Sources of SEP Acceleration during a Flare – CME Event     

N. J. Lehtinen  S. Pohjolainen  K. Huttunen-Heikinmaa  R. Vainio  E. Valtonen  A. E. Hillaris 《Solar physics》2008,247(1):151-169

A high-speed, halo-type coronal mass ejection (CME), associated with a GOES M4.6 soft X-ray flare in NOAA AR 0180 at S12W29 and an EIT wave and dimming, occurred on 9 November 2002. A complex radio event was observed during the same period. It included narrow-band fluctuations and frequency-drifting features in the metric wavelength range, type III burst groups at metric – hectometric wavelengths, and an interplanetary type II radio burst, which was visible in the dynamic radio spectrum below 14 MHz. To study the association of the recorded solar energetic particle (SEP) populations with the propagating CME and flaring, we perform a multi-wavelength analysis using radio spectral and imaging observations combined with white-light, EUV, hard X-ray, and magnetogram data. Velocity dispersion analysis of the particle distributions (SOHO and Wind in situ observations) provides estimates for the release times of electrons and protons. Our analysis indicates that proton acceleration was delayed compared to the electrons. The dynamics of the interplanetary type II burst identify the burst source as a bow shock created by the fast CME. The type III burst groups, with start times close to the estimated electron-release times, trace electron beams travelling along open field lines into the interplanetary space. The type III bursts seem to encounter a steep density gradient as they overtake the type II shock front, resulting in an abrupt change in the frequency drift rate of the type III burst emission. Our study presents evidence in support of a scenario in which electrons are accelerated low in the corona behind the CME shock front, while protons are accelerated later, possibly at the CME bow shock high in the corona.  相似文献   

Possible Contribution of Mature γ-ray Pulsars to Cosmic-ray Positrons     

Quan-Gui Gao Ze-Jun Jiang Li Zhang 《天体物理学报》2008,8(1):87-95

We restudy the possible contribution of mature gamma-ray pulsars to cosmic ray positrons based on the new version of outer gap model. In this model, the inclination angle and average properties of the outer gap are taken into account, and more mature pulsars can have the outer gap and emit high energy photons. Half of the primary particles in the outer gaps will flow back toward the star surface and emit synchrotron photons, which can produce electron/positron pairs by the cascade of pair production. Some of these pairs will escape from the light cylinder and be accelerated to relativistic energies in the pulsar wind driven by low-frequency electromagnetic waves. Using a Monte Carlo method, we obtain a sample of mature gamma-ray pulsars and then calculate the production of the positrons from these pulsars. The observed excess of cosmic positrons can be well explained by this model.  相似文献   

地下工程涌水涌砂诱发的沉降试验研究     

刘成禹  张翔  程凯  陈博文 《岩土力学》2019,40(3):843-851

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Study on wetting deformation characteristics of coarse granular materials and its simulation in core-wall rockfill dams     

Xiongxiong Zhou  Shichun Chi  Maohua Wang  Yufeng Jia 《国际地质力学数值与分析法杂志》2020,44(6):851-873

The wetting deformation of coarse granular materials is often considered to be an important cause of the core wall rockfill dam cracks during impounding. By analyzing existing research results, this paper proposes a hyperbolic relationship between the wetting axial strain and wetting stress level and puts forwards a warped surface relationship among spherical stress, shear stress, and the ratio of wetting volumetric strain to wetting axial strain. To illustrate its practicability, the wetting strain model's parameter determination process is introduced and the rockfill materials wetting parameters are determined using the triaxial wetting test data. Moreover, the collapse settlement of Guanyinyan rockfill dam during first impounding is numerically simulated using the proposed method to calculate rockfill wetting deformation and verified by field measurements and monitoring data. The results show that the calculative method of wetting deformation proposed in this paper is reasonable and practical; the wetting deformation of upstream rockfill materials would cause an adverse deformation trend, which may lead to crack occurrence at the upstream slope and dam crest; and the Guanyinyan rockfill dam cracks on the top of junction mainly caused by the wetting deformation of upstream rockfill.  相似文献   

基于粒子滤波的行车轨迹路网匹配方法     

郑诗晨  盛业华  吕海洋 《地球信息科学学报》2020,22(11):2109-2117

行车轨迹是一种时间序列的地理空间位置采样数据,而传统的轨迹—路网匹配方法主要以全局或局部寻优的方式建立轨迹—路网匹配关系,影响了时空场景中数据的匹配计算过程的相对独立性。针对这个问题,本文基于粒子滤波（Particle Filter,PF）原理建立行车轨迹与道路网络之间的匹配关系。首先,沿轨迹中车辆运动方向在道路网络中搜索邻近道路节点,在与道路节点拓扑邻接的道路弧段上初始化随机生成粒子,根据轨迹中车辆运动模型将粒子沿所在道路弧段移动;然后,基于PF原理计算各时刻粒子运动状态及与行车轨迹采样点之间的距离误差,根据高斯概率密度函数计算粒子权重并利用随机重采样方法进行粒子重采样,迭代更新粒子运动状态;最后,计算与搜索到的道路节点拓扑邻接的每条道路弧段中累计粒子权重,通过各道路弧段累计权重计算轨迹—路网匹配关系。以行车轨迹进行实验表明,利用本文方法可以通过粒子时空变化反映采样点的移动,行车轨迹—路网匹配结果的正确率大于85%,能够实现行车轨迹和路网的准确匹配。  相似文献   

