两个相邻活动区中的相应耀斑     

史忠先  栾蒂 《天文学报》1997,38(3):257-263

本文描述ＮＯＡＡ６２３３活动区中的一组双带耀斑及和与之有时间相关性的ＮＯＡＡ６２４０中的单带耀斑的磁场位形．并着重讨论由观测推断出的磁场拓扑联接性．分析表明：三个单耀斑发生在正极磁区里，与发生在δ黑子区中的双带耀斑，可能有远距离磁环相联系．这一高位磁环与δ黑子中的低位剪切磁环柑互作用，可能是能发双带耀斑的直接原因．在双带耀斑能量初始释放中被加速的电子，可能是沿着高位磁环或磁拓扑分界面（ＮＯＡＡ ６２４０与ＮＯＡＡ６２３３间）传播，并导致ＮＯＡＡ６２４０中的单带耀斑．因此这些单带耀斑都可能是双带耀斑的相应耀斑．  相似文献   

The brightness reversal of submarine sand waves in “HJ-1A/B” CCD sun glitter images     

HE Xiekai  CHEN Ninghu  ZHANG Huaguo  GUAN Weibing 《海洋学报(英文版)》2015,34(1):94-99

The brightness reversal of submarine sand waves appearing in the small satellite constellation for environment and disaster monitoring and forecasting("HJ-1A/B") CCD sun glitter images can affect the observation and depth inversion of sand wave topography. The simulations of the normalized sun glitter radiance on the submarine sand waves confirm that the reversal would happen at a specific sensor viewing angle, defined as the critical angle. The difference between the calculated critical angle position and the reversal position in the image is about 1, which is excellent in agreement. Both the simulation and actual image show that sand wave crests would be indistinct at the reversal position, which may cause problems when using these sun glitter images to analyze spatial characteristics and migration of sand waves. When using the sun glitter image to obtain the depth inversion, one should take the advantage of image properties of sand waves and choose the location in between the reversal position and the brightest position. It is also necessary to pay attention to the brightness reversal when using "HJ-1A/B" CCD images to analyze other oceanic features, such as internal waves, oil slicks, eddies, and ship wakes.  相似文献   

释光技术在水成沉积物测年中的应用进展   总被引：1，自引：0，他引：1  

赵秋月  魏明建  周锐  宋波  潘宝林  陈淑贞  赵晓红 《地质论评》2014,60(1):31-38

准确获得水成沉积物的年龄是第四纪年代学重要的前沿问题之一。随着释光技术的发展,水成沉积物释光测年在如下方面有新的进展：具体释光技术的选择、释光测量方法、测年矿物的种类、矿物的粒级和获得等效剂量的统计方法等。线性调整光释光技术能够提取光释光信号中衰退快的组分;单片再生法应用广泛;单颗粒技术在挑选沉积时晒退充分的颗粒方面具有一定的优势;水成沉积物中的石英比长石更易晒退;较多的实验表明水成沉积物中的粗颗粒比细颗粒更易晒退;获得等效剂量的统计模型很多,但尚无一种统计模型适用于所有样品。在此基础上探讨了水成沉积物释光测年在气候、构造运动、冰川进退历史和人类活动主导的土壤侵蚀量变化研究中的意义及今后的研究方向,为全面了解该领域的最新研究进展提供参考。  相似文献   

Symbolic analytical solution of N‐dimensional radially symmetric polytropes     

A. S. Saad 《Astronomische Nachrichten》2004,325(9):733-739

In this paper, accelerated power series solutions are developed for N‐dimensional symmetric radially polytropes. The solutions are valid for any geometric and polytropic index. The implementation of Padé technique and changing of the independent variable give us identical polytrope solutions to the numerical one. Physical parameters are presented for Ndimensional radially polytropes. In case of the isothermal sphere, the density profile is accurate to 10^–5 per cent whatever the value of ξ is. All the computations are performed using Mathematica software. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

太阳光度计反演大气水汽总量的方法与结果对比分析   总被引：2，自引：0，他引：2  

周宁  刘敏 《遥感学报》2011,15(3):568-577

详述了使用太阳光度计反演大气水汽柱总量的反演方法—单通道法和双通道法,其中双通道法又可采用不同 的非水汽通道来实现。考虑到气溶胶光学厚度及瑞利散射的影响,分析了不同方法反演所得水汽总量相对探空数据的 误差。结果表明,这些方法的反演结果非常接近。在实际应用中,可使用任一种方法来反演水汽。  相似文献   

北方盛夏台风暴雨的天气型及其年际变率   总被引：18，自引：5，他引：18       下载免费PDF全文

仇永炎 《气象》1997,23(7):3-9

１９４９－１９９６年的４８个盛夏期间，我国北方地区共有１０次过程雨量最大值大于４００ｍｍ的台风暴雨实例。从台风与西风槽相互作用的观点对这１０例进行分类。根据实践经验可以把台风槽、可套西风槽、日本海渤海高压、上海地区８５０ｈＰａ东南风急流以及弱冷空气入侵台风等５因子作为分型的判据。结果指出，１０例中只有发生于１９５０、１９６３、１９７５、１９８４和１９９６年８月上旬的５例属于相互作用型，其他５例不是  相似文献   

Long‐term evolution of the magnetic field generated by an ensemble of Rossby vortices     

E. Tikhomolov  V. Mordvinov 《Astronomische Nachrichten》2001,322(3):189-195

The evolution of the large‐scale component of the magnetic field generated by an ensemble of Rossby vortices is numerically simulated. The distribution of the Rossby vortices excited at the beginning of each Carrington rotation is determined from the analysis of Kitt Peak synoptic maps. Our model also considers 11‐year hydrodynamic and 22‐year magnetic field oscillations. In the vicinity of the Rossby vortices, the toroidal magnetic field is significantly amplified and the sign of the angle between the rope of the field lines and the equator is in accordance with observations for “normal” sunspots. We also suggest the possibility of the interpretation by our model of “abnormal” sunspot phenomena. We find that an inverse cascade, namely, the merging of Rossby vortices, gives rise to the formation of large‐scale hydrodynamic structures with a life‐time on the order of a solar cycle period. We conclude from this that the formation of such structures can thus explain the appearance of long‐lived, large‐scale component in the distribution of the magnetic field.  相似文献