A forward-modeling framework combining refractive ray tracing in a 3D coronal model with radiative transfer produces synthetic 40-800 MHz radio maps that reproduce the quiet-Sun spectrum for Carrington rotation 2298.
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12 Pith papers cite this work. Polarity classification is still indexing.
12
Pith papers citing it
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2026 12roles
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First-year SWAYS observations report a superflare on EK Draconis with no low-frequency radio signal, interpreted as evidence that dense coronae in active stars inhibit type II/III burst instabilities.
GMRT sub-GHz survey of 44 magnetic hot stars detects emission in 11 cases and finds scaling of radio luminosity with magnetic field and rotation period consistent with higher-frequency work.
SPADE demonstrates a small, fully digital phased array spectrograph for decameter solar radio observations, with first 2024 data showing temporal and frequency resolution suitable for coronal turbulence and propagation studies.
Rotationally modulated radio pulses with near-100% circular polarization from M dwarf ASKAP J181335-604720 are interpreted as coherent electron cyclotron maser emission from its magnetosphere based on simultaneous radio-optical observations.
A tiered observational strategy is outlined to identify planetary-scale broadband radio technosignatures (BRaTs) from advanced civilizations up to 100 pc away using multi-parameter diagnostics to separate them from natural signals.
Statistical analysis of solar events shows type II radio burst starting frequencies vary by source region and anti-correlate with proton spectral indices, constraining SEP acceleration mechanisms.
Six new Galactic radio transients found and classified into two types, proposed to originate from wide-orbit white dwarf binaries.
VLA observations of six cataclysmic variables reveal polarized radio emission consistent with coherent mechanisms like electron-cyclotron maser emission or plasma radiation.
Reviews coherent and incoherent radio emission in ordered stellar magnetospheres, links massive-star CBO mechanism to UCD luminosity trends, and predicts SKA detection of ~1000 UCDs to test the hypothesis.
This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.
Perspective paper on the importance of circumstellar environments around evolved massive stars for supernova studies and the observational advances expected from the Square Kilometre Array.
citing papers explorer
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A sample of short-lived Galactic radio transients from ASKAP VAST
Six new Galactic radio transients found and classified into two types, proposed to originate from wide-orbit white dwarf binaries.
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A broadband search for coherent radio emission in cataclysmic variables
VLA observations of six cataclysmic variables reveal polarized radio emission consistent with coherent mechanisms like electron-cyclotron maser emission or plasma radiation.