首页> 外文会议>Antenna Measurement Technique Association annual meeting symposium >MEASUREMENTS OF THE SIRIUS 2 TELECOMMUNICATION SATELLITE ANTENNA
【24h】

MEASUREMENTS OF THE SIRIUS 2 TELECOMMUNICATION SATELLITE ANTENNA

机译:SIRIUS 2电信卫星天线的测量

获取原文

摘要

The Sirius 2 telecommunication satellite was build in France by Aerospatiale. As a subcontractor Saab Ericsson Space (SES) developed the telecommunication antenna for direct television broadcast. The satellite was successfully launched November 13, 1997. Three antennas were manufactured by SES: a quality model (QM), a flight model (FM1) and a flight spare (FM2). Each antennas consists of a 1.4 meter in diameter shaped main reflector fed by a shaped subreflector and a dual polarized feed horn. For the test of the antennas, spherical near-field antenna test ranges located at Ericsson Microwave System (EMW)/SES in Sweden and at the Technical University of Denmark (DTU) were used. Each of the three antennas was measured twice. Between the two measurements mechanical and thermal tests were performed. The paper presents the measurements on the satellite antennas together with a discussion of the advantages of using the spherical near-field technique for this type of measurements. Compared to a far-field range the advantages are evident: At both SES and DTU a measurement distance of ten and six meters respectively were used on the indoor ranges. On a far-field range a measurement distance in the excess of 250 meters must be applied. To decrease the measurement time the near fields were only measured in a certain region on the near field sphere. The influence of this truncation will be discussed. Coordinate systems for the antennas were defined using mirror cubes. The RF measurements as well as the optical measurements on the cubes were performed without dismounting the antenna from the antenna positioner. The radiation patterns are therefore precisely defined with respect to the coordinate systems of the cubes.
机译:天狼星2通信卫星是建立在法国的宇航公司。作为分包商萨伯 - 爱立信空间(SES)开发了直接电视广播电信天线。该卫星的成功发射11月13日,1997年三根天线被SES制造:质量模型(QM),飞行模式(FM1)和飞行备用(FM2)。每个天线包括通过一个成形子反射器和双极化馈电喇叭送入直径形主反射器1.4米。对于天线的测试,使用位于爱立信微波系统(EMW)/ SES在瑞典和丹麦技术大学(DTU)球面近场天线测试范围。三个天线中的每一个测量两次。两次测量之间进行机械和热试验。本文介绍了对卫星天线与使用球面近场技术这种类型的测量的优点的讨论一起测量。相比于远场范围中的优点是明显的:在这两个SES和DTU 10的测量距离和分别在室内范围分别使用了六个米。在远场范围中的超过250米的测量距离必须应用。为了减少测量时间的近场只在一定的区域中测量的近场范围。这个截断的影响进行讨论。坐标用于天线使用镜立方体定义的系统。在不脱离天线定位器拆卸天线进行的RF测量结果,以及对所述立方体的光学测量。的辐射图案被精确因此相对于该立方体的坐标系统中定义的。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号