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Record W2135557693 · doi:10.1029/2003ja010374

Simultaneous observations of field‐aligned beams and gyrating ions in the terrestrial foreshock

2004· article· en· W2135557693 on OpenAlexaff
K. Meziane, M. Wilber, C. Mazelle, D. LeQuéau, H. Kucharek, E. Lucek, H. Rème, A. M. Hamza, J. A. Sauvaud, J. M. Bosqued, I. Dandouras, G. K. Parks, Michael McCarthy, B. Klecker, A. Korth, M. B. Bavassano‐Cattaneo, R. Lundin

Bibliographic record

VenueJournal of Geophysical Research Atmospheres · 2004
Typearticle
Languageen
FieldPhysics and Astronomy
TopicIonosphere and magnetosphere dynamics
Canadian institutionsUniversity of New Brunswick
Fundersnot available
KeywordsPhysicsSolar windIonField linePopulationPitch angleAtomic physicsBow shock (aerodynamics)Guiding centerMagnetic fieldProtonShock (circulatory)Interplanetary magnetic fieldBow waveAstrophysicsAmplitudeComputational physicsShock waveGeophysicsOpticsMechanicsNuclear physics

Abstract

fetched live from OpenAlex

We examine an energetic (2–30 keV) upstream ion event presenting a clear double‐peak spectrum observed ∼1 RE upstream from the bow shock. The lower‐energy (E ∼ 3.5 keV) peak is associated with an ion beam propagating along the magnetic field direction, while the higher‐energy (E ∼ 13 keV) peak is associated with gyrating ions having pitch angles ∼30°. The latter population progressively extends to lower energies over the span of the event. During times when the field‐aligned beams were observed, the interplanetary magnetic field was remarkably steady, while the appearance of the 30° pitch angle gyrating ions was accompanied by the onset of large‐amplitude ultralow frequency fluctuations of the magnetic field. Our analysis indicates that the gyrating ions had guiding centers on field lines downstream of the field‐aligned component but that both populations could be sampled simultaneously because of the orbits of the former. We find that the downstream limit of the field‐aligned beams is populated with protons having a speed 1.68 times the solar wind velocity, which is inconsistent with any known shock‐related emission mechanisms. This boundary makes an angle of 77° with respect to the Sun‐Earth line in agreement with theoretical predictions. Just downstream of this rapid transition, gyrating ions having a flow speed of 1.52 times the solar wind speed are observed in association with ULF waves. Like the field‐aligned beams, the gyrating ions reported here have streaming speeds inconsistent with any known shock emission mechanisms. While the simultaneous observation of field‐aligned and gyrating components is possible because of the large gyration orbits of the latter, the observational sequence is consistent with a very sharp (≲1 gyroradius) boundary separating the guiding centers of each. Explicit observations of such a sharp demarcation between these populations have not been reported before, and they place a significant constraint on the production mechanisms of the two populations. Our interpretation of these observations provides a refinement of the usual framework for foreshock morphology.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
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
Bibliometrics0.0010.000
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 head0.312
Teacher spread0.286 · 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

Citations51
Published2004
Admission routes1
Has abstractyes

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