@article{oai:nagoya.repo.nii.ac.jp:00019836,
 author = {TANAKA, Haruo},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Mar},
 note = {A project is proposed of a swept-lobe interferometer to observe a rapidly changing burst at microwave frequency region. The brightness distribution as well as the distribution of circularly polarized components can be observed. A frequency of 5 Gc/s and a bandwidth of 3 Mc/s are recommended. A 2.4-m-dish 32-element interferometer is considered to be suitable for the quick scanning. Additional 2 elements to compose a compound phase-switch interferometer will be useful for the high-resolution study of S-component. A heliographic scanning at a moderate speed is possible by adding 16 N-S elements. The scanning frequency is limited by S/N ratio, and the maximum one is once per 2 seconds for a fan-beam scan, and once per 3 minutes for a heliographic scan.},
 pages = {49--57},
 title = {A PROJECT OF MULTIPLE-ELEMENT SWEPT-LOBE INTERFEROMETER FOR THE STUDY OF SOLAR RADIO BURSTS},
 volume = {13},
 year = {1966}
}