(9):1030-1037
Foreshock and magnetosheath waves in Uranus and Neptune magnetospheres are studied in this work with wavelet analysis. In order to conduct this study, Voyager-2 magnetometer 3-s averaged data are used. The Morlet wavelet transform is applied to the magnetic field vector data. Waves present in the magnetosheath and foreshock regions are highly non-stationary, showing large amplitude variations. It was found that the dominant periods of these waves are longer than the H+ cyclotron period. Overall, high frequency waves are seen near the bow shock crossing and low frequency oscillations near the magnetopause crossing. It can be concluded that non-stationary foreshock and magnetosheath planetary waves can be well characterized with wavelet analysis. 相似文献
327.
R.P. Patel A.K. Singh S. Singh R. Singh K. Singh R.P. Singh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1699-1703
VLF emissions such as hiss, chorus, pulsing hiss, triggered emissions observed at Varanasi (geom. lat. = 14° 55′ N, long. = 153° 55′ E) are reported. An attempt has been made to explain the dynamic spectra in terms of the generation mechanism and propagation through the inhomogeneous magnetoplasma. It is noted that the reported events have propagated along different L-values in the magnetosphere, although they have been recorded at the same station. The ULF waves propagating along geomagnetic field lines modulate the growth rate of VLF waves, which results in the pulsation of VLF hiss intensity. The pulsating growth rate has been computed. 相似文献
329.
In this paper advances on study of middle and upper atmosphere and their cou pling with lower atmosphere in China in recent two years are briefly reviewed.This review emphasized three aspects, ie. (1) analysis and observation of mid and upper atmosphere over China; (2) theoretical and modelling study of grav ity wave activities in middle atmosphere and their relation to lower atmospheric processes; (3) coupling between the stratosphere and troposphere. 相似文献
330.
栅格翼空气动力特性的计算与分析 总被引:6,自引:3,他引:6
将涡格法推广应用于计算外形复杂的蜂窝式栅格翼的气动特性,给出了亚、跨、超音速流中,栅格翼升力,力矩和阻力特性以及载荷分布,并分析了空气动力特点及几何参数的影响。计算结果表明,栅格翼作为一种新型的承力稳定面和控制面,在某些方面优于传统单翼,修正提出了空气动力等效条件,并通过计算进行了验证。 相似文献