A multi-height extrapolation framework using chromospheric vector data recovers a pre-eruptive flux-rope configuration in an observed solar filament, outperforming photosphere-only models in simulation tests.
Title resolution pending
9 Pith papers cite this work, alongside 765 external citations. Polarity classification is still indexing.
9
Pith papers citing it
765
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
years
2026 9roles
background 1polarities
background 1representative citing papers
JWST NIRISS/SOSS data yield a transmission spectrum of the 23 Myr V1298 Tau c showing H2O absorption and an atmospheric metallicity of 14.8^{+56}_{-12} times solar, lower than mature planets of similar mass.
Multi-height data reveal a dominant standing sausage mode (~1-2 mHz) and a propagating fluting mode (m=2, ~2-3.5 mHz) in pore boundary oscillations, with the first mode carrying 66-86% of the eigenvalue power.
Physics-based annual TSI reconstruction over three millennia yields a maximum difference of 1.04 W/m² in 50-year running means.
The transmission spectrum of AU Mic b is dominated by the transit light source effect from stellar spots, yielding only weak atmospheric constraints with a preferred scale height below 185 km.
Pandora simulations recover stellar photospheric temperatures to ~30 K with no bias and reduce simple spot contamination from 100-1000 ppm to under 10 ppm, but complex spot geometries leave ~1000 ppm residuals.
Magnetic filaments in the solar convection zone form in two stages: a kinematic frozen-in phase at convective cell boundaries followed by a dynamic phase where magnetic pressure alters the flow until kinetic and magnetic energy densities become comparable.
Light bridge transverse motions appear as projections of umbral core dynamics with coupling to coronal loops.
Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.
citing papers explorer
-
Chromospheric magnetic field extrapolations reveal the flux-rope configuration of a solar filament
A multi-height extrapolation framework using chromospheric vector data recovers a pre-eruptive flux-rope configuration in an observed solar filament, outperforming photosphere-only models in simulation tests.
-
KRONOS I: The $1{-}2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
JWST NIRISS/SOSS data yield a transmission spectrum of the 23 Myr V1298 Tau c showing H2O absorption and an atmospheric metallicity of 14.8^{+56}_{-12} times solar, lower than mature planets of similar mass.
-
Multi-height Identification of Sausage and Fluting Eigenmodes in a Solar Pore
Multi-height data reveal a dominant standing sausage mode (~1-2 mHz) and a propagating fluting mode (m=2, ~2-3.5 mHz) in pore boundary oscillations, with the first mode carrying 66-86% of the eigenvalue power.
-
Reconstruction of annual solar irradiance over the last three millennia
Physics-based annual TSI reconstruction over three millennia yields a maximum difference of 1.04 W/m² in 50-year running means.
-
The HST/WFC3 Transmission Spectrum of AU Mic b Part I: An Atmosphere Obscured by Contamination and Systematics
The transmission spectrum of AU Mic b is dominated by the transit light source effect from stellar spots, yielding only weak atmospheric constraints with a preferred scale height below 185 km.
-
NASA's Pandora SmallSat Mission: Simulating the Impact of Stellar Photospheric Heterogeneity and Its Correction
Pandora simulations recover stellar photospheric temperatures to ~30 K with no bias and reduce simple spot contamination from 100-1000 ppm to under 10 ppm, but complex spot geometries leave ~1000 ppm residuals.
-
Two stages of magnetic filament formation in the solar convective zone
Magnetic filaments in the solar convection zone form in two stages: a kinematic frozen-in phase at convective cell boundaries followed by a dynamic phase where magnetic pressure alters the flow until kinetic and magnetic energy densities become comparable.
-
Apparent Transverse Motion of Light Bridges Coupled to Coronal Loop Dynamics
Light bridge transverse motions appear as projections of umbral core dynamics with coupling to coronal loops.
-
Sunrise III: Instrument, mission, data, and first results
Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.