Over seven decades of solar microwave data obtained with Toyokawa and Nobeyama Radio Polarimeters
arXiv:2205.07454 · doi:10.1002/gdj3.165
Abstract
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.
29 pages, 12 figures, accepted to Geoscience Data Journal
References in corpus (2)
Cited by in corpus (3)
- Relationship of peak fluxes of solar radio bursts and X-ray class of solar flares: Application to early great solar flares
- Comparison of solar multifrequency microwave data with other solar indices for understanding solar and stellar microwave data
- Centennial solar EUV irradiance from ionospheric currents: Varying sunspot-EUV irradiance relation and modified spot-facula ratio