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Record W4408484602 · doi:10.5194/egusphere-egu25-19935

Solar Wind Speed Maps from the Metis coronagraph observations

2025· preprint· en· W4408484602 on OpenAlexaboutno aff
S. Giordano, D. Spadaro, Roberto Susino, R. Ventura, M. Romoli, Silvano Fineschi, L. Zangrilli, Daniele Telloni

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsnot available
Fundersnot available
KeywordsMetisCoronagraphPhysicsAstronomyComputer scienceExoplanetWorld Wide WebPlanet

Abstract

fetched live from OpenAlex

This presentation outlines the Doppler dimming diagnostic method, the computational tools developed, and the solar wind speed maps derived from Metis data spanning a wide range of heliocentric distances, from approximately 1.5 to 10 solar radii, during the solar activity minimum.The Doppler dimming diagnostic, which combine simultaneous Metis observations from its two channels, polarized broadband visible light and narrowband ultraviolet H I Lyα intensity, allows for the measurement of the expanding coronal plasma speed. The presented wind speed maps are obtained from Metis data sets collected during the cruise phase of the Solar Orbiter mission, shortly after its first perihelion at approximately 0.5 AU in June 2020, as well as before and after its second perihelion in January and February 2021. These observations provide critical insights into the solar corona above approximately 3.0 solar radii, while future Solar Orbiter perihelion passages will extend this analysis to distances as close as 1.7 solar radii.The reliability of the derived wind speed values is evaluated, considering instrumental uncertainties, the inherent limitations of the diagnostic method, and key assumptions about solar corona model parameters, including electron and neutral atom kinetic temperatures and the 3D geometric configuration of the corona.As expected at the minimum of the solar cycle, the obtained maps show a clear bipolar topology with a rapid transition to higher speeds in the interface zone between equatorial streamers and high-latitude regions. The equatorial regions, where intense and relatively stable streamer belt persists, do not exhibit speeds higher than 220 km/s up to the maximum observed distance, around 6 solar radii. In contrast, within the coronal holes, already just above the minimum observed heights, around 3.5 solar radii, the wind speed reaches the maximum values detectable using Doppler dimming diagnostics applied to the neutral hydrogen line, approximately 350 km/s.The method and algorithms are further tested and applied to a sample of daily ultraviolet intensity images reconstructed from spectral data obtained by the UVCS instrument, in conjunction with visible light coronal observations performed by LASCO, both instruments onboard the SOHO mission during solar cycle 23. This extended analysis provides valuable insights into the solar wind acceleration region, covering distances between approximately 1.5 and 4.0 solar radii, encompassing nearly a full solar activity cycle, providing essential context to complement the present Solar Orbiter observations.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.024
GPT teacher head0.246
Teacher spread0.222 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations0
Published2025
Admission routes1
Has abstractyes

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