

Publisher: Springer Publishing Company
ISSN: 0038-0938
Source: Solar Physics, Vol.176, Iss.1, 1997-11, pp. : 171-179
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Abstract
Long-periodic pulsations with a period of tens of seconds associated with a type IV solar radio emission are found at 1420 and 2000 MHz. Some features (such as the bandwidth, periodicity, frequency drift, amplitude, and relative amplitude) of the pulsations are introduced and discussed in this paper.
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