Concerning five-minute variations of the
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V. M. Grigoryev; M. L. Demidov
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Article
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1991
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Springer
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English
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For the purpose of identifying five-min oscillations we analyze long-term continuous observations of the solar magnetic field (with a duration from 3 to 11 hours) with 0.5 D e spatial resolution obtained with the STOP telescope (Solar Telescope for Operative Predictions) at the Sayan observatory in