A multi-scale spectral pipeline using deep learning filament detection automatically identifies 91 oscillatory events in two weeks of 2014 GONG data, recovering known events and finding new ones with periods 20-126 min.
Bulletin of the American Meteorological Society , year = 1998, month = jan, volume =
15 Pith papers cite this work. Polarity classification is still indexing.
15
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
verdicts
UNVERDICTED 15roles
background 2polarities
background 2representative citing papers
Frequent EUV microflashes at solar plume bases, each releasing ~10^24 erg, are identified as a new unipolar network event and suggested as a candidate mechanism to power the open corona and solar wind.
pKANrtm uses a physics-aware multi-fidelity KAN to emulate high-fidelity radiative transfer coefficients for atmospheric correction with superior accuracy and large speedups over direct libRadtran runs.
The atmosphere of TOI-1130b shows high metallicity, low C/O, and elevated mean molecular weight consistent with ex-situ formation beyond the water ice line.
Experimental characterization of a turbulent boundary layer's response to a plasma-actuated synthetic large-scale structure reveals correlations between induced near-wall motions and phase-dependent modulation of turbulence production and transport.
A hybrid MCMC-CWT approach infers time-dependent power-law plus white-noise backgrounds to evaluate local significance of oscillations in non-stationary astrophysical signals.
Atmospheric response to Gulf Stream front shifts is strongly resolution-dependent below 50 km and NAO leads GSF shifts by 2-3 years only during 1972-2018 with non-stationary behavior linked to oceanic circulation and Rossby waves.
Multi-height Hα observations of a sunspot reveal standing and propagating slow magnetoacoustic waves whose phase relations support a non-ideal chromospheric acoustic resonator model.
The assessment finds that standard TOA methods detect both symmetric and anti-symmetric Lamb modes in noise-free simulations, with noise mainly affecting early symmetric arrivals, and introduces frequency-domain thresholding in CWT plus local-minima AIC to improve robustness.
Hybrid simulations of tearing reconnection show magnetic energy converts to ion bulk flows and heating in the nonlinear phase, with island contraction driving parallel ion temperature anisotropy that firehose instabilities regulate by redistributing energy to the perpendicular direction.
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.
Pre-flare IRIS observations of an X9 flare reveal 7-21 minute oscillations and rising Si IV velocities consistent with slow coronal magnetic destabilization before rapid reconnection.
In a bias-cleaned sample of main-sequence stars, magnetic activity above solar maximum accounts for non-detection of p-modes in 32% of cases where amplitude is predicted sufficient, while stars with photometric activity index above 2000 ppm have 98.3% probability of no detected oscillations.
Collates archival stellar activity and rotation data for potential HWO targets, finding measurements for at least 70% of high-interest systems but activity cycles for fewer than 20%.
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
-
Response of a Turbulent Boundary Layer to a Synthetic Periodic Large-Scale Structure
Experimental characterization of a turbulent boundary layer's response to a plasma-actuated synthetic large-scale structure reveals correlations between induced near-wall motions and phase-dependent modulation of turbulence production and transport.