Measurement of linear polarization in the Hα line in solar flares

Large solar telescopes built at places with a quite excellent seeing, equipped with a sophisticated optics and control system are too expensive and unique to be used currently in hunting of sudden and short‐lasting activity events, e.g. flares and eruptive prominences. For a systematic observation of selected kinds of active phenomena it is still necessary to use smaller or medium‐sized telescopes equipped with a special setup of devices. Detection of linear polarization in the Hα line emitted in a flare seems to be just a right task and delicate matter for such a systematic observation. This kind of polarization is supposed to be generated by particle beams accelerated in thke corona and directed towards denser chromospheric layers where the particle beams deposit their kinetic energy. As the accelerated particle beams possess a preferred direction of velocity they can produce a linearly polarized light. However, the occurrence of the accelerated particle beams and the related linear polarization in the Hα line may have a tendency to appear: 1) at the early beginning of a flare 2) in pulses lasting just a few seconds or even less. To measure the linear polarization in flares regularly we have built an additional branch in the Ondřejov multichannel flare spectrograph. In this paper we describe the optical system, the detectors, the method used for data recording and reduction and we also briefly discuss the first results.     

Study on multiple induced polarization parameters in groundwater exploration in Bashang poverty alleviation area of Heibei Province,China

The study examines a water exploration and poverty alleviation project in Guyuan county. The study analyzes correlations between aquifers and multiple induced polarization (IP) parameters, including resistivity, polarizability, deviation, half decay time, water-bearing factors, and Kc, a new parameter refined in this study. Based on the study, the well was placed accurately, and its maximum water inflow reached 30 m³/h. Kc value highlights the rate of change at early stages of IP secondary field. Kc value served as a quick indicator in this groundwater prospecting and is validated in practice. Progress has been made in finding new parameters in exploring water with IP method. Thanks to the project, local people have access to water and poverty alleviation has scored some achievements.     

TRES-Ⅰ型多分量瑞利波勘探仪的研究及应用

提出多分量瑞利波勘探的技术思想和方法,研制成功专用的防爆型多分量瑞利波勘探仪器,建立了在用极化分析对瑞利波勘探记录的多分量信号分析的基础上,用极化滤波提取有效瑞利波信号的方法。在煤矿井下及地面实际应用表明,多分量瑞利波勘探与单分量法比较,信号的信噪比、勘探深度和可靠性均有一定的提高。     

激发极化法在早前寒武纪变质岩系找水中的应用

通过对在早前寒武纪变质岩系进行抗旱找水中利用地球物理勘探定井的实例分析,阐述了利用激发极化法在早前寒武纪变质岩分布区辨认含水层,确定含水层埋深,最终确定较好井位的方法。该方法对解决早前寒武纪变质岩系的干旱缺水现状有广泛深远的意义。     

储层岩石流动电位的电化学影响因素

利用储层岩石的流动电位特性描述油藏的流动特性已引起地球物理领域的关注。依据多孔介质中的双电层模型与毛管电化学理论,建立了渗流场、离子流场和电流场的耦合关系,数值模拟了泥质砂岩储渗特性和电化学因素对流动电位耦合系数的影响。结果表明:当考虑储层岩石中存在浓差极化效应时,流动电位耦合系数的绝对值随溶液浓度、阳离子交换量、孔隙度和渗透率的增大而增大;浓差极化效应对流动电位具有放大作用。     

一次东北冷涡天气过程双偏振雷达降水粒子相态识别

本文利用双偏振天气雷达资料,对2019年6月7-9日辽宁地区一次东北冷涡强对流天气过程进行分析。分析了东北冷涡的演变过程以及双偏振雷达的偏振参量在降水粒子相态识别中的作用,研究了不同判别规则对模糊逻辑算法识别结果的影响。结果表明：双偏振雷达的偏振参量可以对水凝物的种类、空间分布、物理形态进行大致判断,但水凝物相态识别结果仍需细化。模糊逻辑算法在强回波区域的识别结果更准确,采用不同的判别规则得到的水凝物分类结果虽存在一定差异,但在大部分观测区域的分类结果基本一致,符合天气演变规律,能够为气象预报预警提供鉴别参考。具有广泛时间、空间适配性的模糊逻辑算法,仍需大量实测案例数据的验证与仿真。     

海盐粒子沉积下碳钢的大气腐蚀初期行为

利用体视显微镜和电化学极化技术原位考察了碳钢上NaCl盐粒的吸潮及其液滴的扩展行为。实验结果表明,NaCl液滴的吸潮水解过程主要受环境相对湿度的影响。相对湿度越高,水解越容易。在极化状态下,NaCl液滴的扩展随极化电流的增加而线性加速。NaCl液滴的扩展与碳钢大气腐蚀的电化学过程相互影响。一方面,NaCl液滴扩展的动力来自于大气腐蚀过程所形成的腐蚀电流,另一方面,NaCl液滴的扩展加大了大气腐蚀过程的阴极面积。进而加速了碳钢的腐蚀过程。     

双线偏振双波段（X／Ka）主被动微波遥感系统的研制与初步试验

为拓展主波，动生波探测系统遥感降水云雨的功能，使系统的原理先进性能有进一步的体现，将一套主被动双波段（X／Ka)微波遥感系统研制升级为双线偏振双波段主被动微波遥感系统。对新系统及主要部件的工作原理，技术指标及研制改造方法作了介绍，还给出了一些初步的观测结果。     

GNSS-R/IR监测地表冻融状态对延迟多普勒波形和多路径数据影响分析

将GNSS-R/IR技术的应用领域拓展到地表冻融状态的监测中,本文利用冻融土混合介质介电常数模型计算土壤介电常数,采用双站全极化相干反射率模型和随机粗糙面散射模型,分别计算了经冻融土反射的GPS相干反射量的镜像反射率,以及GPS非相干反射分量的漫散射特性。模拟分析了冻融转换时,GPS多路径信息(GNSS-IR)以及包含漫散射信号的延迟多普勒图(GNSS-R)的变化特征。理论研究表明冻融转换过程中,地表介电常数的变化导致GPS多路径信息和延迟多普勒图的明显变化。本文从散射机理上揭示了利用GNSS-R和GNSS-IR遥感进行地表冻融特性监测的理论依据。