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.
Bulletin of the American Meteorological Society , year = 1998, month = jan, volume =
13 Pith papers cite this work. Polarity classification is still indexing.
13
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
verdicts
UNVERDICTED 13roles
background 2polarities
background 2representative citing papers
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.
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
-
Extreme Ultraviolet Microflashes at Plume Bases: A Candidate for Powering the Corona and Solar Wind?
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.
-
Multi-Fidelity Emulation of Atmospheric Correction Coefficients with Physics-Guided Kolmogorov-Arnold Networks
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.
-
JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line
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.
-
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.
-
A Markov-Chain-Monte-Carlo-based Hybrid Noise Inference for Continuous Wavelet Power Spectra: with Applications to Solar and Stellar Oscillatory Signals
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.
-
Chromospheric resonator model for sunspot revealed by multi-height observation of umbral wave
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.
-
Assessment of Time-of-Arrival Estimation Methods for Impact Detection in Isotropic Plates using Piezoceramic Sensors
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.
-
Tearing Driven Reconnection: Energy Conversion Involving Firehose Kinetic Instabilities (2D Hybrid M\"obius Simulations)
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 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.
-
Investigating Pre-flare Signatures in Spectroscopic Observations of an X9-class Solar Flare
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.
-
Revisiting the impact of stellar magnetic activity on the detectability of solar-like oscillations by Kepler
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.
-
HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
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%.
-
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.