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Decametric Radio Pulses from Jupiter: Characteristics

C. N. Olsson and Alex G. Smith
Science
New Series, Vol. 153, No. 3733 (Jul. 15, 1966), pp. 289-290
Stable URL: http://www.jstor.org/stable/1719499
Page Count: 2
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Abstract

On occasion the decametric radio bursts from Jupiter contain pulses of millisecond duration. Study of data for 2 years shows that the distribution in Jovian longitude of these fast pulses is different from that of the more common pulses of longer duration. The two classes of pulses also appear to be differently affected by the position of the innermost Galilean satellite.

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