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.
Title resolution pending
2 Pith papers cite this work, alongside 9 external citations. Polarity classification is still indexing.
2
Pith papers citing it
9
external citations · OpenAlex
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Recurrent coronal jets show QPPs of 6-13 min periods driven by periodic reconnection, with flux periodicities and sub-cooling timescales implying persistent localized heating in fan-spine structures.
citing papers explorer
-
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.
-
Recurrent Coronal Jets and QPPs: Periodic Reconnection and Localized Heating Across Quiet-Sun to Active Regions
Recurrent coronal jets show QPPs of 6-13 min periods driven by periodic reconnection, with flux periodicities and sub-cooling timescales implying persistent localized heating in fan-spine structures.