@article{oai:nagoya.repo.nii.ac.jp:00019464, author = {田中, 春夫 and 柿沼, 隆清 and TANAKA, Haruo and KAKINUMA, Takakiyo}, issue = {1-2}, journal = {空電研究所報告}, month = {Mar}, note = {With the intention of locating sources of radio noise from the disturbed sun at 4000 MC,an interferometer with 5 aerials has been constructed since May in 1952. Each aerial has a paraboloidal reflector of size 1.5 metre in diameter,which can be rotated equatorially. They are placed in E-W direction at 6 m intervals. The lobes will be spaced 43' apart and each lobe will have a half-power width of 7.8'. As the sun passes through the aerial pattern,it would be scanned stripwise by each lobe in turn for a few hours near meridian passage. It is preferable to use 8 aerials in order to join them together with minimum loss,but the financial condition compelled us to 5 for the time being. Test observations are expected to be performed in March 1953. Details will be reported in the next bulletin.}, pages = {55--61}, title = {4,000MCにおける太陽雑音源探知装置I : 設計概要}, volume = {3}, year = {1953} }