Sun-as-a-star Hα spectra show location-dependent signatures (blueshifted/redshifted emission for limbs, absorptions for disks, timing and wing differences by front/far side and active/quiet regions) that can diagnose stellar eruption source regions.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Proposes the Nautilus observatory concept for time-resolved flare spectroscopy on GKM stars to create empirical spectral templates for improved planetary habitability simulations.
A review synthesizing manifestations of magnetic activity in cool stars and its relevance to exoplanet science via the solar-stellar connection.
citing papers explorer
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Can We Distinguish the Source Region Location of Filament/Prominence Eruptions from the Sun-as-a-star H$\alpha$ Spectrum?
Sun-as-a-star Hα spectra show location-dependent signatures (blueshifted/redshifted emission for limbs, absorptions for disks, timing and wing differences by front/far side and active/quiet regions) that can diagnose stellar eruption source regions.
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Nautilus: Fast Time-Resolved Spectroscopy of GKM Stellar Flares and Their Implications for Planetary Habitability
Proposes the Nautilus observatory concept for time-resolved flare spectroscopy on GKM stars to create empirical spectral templates for improved planetary habitability simulations.
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Magnetic activity in cool stars: manifestations and relevance to exoplanets
A review synthesizing manifestations of magnetic activity in cool stars and its relevance to exoplanet science via the solar-stellar connection.