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Record W4292602907 · doi:10.3847/1538-4357/ac8103

Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations

2022· article· en· W4292602907 on OpenAlexaboutno aff
Daniele Telloni, G. P. Zank, L. Sorriso‐Valvo, R. D’Amicis, O. Panasenco, Roberto Susino, R. Bruno, Denise Perrone, L. Adhikari, Haoming Liang, Masaru Nakanotani, Lingling Zhao, Lina Hadid, Beatriz Sánchez‐Cano, Daniel Verscharen, M. Velli, C. Grimani, Raffaele Marino, Francesco Carbone, Salvatore Mancuso, Ruggero Biondo, P. Pagano, F. Reale, S. D. Bale, J. C. Kasper, A. W. Case, Thierry Dudok de Wit, K. Goetz, P. Harvey, K. E. Korreck, D. E. Larson, R. Livi, R. J. MacDowall, D. Malaspina, M. Pulupa, M. L. Stevens, P. L. Whittlesey, M. Romoli, V. Andretta, Vania Da Deppo, Silvano Fineschi, P. Heinzel, J. D. Moses, G. Naletto, G. Nicolini, D. Spadaro, M. Stangalini, L. Teriaca, Gerardo Capobianco, G. Capuano, C. Casini, Marta Casti, Paolo Chioetto, Alain Jody Corso, Yara De Leo, Michele Fabi, F. Frassati, Fabio Frassetto, S. Giordano, S. L. Guglielmino, G. Jerse, Federico Landini, Alessandro Liberatore, Enrico Magli, G. Massone, M. Messerotti, M. Pancrazzi, Maria Guglielmina Pelizzo, P. Romano, C. Sasso, U. Schühle, T. Straus, M. Uslenghi, A. Volpicelli, L. Zangrilli, Paola Zuppella, L. Abbo, F. Auchère, R. Aznar Cuadrado, A. Berlicki, A. Ciaravella, P. Lamy, A. C. Lanzafame, A. M. Malvezzi, P. Nicolosi, Giuseppe Nisticó, Hardi Peter, S. K. Solanki, L. Strachan, K. Tsinganos, R. Ventura, J. C. Vial, J. Woch, G. Zimbardo

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsnot available
FundersHeliophysics DivisionScience and Technology Facilities CouncilGoddard Space Flight CenterOffice of Experimental Program to Stimulate Competitive ResearchSwedish National Space AgencyUniwersytet WrocławskiOffice of Naval ResearchBundesministerium für Wirtschaft und EnergieNational Science FoundationAgenzia Spaziale ItalianaNuclear Safety and Security CommissionNational Aeronautics and Space AdministrationIstituto Nazionale di Astrofisica
KeywordsPhysicsSolar windCoronal holeNanoflaresOrbiterCorona (planetary geology)HeliosphereSolar minimumAstronomyAstrophysicsCoronal mass ejectionSolar observatorySolar cycle 23Coronal loopSolar cyclePlasmaMagnetic fieldAstrobiologyVenus

Abstract

fetched live from OpenAlex

Abstract The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R ⊙ above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local properties of the two streams are different. Specifically, the solar wind emanating from the stronger magnetic field region has a lower bulk flux density, as expected, and is in a state of well-developed Alfvénic turbulence, with low intermittency. This is interpreted in terms of slab turbulence in the context of nearly incompressible magnetohydrodynamics. Conversely, the highly intermittent and poorly developed turbulent behavior of the solar wind from the weaker magnetic field region is presumably due to large magnetic deflections most likely attributed to the presence of switchbacks of interchange reconnection origin.

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 categoriesMeta-epidemiology (narrow), Science and technology studies, Research integrity
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.331
Threshold uncertainty score1.000

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 studies0.0030.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.002
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 head0.026
GPT teacher head0.208
Teacher spread0.183 · 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.

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

Citations15
Published2022
Admission routes1
Has abstractyes

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