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11.
A. Aran B. Sanahuja D. Lario 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2333-2338
We present a preliminary version of a potential tool for real time proton flux prediction which provides proton flux profiles and cumulative fluence profiles at 0.5 and 2 MeV of solar energetic particle events, from their onset up to the arrival of the interplanetary shock at the spacecraft position (located at 1 or 0.4 AU). Based on the proton transportation model by Lario et al. [Lario, D., Sanahuja, B., Heras, A.M. Energetic particle events: efficiency of interplanetary shocks as 50 keV E < 100 MeV proton accelerators. Astrophys. J. 509, 415–434, 1998] and the magnetohydrodynamic shock propagation model of Wu et al. [Wu, S.T., Dryer, M., Han, S.M. Non-planar MHD model for solar flare-generated disturbances in the Heliospheric equatorial plane. Sol. Phys. 84, 395–418, 1983], we have generated a database containing “synthetic” profiles of the proton fluxes and cumulative fluences of 384 solar energetic particle events. We are currently validating the applicability of this code for space weather forecasting by comparing the resulting “synthetic” flux profiles with those of several real events. 相似文献
12.
D. B. Melrose 《Space Science Reviews》1994,68(1-4):159-170
The theory of electron cyclotron maser emission and its application to solar spike bursts are reviewed. By analogy with the Earth's AKR, three sources of free energy are considered: a loss-cone anisotropy, a velocity-space hole, and a trapped distribution. The problem of how the radiation escapes through the second harmonic absorption layer is emphasized. Harmonic emission due to z mode coalescence may operate for some bursts, but the 2–5s delay between hard X-ray bursts and spike bursts suggests that some other mechanisms is required for most spike bursts. A model involving formation of a trapped distribution in low-density regions neighboring the flaring flux tube is considered. 相似文献
13.
14.
顺序函数法求解二维非稳态热传导逆问题 总被引:2,自引:0,他引:2
基于有限控制体积法对二维非稳态热传导问题的数值模拟,导出了处理二维非稳态热传导逆问题的顺序函数法,并用该方法来对一典型的圆环域边界条件反演问题进行了反演计算,结果表明,顺序函数法是求解二维非稳态热传导逆问题的有效方法,当测量噪声比较小时,顺序函数法能得出较高精度的反演结果;当测量噪声增大时,反演结果仍能较好地再现出精确解在空间和时间方向上的变化趋势,具有一定精度。 相似文献
15.
结合数值Riemann不变量和通量限制器(FluxLimiter)的概念,将基于Chakravarthy和Osher半离散差分格式的等价差分格式应用于三维复杂流场计算,应用时间相关法和全流场捕捉技术,获得了Ma=10,a=10°状态下球头绕流结果,壁面压力分布与Rusanov的计算结果相符合,在此基础上细致地刻画了在Ma=7,a=20°状态下绕流带座能飞船的复杂流场。 相似文献
16.
本文首先将粒子云侵蚀条件下的驻点表面后退分解为无粒子烧蚀部分、粒子云引起的烧蚀增量部分和粒子撞击物面引起的直接侵蚀部分。然后研究了表面能量平衡关系,给出了粒子云引起的烧蚀增量表达式。最后分三类讨论粒子与飞行器的碰撞:(1)完全弹性碰撞(不符合实际);(2)完全非弹性碰撞;(3)部分弹性碰撞。对于后两种碰撞,本文分析了动能通量模拟适用的条件。 相似文献
17.
F.B. Rizzato A.C.-L. Chian M.V. Alves R. Erichsen S.R. Lopes G.I. de Oliveira R. Pakter E.L. Rempel 《Space Science Reviews》2003,107(1-2):507-514
Langmuir waves and turbulence resulting from an electron beam-plasma instability play a fundamental role in the generation
of solar radio bursts. We report recent theoretical advances in nonlinear dynamics of Langmuir waves. First, starting from
the generalized Zakharov equations, we study the parametric excitation of solar radio bursts at the fundamental plasma frequency
driven by a pair of oppositely propagating Langmuir waves with different wave amplitudes. Next, we briefly discuss the emergence
of chaos in the Zakharov equations. We point out that chaos can lead to turbulence in the source regions of solar radio emissions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
18.
Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II
bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and
shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection
model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures
of eruptive solar flares and thus used for the prediction of heliospheric effects.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
19.
20.
空间任意形状凸面的轨道空间外热流计算方法 总被引:11,自引:1,他引:11
采用蒙特卡罗(MonteCarlo)方法,进行了平板、半球面、抛物面的地球反照角系数和地球红外角系数计算,通过与文献数据的比较,证明了由此方法所编程序的可靠性和实用性。利用这种方法,可以计算空间任意形状凸表面的轨道空间外热流。 相似文献