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Record W4402863437 · doi:10.3847/2041-8213/ad5a8c

Metis Observation of the Onset of Fully Developed Turbulence in the Solar Corona

2024· article· en· W4402863437 on OpenAlexaboutno aff
Daniele Telloni, L. Sorriso‐Valvo, G. P. Zank, M. Velli, V. Andretta, Denise Perrone, Raffaele Marino, Francesco Carbone, A. Vecchio, L. Adhikari, Lingling Zhao, Sabrina Guastavino, Fabiana Camattari, Chen Shi, Nikos Sioulas, Zesen Huang, M. Romoli, E. Antonucci, Vania Da Deppo, Silvano Fineschi, C. Grimani, P. Heinzel, J. D. Moses, G. Naletto, G. Nicolini, D. Spadaro, M. Stangalini, L. Teriaca, M. Uslenghi, L. Abbo, F. Auchère, R. Aznar Cuadrado, A. Berlicki, R. Bruno, A. Burtovoi, Gerardo Capobianco, C. Casini, Marta Casti, Paolo Chioetto, Alain Jody Corso, R. D’Amicis, Yara De Leo, Michele Fabi, F. Frassati, Fabio Frassetto, S. Giordano, S. L. Guglielmino, G. Jerse, Federico Landini, Alessandro Liberatore, Enrico Magli, G. Massone, Giuseppe Nisticó, M. Pancrazzi, Maria Guglielmina Pelizzo, Hardi Peter, Christina Plainaki, Luca Poletto, F. Reale, P. Romano, G. Russano, C. Sasso, U. Schühle, S. K. Solanki, L. Strachan, T. Straus, Roberto Susino, R. Ventura, A. Volpicelli, J. Woch, L. Zangrilli, G. Zimbardo, Paola Zuppella

Bibliographic record

VenueThe Astrophysical Journal Letters · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsnot available
FundersGoddard Space Flight CenterOffice of Experimental Program to Stimulate Competitive ResearchUniwersytet WrocławskiOffice of Naval ResearchBundesministerium für Wirtschaft und EnergieIstituto Nazionale di AstrofisicaAgenzia Spaziale ItalianaNational Science FoundationVetenskapsrådetGrantová Agentura České RepublikyHeliophysics DivisionNational Aeronautics and Space Administration
KeywordsPhysicsCorona (planetary geology)TurbulenceAstrophysicsSolar windSolar radiusSpectral densityScalingPlasmaCoronal mass ejectionMeteorologyGeometry

Abstract

fetched live from OpenAlex

Abstract This Letter reports the first observation of the onset of fully developed turbulence in the solar corona. Long time series of white-light coronal images, acquired by Metis aboard Solar Orbiter at 2 minutes cadence and spanning about 10 hr, were studied to gain insight into the statistical properties of fluctuations in the density of the coronal plasma in the time domain. From pixel-by-pixel spectral frequency analysis in the whole Metis field of view, the scaling exponents of plasma fluctuations were derived. The results show that, over timescales ranging from 1 to 10 hr and corresponding to the photospheric mesogranulation-driven dynamics, the density spectra become shallower moving away from the Sun, resembling a Kolmogorov-like spectrum at 3 R ⊙ . According to the latest observation and interpretive work, the observed 5/3 scaling law for density fluctuations is indicative of the onset of fully developed turbulence in the corona. Metis observation-based evidence for a Kolmogorov turbulent form of the fluctuating density spectrum casts light on the evolution of 2D turbulence in the early stages of its upward transport from the low corona.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.851
Threshold uncertainty score0.245

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

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 head0.012
GPT teacher head0.229
Teacher spread0.217 · 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 teacher head, 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".

Quick stats

Citations12
Published2024
Admission routes1
Has abstractyes

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