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Lower atmospheric characteristics and Ionospheric backscatter observed using Calcutta University ST Radar (CU-STR)

机译:使用加尔各答大学的ST雷达(CU-STR)观测到较低的大气特征和电离层反向散射

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Summary form only given. A new Stratosphere-Troposphere Radar has been installed at Ionosphere Field Station (IFS) (22.93°N, 88.50°E geomagnetic dip: 34°N) of University of Calcutta (CU) located about 50km north-east of the city. The main objectives of this radar are to carry out studies on tropopause convection, gravity waves, equatorial/planetary waves and ionospheric E and F region irregularities. This Radar comprises of fully active phased array having 475 Yagi antennas operating at 53 MHz, each transmitting peak power of 2kw. The location of this radar is unique being located in the transition region from the tropics to the sub-tropics and around the northern crest of Equatorial Ionization Anomaly (EIA) in the geophysically sensitive Indian longitude sector. In fact, to the best of our knowledge, no such radars are presently operational in the entire eastern and north eastern part of the country and also in the south-east Asian longitude sector. The main radar is configured into 25 sub-arrays each having 19 transmitter receiver modules. A pilot version of the main radar is operational at IFS since April 2018. The location offers an interesting platform for studying the dynamics of the lower atmosphere with distinctive wind velocities, Doppler width and SNR measured during Premonsoon and Monsoon period, often varying at different times of the day and also from one day to the next. This radar operated at a maximum duty ratio of 5% is capable of measuring various atmospheric parameters mentioned above with height resolution of 50 meters could provide vital information for convective activity and cyclone forecast. The present paper reports the three components wind velocities and other related parameters for some representative days of pre-monsoon and post-monsoon periods of 2018. Ionospheric E-region backscattered signals are usually observed during the local summer months of May to July. Some initial RTI maps have been generated using this facility which shows operated in ionospheric mode during post sun-set hours. It shows appreciable lower height of E-region echoes often around 110km during 23:00-02:00 IST.
机译:仅提供摘要表格。在距城市东北约50公里的加尔各答大学(CU)的电离层现场站(IFS)(北纬22.93°,北纬88.50°E地磁倾角:34°N)处安装了新的平流层-对流层雷达。该雷达的主要目的是对对流层顶对流,重力波,赤道/行星波以及电离层E和F区域的不规则性进行研究。该雷达由全有源相控阵组成,该相控阵具有475个八木天线,工作频率为53 MHz,每个天线发射2kw的峰值功率。该雷达的位置是唯一的,位于从热带到亚热带的过渡地区,以及对地球物理敏感的印度经度区中的赤道电离异常(EIA)的北顶。实际上,据我们所知,目前在该国的整个东部和东北部以及东南亚经度部门都没有这种雷达在运行。主雷达配置为25个子阵列,每个子阵列具有19个发射器-接收器模块。自2018年4月起,主雷达的试验版已在IFS投入运行。该地点提供了一个有趣的平台,用于研究低层大气的动态,具有独特的风速,多普勒宽度和SNR,在季风和季风期间测量,通常在不同时间变化以及一天到第二天的时间。该雷达的最大占空比为5%,能够测量上述各种大气参数,高度分辨率为50米,可以为对流活动和气旋预报提供重要信息。本文报告了2018年季风前后季风中某些代表性日的三个分量风速及其他相关参数。通常在5月至7月的夏季夏季,观测到电离层E区反向散射信号。使用此工具已生成了一些初始RTI图,该图显示了太阳下山后在电离层模式下运行的情况。它显示了IST在23:00-02:00期间E区域回波的明显较低高度通常在110 km左右。

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