@article{oai:nagoya.repo.nii.ac.jp:00019535,
 author = {TANAKA, HARUO and KAKINUMA, TAKAKIYO},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Jan},
 note = {An 8-element interferometer with quarter-wavelength plates was completed in June, 1954. Each aerial has a paraboloidal reflector, 1.5 metre in diameter which can automatically follow the sun. Aerials are placed in E-W direction at 6.45 metres (86λ) intervals. The main lobes are spaced 40' apart and have half-power widths of 4.5' around the local noon. Observations can be made for about five hours a day. Two dimensional location of radio spots is partially possible because the scanning direction gradually changes in a day except for the periods around the equinoxes. Quarter-wavelength plates are mounted over the paraboloidal reflectors and they can be driven simultaneously. They are so designed as to minimize the reflection. To improve the accuracy of measurement, a square-law detector is used and a hot load is prepared for daily calibrations.},
 pages = {102--109},
 title = {MULTIPLE ELEMENT INTERFEROMETER FOR LOCATING SOURCES OF SOLAR NOISE AT 4,000 MEGACYCLES (2)},
 volume = {3},
 year = {1956}
}