PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.
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5 Pith papers cite this work. Polarity classification is still indexing.
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Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.
A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.
The paper presents quantitative metrics and thresholds for selecting the Prime Sample of 15,000 stars in the PLATO LOPS2 field to enable ground-based follow-up of exoplanet candidates.
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
citing papers explorer
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PIMMS: Pulsation-Informed Magnetic Mapping of Stars with Zeeman-Doppler Imaging I. Formalism and numerical tests
PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.
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Investigating the impact of Solar Fusion III reaction rates on helioseismic constraints and solar neutrino fluxes
Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.
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How plasma coupling and convective-zone depth shape the rotation of solar-mass stars
A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.
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The PLATO field selection process III. Selection of the Prime Sample for the LOPS2 field
The paper presents quantitative metrics and thresholds for selecting the Prime Sample of 15,000 stars in the PLATO LOPS2 field to enable ground-based follow-up of exoplanet candidates.
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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.