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121.
在相对论性框架下,研究了冷离子流产生的右旋共振模,非共振模电磁不稳定性的特征结果表明,非共振模不稳定性增长率受离子流初始参数影响较大,而右旋共振模的增长率则受离子流初始参数影响较小。此结果可应用于太阳高能离子流通过低日冕区和地球磁层辐射带俘获的高能质子情形。 相似文献
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The magnetopause is in continuous motion and shock waves and impulsive acceleration events can occur. As an example, we show
that the interaction of an interplanetary shock with the bow shock can generate a shock wave that after passing through the
magnetosheath can interact with the magnetopause. In fluid dynamics, when a shock wave encounters a fluid discontinuity, the
interface may become unstable and form bubbles and spikes. We consider this Richtmyer-Meshkov instability in magnetohydrodynamics.
At the dayside magnetopause, the instability tends to be stabilized by the magnetic field. However, the shock wave interaction
can initiate magnetic field reconnection for the southward IMF, which may be important in strong interplanetary shock events.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
123.
G. Uma P.S. Brahmanandam V.K.D. Srinivasu D.S.V.V.D. Prasad P.V.S. Rama Rao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1736-1743
In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased. 相似文献
124.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(6):2954-2966
The Two-stream Instability (TSI) generation is studied analytically in the lunar ionosphere. The TSI is a tiny perturbation in the electron plasma density, due to which an electric field grows with time and this growth is facilitated by the electron plasma in the background. In lunar ionosphere, the TSI comes into existence when the solar wind interacts unhindered with the tenuous lunar electron plasma in the surface bound exosphere. In this study, the conditions which allow the TSI to form and the subsequent instability growth with time i.e. the growth factor, is estimated. Initially, the threshold condition for the TSI to take place is determined. Thereafter, the solar wind and lunar plasma parameter contribution to trigger TSI is investigated along with the effect of these parameters in the evolution of TSI. The plasma TSI evolution with the passage of time is also depicted in phase space diagram with Particle-In-Cell simulations. 相似文献
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部分球壳分布离子流激发的电磁不稳定性 总被引:1,自引:1,他引:0
在离子环束流和低频电磁波相互作用的过程中廓了环束流将演化成具有投掷角展宽的部分球壳速度分布离子流,其投掷角展宽随时间增大,低频右旋电磁不稳定性增长率峰值,总的说来也逐渐增大,并向高频短波方向移动,与此相反,低频左旋电磁不稳定性增长率峰值,当投掷 角展宽等于0时,大于右旋不稳定性峰值,但随着投掷角展宽增加而迅速低于右 性增长率峰值,并向工波方向移动。 相似文献
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为研究空气节流时序对超燃冲压发动机点火和火焰稳定的影响,本文通过实验方法研究了13个状态的煤油燃料超燃冲压发动机的燃烧特性,煤油燃烧通过先锋氢气和节流空气增强稳定性。通过两个固定位置的压力传感器来监测火焰稳定状态,采用纹影和OH-PLIF相结合的测量手段,获得了流场结构和火焰发展信息。发动机入口来流条件为Ma = 2.0,总温950 K,总压0.82 MPa。在空气节流的作用下,煤油被先锋火焰引燃;在先锋氢撤除后,煤油仍然可以稳定燃烧。在扩张段中,空气节流和燃烧共同作用产生的激波串移动速度约为52 m/s,但在凹槽内其速度仅为3.7 m/s。通过监测点压力变化情况可以区分所研究状态的火焰稳定与否,通过对13个研究状态的考察,获得了火焰稳定临界曲线。当所研究状态点在临界曲线右上方区域时,火焰状态稳定;当所研究状态点在临界曲线左下方区域时,火焰将被吹熄;当所研究状态点在临界曲线上时,火焰不稳定,在空气节流撤除之前将被吹熄。 相似文献