论文标题
通过Toyokawa和Nobeyama Radio Polarimeters获得的超过七十年的太阳微波数据
Over seven decades of solar microwave data obtained with Toyokawa and Nobeyama Radio Polarimeters
论文作者
论文摘要
监测太阳微波通量及其两极分化的观察结果始于1950年代在Toyokawa和Mitaka。目前（2022年4月），日本国家天文天文台（NAOJ）的Nobeyama校园的Nobeyama无线电极化器（NORP）继续进行监测观察。在本文中，我们介绍了在NORP现在进行的太阳微波监测观察结果的简短历史。然后，我们审查在Toyokawa和Nobeyama及其元数据中获得的太阳微波炉。该数据集由NAOJ天文学数据中心操作的太阳能数据存档系统（SDA）通过HTTP（https://solar.nro.no.nao.ac.jp/norp/）和ftp（ftp:/solar-polar-polar-pub..aac.ac.jp/nsro/nsro/nsro/nsro/norp/）通过HTTP（https://solar.nro.no.ac.jp/norp/）公开提供。
Monitoring observations of solar microwave fluxes and their polarization began in Japan during the 1950s at Toyokawa and Mitaka. At present (April 2022), monitoring observations continue with the Nobeyama Radio Polarimeters (NoRP) at the Nobeyama campus of the National Astronomical Observatory of Japan (NAOJ). In this paper, we present a brief history of the solar microwave monitoring observations preceding those now carried out by NoRP. We then review the solar microwave obtained at Toyokawa and Nobeyama and their metadata. The datasets are publicly provided by the Solar Data Archive System (SDAS) operated by the Astronomy Data Center of the NAOJ, via http (https://solar.nro.nao.ac.jp/norp/) and FTP (ftp://solar-pub.nao.ac.jp/pub/nsro/norp/) protocols.
