Periodic beaded stripes in meter-wave solar radio bursts are modeled via DPR instability to constrain source magnetic fields to 0.2-1.7 G and densities to (1-7)×10^8 cm^{-3}.
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New observations of ~160 s VLPs in metric type-I bursts show spatiotemporal correlation with ~170 s oscillations in sunspot umbrae, supporting modulation by slow magnetoacoustic waves via plasma emission.
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Coronal Diagnostics Via Modelling Periodic-Beaded Stripes of Solar Radio Bursts
Periodic beaded stripes in meter-wave solar radio bursts are modeled via DPR instability to constrain source magnetic fields to 0.2-1.7 G and densities to (1-7)×10^8 cm^{-3}.
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Spatio-temporal Characteristics of Very Long-periodic Pulsations in Solar Metrewave Bursts: Implications for their Origins
New observations of ~160 s VLPs in metric type-I bursts show spatiotemporal correlation with ~170 s oscillations in sunspot umbrae, supporting modulation by slow magnetoacoustic waves via plasma emission.