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Cited article:

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SPECTRAL STRUCTURES AND THEIR GENERATION MECHANISMS FOR SOLAR RADIO TYPE-I BURSTS

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PEAK FLUX DISTRIBUTIONS OF SOLAR RADIO TYPE-I BURSTS FROM HIGHLY RESOLVED SPECTRAL OBSERVATIONS

K. Iwai, S. Masuda, Y. Miyoshi, et al.
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Waveform and envelope field statistics for waves with stochastically driven amplitudes

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Equivalent Electric Circuit Models of Coronal Magnetic Loops and Related Oscillatory Phenomena on the Sun

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High Spectral Resolution Observation of Decimetric Radio Spikes Emitted by Solar Flares – First Results of the Phoenix-3 Spectrometer

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Spike Decomposition Technique: Modeling and Performance Tests

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New regimes of stochastic wave growth: Theory, simulation, and comparison with data

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Low-frequency modulations in the solar microwave radiation as a possible indicator of inductive interaction of coronal magnetic loops

M. L. Khodachenko, V. V. Zaitsev, A. G. Kislyakov, H. O. Rucker and S. Urpo
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Analysis of solar narrow band dm-spikes observed at 1420 and 2695 MHz

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Intrinsic variability and field statistics for the Vela pulsar -- II. Systematics and single-component fits

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Intrinsic variability and field statistics for the Vela pulsar -- III. Two-component fits and detailed assessment of stochastic growth theory

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Temporal aspects and frequency distributions of solar soft X-ray flares

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The Peak Flux Distribution of Solar Radio Bursts

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Intrinsic Variability of the Vela Pulsar: Lognormal Statistics and Theoretical Implications

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