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11.
Mohamed Nedal M. Youssef Ayman Mahrous Rabab Helal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1824-1836
We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (~62%), while the partial HCMEs comprised ~35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts. 相似文献
12.
利用1992年10月27日耀斑极为完整的高质量观测资料,通过对可见光、软X射线和硬X射线图像和光谱的综合分析,诊断耀斑过程中的热与非热性质,结果表明,在这个事件中,热与非热过程并存且在时空演化上呈现不同的特征 相似文献
13.
太阳活动与空间坏境紧密相关,大耀斑会引起空间环境的剧烈扰动.太阳活动预报便成空间环境预报的基本依据.太阳预报水平长期以来提高缓慢,太阳物理学家皆有共识,寄希望于物理预报的进展,但举步维艰.近来,“太阳活动的行星潮汐效应”的研究取得了新进展1)[1,2],引潮力可以触发耀斑,从而,利用这类效应发展物理预报技术,呈现良好前景.“太阳耀斑发生率按行星引潮力的分布”已有几个具体结果,表面看来,其间似乎有出人需予澄清.1972年,董土仑和林柏森发现1958-1968年94个质子耀斑的发生率在其目面经度处(活动经度上)技引潮力… 相似文献
14.
本文分析了太阳射电短厘米、毫米波段准周期脉动现象(精细结构)的频率特性,得知该现象是由非热电子准周期注入的回旋同步辐射所致. 相似文献
15.
太阳活动对VLF传播的一种影响 总被引:1,自引:0,他引:1
本文以实验数据为基础, 讨论了在太阳耀斑期间产生的相位周期丢失, 并用对极传播理论解释了这种相位周期丢失的机理。相位周期丢失是电波传播中的一个重要传播现象, 特别是对于低频和甚低频传播。由于太阳耀斑引起的这一传播现象在以往的讨论中比较罕见, 因此, 对这一问题的讨论具有特殊意义。 相似文献
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17.
Input data of the system are two-dimensional images and one-dimensional distributions of total and polarized solar emission at 5.2 cm wavelength obtained with SSRT. Together with photoheliograms, magnetograms, Hα-filtergrams and characteristics of active regions received from other sources, they form the initial database. The first stage includes superimposing the images, identifying microwave sources with active regions, assigning NOAA numbers to the sources, and determining for each active region the heliolatitude, extent, and inclination angle of the group's axis to the equator. These data are used to calculate the boundaries of longitude zones for each active region. A next stage involves determining the brightness temperatures of microwave sources less than the polarization distribution, the degree of polarization, and microwave emission flux, as well as calculating the parameters of microwave sources. Each parameter is assigned its own value of the weight factor, and the sum of values is used to draw the conclusion about the flare occurrence probability in each active region and on the Sun in general. 相似文献
18.
燃料电池因其高效、无污染、噪声小等特点,被认为是未来最具有潜力的无人机(UAV)用动力源,燃料电池阴极供气系统的控制技术是决定燃料电池系统性能和可靠性的关键。针对无人机用质子交换膜燃料电池(PEMFC)阴极供气系统,首先,考虑外界温度、压力、空气密度以及雷诺数等随高度变化的参数,建立了跨高度离心空压机模型并分析了其在不同高度下的工作特性,基于无刷直流电机反电势特征构建了高速空压机驱动电机模型。其次,通过计算燃料电池阴极氧气和氮气的动态分压获取了PEMFC电堆输出电压。设计了基于分数阶PIλDμ的过氧比和阴极气压控制方法,驱动电机采用有限集模型预测控制(MPC)实现快速的转矩响应,仿真结果表明设计的控制器可在无人机跨高度运行条件下实现过氧比的快速调节,同时维持阴极气压稳定,满足燃料电池阴极供气需求。 相似文献
19.
O.V. Dudnik M.L. Kaiser 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The analysis of observations of very high frequency radio noise intensity at the middle latitude on a frequency f = 500 MHz from 14th till 26th of October, 2003 is presented. These data are compared with the solar radio bursts in the range of frequencies 1–14 MHz registered by RAD2 receiver of the WAVES device installed on board the WIND spacecraft. 相似文献
20.