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Brazilian Solar Spectroscope (bss)

机译:巴西太阳光谱仪(BSS)

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Digital, decimetric (200–2500 MHz) Brazilian Solar Spectroscope (BSS) with high time (10–1000 ms) and frequency (1–10 MHz) resolution is in regular operation since April, 1998, at National Space Research Institute (INPE) at São José dos Campos, Brazil. BSS operates in conjunction with a 9-m diameter polar mounted antenna. It allows to select suitable observing frequency range, frequency and time resolutions and data can be digitized up to 100 channels. BSS has capabilities of quasi-real time display of the ongoing dynamic spectra of the solar activity that enables the observer to modify observational parameters so as to suit a specific type of activity such as spikes and improve the quality of data acquisition and storage. Minimum detectable flux density of the spectroscope, for different combinations of the observational parameters, is ∼3 s.f.u. Observations are carried out routinely from 11 UT to 19 UT. Necessary software for data acquisition and reductions has been developed in IDL 5.3 environment. Data are available in FITS and ASCII formats. Absolute timing accuracy of the station is less than 3 ms. Here, we present examples of the bursts which have been recorded by BSS and available display facilities.
机译:自1998年4月以来,具有高分辨率(10–1000 ms)和频率(1–10 MHz)分辨率的数字分米(200–2500 MHz)巴西太阳光谱仪(BSS)在美国国家太空研究所(INPE)投入正常运行在巴西圣何塞·多斯·坎波斯。 BSS与直径为9 m的极地安装天线配合使用。它允许选择合适的观测频率范围,频率和时间分辨率,并且数据可以数字化多达100个通道。 BSS具有实时实时显示太阳活动动态光谱的功能,使观察者能够修改观测参数,以适应特定类型的活动,例如峰值,并提高数据采集和存储的质量。对于不同的观测参数组合,分光镜的最小可检测通量密度约为3s.f.u。观察是从11 UT到19 UT常规进行的。在IDL 5.3环境中已经开发了用于数据获取和缩减的必要软件。数据以FITS和ASCII格式提供。站的绝对定时精度小于3 ms。在这里,我们介绍由BSS和可用的显示设备记录的突发示例。

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