{"total":11,"items":[{"citing_arxiv_id":"2606.26304","ref_index":11,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"DKIST Unveils Four-Lobed Stokes U Profiles in a Magnetically Complex Sunspot Penumbra","primary_cat":"astro-ph.SR","submitted_at":"2026-06-24T18:50:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"DKIST observations identify four-lobed Stokes U profiles as a potential signature of line-of-sight magnetic azimuth variation in sunspot penumbrae.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25217","ref_index":112,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Standing oscillations in a resonant sunspot atmosphere captured by integral field spectroscopy","primary_cat":"astro-ph.SR","submitted_at":"2026-06-23T22:32:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Integral field spectroscopy of Na I D1/D2 lines reveals standing ~5.5 mHz oscillations at a sunspot umbral center indicating resonance-cavity dynamics, with propagating modes and damping at the boundary.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17677","ref_index":21,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST","primary_cat":"astro-ph.SR","submitted_at":"2026-06-16T08:44:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"DKIST VBI observations identify 30 spicule events triggered by microfilaments as small as 0.17 Mm, revealing two morphological classes and occasional twisting motions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13291","ref_index":46,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Automatic detection of Flare Ribbon Fine Structures as Proxies for Plasmoid Dynamics in Flare Reconnection","primary_cat":"astro-ph.SR","submitted_at":"2026-06-11T12:46:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"An automated detection method applied to simulated flare ribbon data identifies fine structures whose motions and flux distribution are consistent with plasmoid-mediated reconnection.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.07989","ref_index":80,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Sunrise III: Instrument, mission, data, and first results","primary_cat":"astro-ph.SR","submitted_at":"2026-06-06T05:42:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Overview paper introducing the Sunrise III balloon-borne solar observatory, its 2024 flight, data volume, and the focus issue containing first scientific results.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06886","ref_index":26,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Temperature Diagnostics of Chromospheric Fibrils using DKIST/ViSP Observations: K-Means Clustering Approach","primary_cat":"astro-ph.SR","submitted_at":"2026-06-05T04:06:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"K-means clustering of NICOLE inversions on DKIST/ViSP observations shows temperature dropping ~1000 K along fibrils from footpoints to mid-axis, abrupt lateral changes of hundreds of K, and denser fibrils associated with cooler downflowing plasma.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21230","ref_index":14,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Solar Vortices: Catalysts of Magnetoacoustic Wave Dissipation and Atmospheric Heating","primary_cat":"astro-ph.SR","submitted_at":"2026-05-20T14:21:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations find vortex regions exhibit higher temperatures and faster shock upflows, indicating they boost magnetoacoustic wave dissipation in the chromosphere.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19472","ref_index":63,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Chromospheric resonator model for sunspot revealed by multi-height observation of umbral wave","primary_cat":"astro-ph.SR","submitted_at":"2026-05-19T07:23:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"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.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.01511","ref_index":102,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"On the Radial Evolution of the Solar Wind : The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations","primary_cat":"astro-ph.SR","submitted_at":"2026-05-02T16:05:34+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A new source alignment technique applied to PSP and SO data reveals the solar wind speed increases by an average of 45% per radial decade between the spacecraft, indicating ongoing acceleration beyond 15 solar radii.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.17330","ref_index":78,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Quasi-periodic pulsations and three-dimensional magnetic reconnection during 2022 March 31 flare observed by IRIS & STIX","primary_cat":"astro-ph.SR","submitted_at":"2026-04-19T08:53:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In the 2022 March 31 solar flare, hard X-ray QPPs correlate with UV pulsations in stationary ribbon regions tied to a specific loop system in a large-scale 3D reconnection structure, while slipping kernels experience weaker non-thermal energization.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.07137","ref_index":17,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Assessment of DKIST/VTF Capabilities for the Detection of Local Acoustic Source Wavefronts","primary_cat":"astro-ph.SR","submitted_at":"2026-02-06T19:19:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Optimal wavelength strategies for DKIST/VTF enable detection of local acoustic source wavefronts from solar simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}