Title: Reception of the Jupiter Decameter Waves at Mt. Zao Observatory
Abstract: HIROSHI OYA, AKIRA MORIOKA, and MINORU KONDO Upper Atmosphere and Space Research Laboratory TOhoku University, Katahira, Sendai 980, Japan (Received January 11, 1975) Abstract: A new station for the observation of Jovian decameter wave emissions has been developed at Mt. Zao Observatory . Using the dipole antenna with quarter wavelength elements, that is equipped with a reflector element, gives a threshold value, 10-21 Watt/m2Hz. From Oct. 20, 1974 , a succesful observation of the decameter wave emissions provides the data that give an identification of the main and the early sources of the emissions; it is also confirmed that the early source emissions are controlled by the position of Io satellite. The galactic decameter waves are also identified; the maximum value of the measured galactic intensity is 5 X 10-19 Wattim2Hz.
Publication Year: 1975
Publication Date: 1975-04-01
Language: en
Type: article
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Cited By Count: 3
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