Superposition of standing slow and entropy modes in a 1D coronal loop with thermal conduction produces non-exponential damping and phase shifts in compressive oscillations.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.SR 3years
2026 3verdicts
UNVERDICTED 3representative 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.
A review synthesizing Fourier, Lomb-Scargle, wavelet, synchrosqueezed, and EMD methods plus statistical tests for solar/stellar periodicity detection, with synthetic benchmark guidelines.
citing papers explorer
-
Entropy-mode imprints in the solar corona: non-exponential damping and phase shifts of compressive oscillations
Superposition of standing slow and entropy modes in a 1D coronal loop with thermal conduction produces non-exponential damping and phase shifts in compressive oscillations.
-
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.
-
Modern Time-Series and Spectral Methods for Analyzing Solar and Stellar Oscillatory Signals
A review synthesizing Fourier, Lomb-Scargle, wavelet, synchrosqueezed, and EMD methods plus statistical tests for solar/stellar periodicity detection, with synthetic benchmark guidelines.