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Indian Payloads (RT-2 Experiment) Onboard CORONAS-PHOTON Mission

机译:印度有效载荷(RT-2实验)板载CORONas-pHOTON任务

摘要

RT-2 Experiment (RT - Roentgen Telescope) is a low energy gamma-rayinstrument which is designed and developed as a part of Indo-Russiancollaborative project of CORONAS-PHOTON Mission to study the Solar flares inwide energy band of electromagnetic spectrum ranging from UV to high-energygamma-rays (~2000 MeV). RT-2 instruments will cover the energy range of 15 keV to 150 keV extendableup to ~1 MeV. It consists of three detectors (two Phoswich detectors, namely,RT-2/S, RT-2/G and one solid-state imaging detector RT-2/CZT) and oneprocessing electronic device (RT-2/E). Both Phoswich detectors will have timeresolved spectrum, whereas the solid-state imaging detector will have highresolved image of the solar flares in hard X-rays. We have used Co-57 (122 keV)radio-active source for onboard calibration of all three detectors. In thispaper, we briefly discuss the in-flight performance of RT-2 instruments andpresent initial flight data from the instruments. This mission was launched into polar LEO (Low Earth Orbit) (~550 km) on 30thJanuary 2009 from Plesetsk Cosmodrome, Russia.
机译:RT-2实验(RT-伦琴望远镜)是一种低能伽马射线仪器,它是CORONAS-PHOTON任务的印俄合作项目的一部分,设计和开发了该项目,用于研究从UV到UV的电磁光谱宽能带中的太阳耀斑高能伽玛射线(〜2000 MeV)。 RT-2仪器将涵盖15 keV至150 keV的能量范围,可扩展至约1 MeV。它由三个检测器(两个Phoswich检测器,即RT-2 / S,RT-2 / G和一个固态成像检测器RT-2 / CZT)和一个处理电子设备(RT-2 / E)组成。这两个Phoswich检测器将具有时间分辨光谱,而固态成像检测器将在硬X射线中具有太阳耀斑的高分辨率图像。我们已经使用Co-57(122 keV)放射源对所有三个探测器进行了机载校准。在本文中,我们简要讨论了RT-2仪器的飞行性能,并介绍了这些仪器的初始飞行数据。这项任务于2009年1月30日从俄罗斯普列塞茨克国际天文望远镜发射到极地LEO(低地球轨道)(约550公里)。

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