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831.
R. Modzelewska M.V. Alania 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We show that the higher range of the heliolongitudinal asymmetry of the solar wind speed in the positive polarity period (A > 0) than in the negative polarity period (A < 0) is one of the important reasons of the larger amplitudes of the 27-day variation of the galactic cosmic ray (GCR) intensity in the period of 1995–1997 (A > 0) than in 1985–1987 (A < 0). Subsequently, different ranges of the heliolongitudinal asymmetry of the solar wind speed jointly with equally important corresponding drift effect are general causes of the polarity dependence of the amplitudes of the 27-day variation of the GCR intensity. At the same time, we show that the polarity dependence is feeble for the last unusual minimum epoch of solar activity 2007–2009 (A < 0); the amplitude of the 27-day variation of the GCR intensity shows only a tendency of the polarity dependence. We present a three dimensional (3-D) model of the 27-day variation of GCR based on the Parker’s transport equation. In the 3-D model is implemented a longitudinal variation of the solar wind speed reproducing in situ measurements and corresponding divergence-free interplanetary magnetic field (IMF) derived from the Maxwell’s equations. We show that results of the proposed 3-D modeling of the 27-day variation of GCR intensity for different polarities of the solar magnetic cycle are in good agreement with the neutron monitors experimental data. To reach a compatibility of the theoretical modeling with observations for the last minimum epoch of solar activity 2007–2009 (A < 0) a parallel diffusion coefficient was increased by ∼40%. 相似文献
832.
M.B. Krainev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The different types of the data recorded in the experiment of the regular balloon monitoring of cosmic rays (carried out since 1957 by Lebedev Physical Institute, Moscow, Russia, in several locations) are described. So called detailed information (the form of each pulse detected by the ground-based receiver) recorded during the last 12 years is discussed in more details. The use of these data both for getting and correcting the standard results of the experiment and for obtaining some additional information on the cosmic rays in the Earth’s atmosphere is considered. 相似文献
833.
A. Dosch A. Shalchi B. Weinhorst 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(11):2287
In the past few year several theories have been presented for describing cosmic ray scattering across the mean magnetic field. It is the purpose of the present article to discuss the relation between these different theories in order to improve our understanding of cosmic ray perpendicular scattering and to explore the parameter regimes for which these different theories are valid. 相似文献
834.
835.
杜爽 《郑州航空工业管理学院学报(管理科学版)》2008,26(1):106-109
乡村债务包括存量债务和增量债务两个部分,解决乡村债务问题就要从这两个方面入手。对于存量债务,可以通过债务重组的方式进行化解;对于增量债务文章提出了在新农村建设中,不仅不应一味地避免乡村新增债务,而且应该积极地采取有效措施,使乡村新增债务尤其是良性债务维持在适度的规模和水平之上的观点。 相似文献
836.
837.
R.P. Kane 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The early history of solar wind was replete with prejudices and strong opposition to Parker’s formulation. It was only after conclusive evidence from satellite data was obtained that the idea of solar wind was accepted. Some personal experiences of mine during my stay at the University of Chicago in 1953–1954, including the encounter of Dr. Simpson with Dr. Biermann and the inconclusive discussion between them about a possible perpetual solar outflow of particles are presented and further developments when Parker came to Chicago in 1956 and formulated his idea of solar wind, as narrated to me later by Dr. Simpson, are described. 相似文献
838.
Ingrid Mann 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):160-167
The average mass of dust per volume in space equals that of the solar wind so that the interplanetary medium should provide an obvious region to study dust plasma interactions. While dust collective behavior is typically not observed in the interplanetary medium, the dust component rather consists of isolated grains screened by and interacting with the plasma. Space measurements have revealed several phenomena possibly resulting from dust plasma interactions, but most of the dust plasma interactions are at present not quantified. Examples are the production of neutrals and pick-up ions from the dust, dust impact generated field variations at spacecraft and magnetic field variations possibly caused by solar wind interacting with dust trails. Since dust particles carry a surface charge, they are exposed to the Lorentz force in the interplanetary magnetic field and for grains of sub-micrometer sizes acceleration can be substantial. 相似文献
839.
本文从力学指导思想的认识与落实教学改革,师资队伍建设3个方面结合本院实际进行浅议。 相似文献
840.
针对GNSS-R进行海面风速反演过程中时频域相关物理量较多,数据耦合性强等问题,提出了基于反向传播(BP)神经网络反演海面风速的方法。建立反演过程中相关观测量与风速的对应关系,选取多观测量作为输入,对输入数据进行处理,设置神经元与激励函数,使用BP神经网络自适应调整拟合参数,将风速作为神经网络输出端的特征量提取。反演结果,风速≤ 20 m/s时,反演均方根误差RMSE=1.21 m/s,风速>20 m/s时反演均方根误差RMSE=2.54 m/s,反演结果优于使用时延相关曲线前沿斜率(LES)和时延多普勒相关功率均值(DDMA)方法得到的反演结果,且迭代次数较少,复杂度较低,证明该方法可以应用于GNSS-R海面风速反演。 相似文献