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Record W4327750075 · doi:10.1007/s11207-023-02137-2

Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter

2023· article· en· W4327750075 on OpenAlexaboutno aff
M. Mierla, H. Cremades, V. Andretta, Iulia Chifu, A. N. Zhukov, Roberto Susino, F. Auchère, A. Vourlidas, Dana-Camelia Talpeanu, L. Rodríguez, Jan Janssens, B. Nicula, R. Aznar Cuadrado, D. Berghmans, А. Бемпорад, Elke D’Huys, Laurent Dolla, S. Gissot, G. Jerse, Emil Kraaikamp, David M. Long, Benjamin Mampaey, Christian Möstl, P. Pagano, S. Parenti, Matthew J. West, O. Podladchikova, M. Romoli, C. Sasso, K. Stegen, L. Teriaca, W. T. Thompson, C. Verbeeck, Emma E. Davies

Bibliographic record

VenueSolar Physics · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicSolar and Space Plasma Dynamics
Canadian institutionsnot available
FundersU.S. Naval Research LaboratoryOffice of Naval ResearchBundesministerium für Wirtschaft und EnergieDeutsches Zentrum für Luft- und RaumfahrtConsejo Nacional de Investigaciones Científicas y TécnicasCentre National d’Etudes SpatialesScience and Technology Facilities CouncilEuropean CommissionAkademie Věd České RepublikyNational Aeronautics and Space AdministrationEuropean Space AgencyUK Space AgencyBelgian Federal Science Policy Office
KeywordsOrbiterSolar prominenceCoronal mass ejectionPhysicsCoronagraphObservatoryAstronomyCorona (planetary geology)Extreme ultravioletSpace weatherSolar observatorySolar windAstrophysicsRemote sensingAstrobiologyMagnetic fieldGeologyExoplanetVenusPlanetOptics

Abstract

fetched live from OpenAlex

Abstract On February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better.

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 score0.005
Threshold uncertainty score0.009

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)0.0010.000

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 head0.027
GPT teacher head0.246
Teacher spread0.220 · 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".

Quick stats

Citations4
Published2023
Admission routes1
Has abstractyes

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