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POlarization Emission of Millimeter Activity at the Sun (POEMAS): New Circular Polarization Solar Telescopes at Two Millimeter Wavelength Ranges

机译:太阳毫米活动的极化发射(POEMAS):两个毫米波长范围内的新型圆偏振太阳望远镜

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摘要

We present a new system of two circular polarization solar radio telescopes, POEMAS, for observations of the Sun at 45 and 90 GHz. The novel characteristic of these instruments is the capability to measure circular right- and left-hand polarizations at these high frequencies. The two frequencies were chosen so as to bridge the gap at radio frequencies between 20 and 200 GHz of solar flare spectra. The telescopes, installed at CASLEO Observatory (Argentina), observe the full disk of the Sun with a half power beam width of 1. 4~({ring operator}), a time resolution of 10 ms at both frequencies, a sensitivity of 2 - 4 K that corresponds to 4 and 20 solar flux unit (=10~4 Jy), considering aperture efficiencies of 50±5 % and 75±8 % at 45 and 90 GHz, respectively. The telescope system saw first light in November 2011 and is satisfactorily operating daily since then. A few flares were observed and are presented here. The millimeter spectra of some flares are seen to rise toward higher frequencies, indicating the presence of a new spectral component distinct from the microwave one.
机译:我们提出了一个由两个圆偏振太阳射电望远镜POEMAS组成的新系统,用于观测45 GHz和90 GHz的太阳。这些仪器的新颖特性是能够在这些高频下测量圆形右旋和左旋极化。选择这两个频率是为了弥合太阳耀斑光谱在20至200 GHz之间的无线电频率之间的差距。安装在阿根廷CASLEO天文台的望远镜观测太阳的整个圆盘,其半功率光束宽度为1. 4〜({ring operator}),两个频率下的时间分辨率均为10 ms,灵敏度为2 -4 K对应4和20太阳通量单位(= 10〜4 Jy),分别考虑在45 GHz和90 GHz时的孔径效率为50±5%和75±8%。望远镜系统于2011年11月首次亮起,此后每天运行令人满意。观察到了一些耀斑,并在此处介绍。可以看到某些耀斑的毫米波频谱朝着更高的频率上升,这表明存在与微波不同的新频谱成分。

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