Multi-wavelength timing analysis of an X-class flare reveals temperature-dependent phase drifting in 5-minute QPPs, interpreted as evidence for periodic magnetic reconnection triggered by lower-atmosphere oscillations.
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Simulations show MUSE-resolution intensity spectra can infer the density fluctuation spectrum inside coronal loops.
citing papers explorer
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Phase-drifting with emitting plasma temperature in the quasi-periodic pulsations of an X-class solar flare
Multi-wavelength timing analysis of an X-class flare reveals temperature-dependent phase drifting in 5-minute QPPs, interpreted as evidence for periodic magnetic reconnection triggered by lower-atmosphere oscillations.
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Numerical simulations of waves and turbulence in coronal loops: observables and spectra
Simulations show MUSE-resolution intensity spectra can infer the density fluctuation spectrum inside coronal loops.