黄河中游多沙粗沙区水沙变化趋势及其主控因素的贡献率   总被引：5，自引：0，他引：5  

孙倩  于坤霞  李占斌  李鹏  张晓明  龚珺夫 《地理学报》2018,73(5):945-956

随着气候变化和人类活动影响加剧,黄河中游多沙粗沙区的水沙变化剧烈,因此研究影响黄河中游多沙粗沙区径流量和输沙量的驱动因素对预测未来水沙变化具有重要意义。本文选取Mann-Kendall趋势检验法,Pettitt突变点检验法,位置、尺度、形状的广义可加模型以及累积量斜率变化率比较法对黄河中游多沙粗沙区15个水文站控制流域1956-2010年的年降水量、年径流量以及年输沙量变化特征及其贡献率进行分析,确定影响黄河中游多沙粗沙区径流量和输沙量变化的主要原因。结果表明：① Mann-Kendall趋势检验在5%的显著性水平下,表明降水量虽呈减少趋势但并不显著,径流量和输沙量则有显著的减少趋势;② Pettitt突变点检验得出所研究区域径流量和输沙量的突变年份在1972年、1985年以及1996年左右;③ GAMLSS模型分析结果同样表明降水的均值不随时间发生变化,但降水的方差有减小的趋势;④ 通过累积量斜率变化率比较法得出,人类活动对窟野河流域径流输沙的影响大于无定河流域。通过分析黄河中游多沙粗沙区径流量和输沙量变化的原因,可为黄河中游多沙粗沙区水资源合理分配提供一定的理论支持。  相似文献   

On particle energization in accretion flows     

Eric G. Blackman 《Monthly notices of the Royal Astronomical Society》1999,302(4):723-730

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黄土高原多沙粗沙区侵蚀模型探讨   总被引：23，自引：4，他引：19  

李钜章  景可  李凤新 《地理科学进展》1999,18(1):46-53

国内外曾研究出不同类型的坡面侵蚀计算模型,但还没有一个成熟的流域侵蚀计算模型,至今流域侵蚀量仍以输沙量替代。本文充分利用黄河中游不同区域具有大量淤地坝的条件,再通过侵蚀影响因素机理的分析、在侵蚀形态类型区的划分等基础上探讨侵蚀变权模型的建设。首先选择了155个“闷葫芦”淤地坝,采集每个坝的年均淤积量,以及相应流域的侵蚀影响因素：植被盖度、降雨量、沟谷密度、切割深度、地表组成物质、>15°的坡耕地面积比等资料,采用变权形式,建立侵蚀强度宏观估算模型。最后用年降水量与年输沙量的关系对模型进行改进。  相似文献   

不同栽杉代数土壤抗蚀性的变化   总被引：7，自引：2，他引：5  

杨玉盛  陈光水  彭加才  邱仁辉 《山地学报》1999,17(2):163-167

采用标准地定位研究方法对杂木林及１代,２代,３代和４代杉木人工林土壤颗粒,土壤团聚体组成进行比较分析,结果表明：杂木要受人为干扰少,土壤颗粒及土壤团聚体组成较好,抗蚀性最好;但１代,２代,３代和４代分别是在杂木林及前１代林的采伐迹地上经再度干扰建立起来的,土壤结构破坏率加大,土壤团聚体稳定性减小,因而随着杉木林取代杂木林及杉木连栽代数增加,土壤抗蚀性减弱。  相似文献   

海水中碳酸根与固体粒子的相互作用     

王江涛  张正斌 《海洋湖沼通报》1998,(2):12-16

本文研究了海水中碳酸根在固体粒子上的吸附。碳酸根在各种因素颗粒物上的吸附程度上大小顺序为：赤铁矿〉δ－ＭｎＯ２〉水锰矿〉ＳｉＯ２,最大吸附量可达到约２ｍｇＣ／ｇ吸附剂,且最大吸附值均在天然海水ｐＨ（ｐＨ８）左右。在低ＰＨ时,碳酸根对ＮａＣｌ介质中砷酸根的吸附没有影响,在高ｐＨ时,则降低了砷酸根在固体颗粒物上的吸附量,因此碳酸根的存在对其他阴离子的吸附会产生竞争作用。  相似文献