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Record W2079014635 · doi:10.1029/2001ja900040

A global MHD and empirical magnetic field model investigation of the magnetospheric cusp

2001· article· en· W2079014635 on OpenAlexfundno aff
F. R. Fenrich, J. G. Luhmann, J. A. Fedder, S. P. Slinker, C. T. Russell

Bibliographic record

VenueJournal of Geophysical Research Atmospheres · 2001
Typearticle
Languageen
FieldPhysics and Astronomy
TopicIonosphere and magnetosphere dynamics
Canadian institutionsnot available
FundersNatural Sciences and Engineering Research Council of Canada
KeywordsMagnetohydrodynamicsPhysicsField lineInterplanetary magnetic fieldMagnetosphereGeophysicsCusp (singularity)Magnetic fieldDipole model of the Earth's magnetic fieldAstrophysicsSolar windGeometryMathematics

Abstract

fetched live from OpenAlex

Magnetic field configurations, cusp locations, merging, and interconnection regions for the Lyon‐Fedder global magnetohydrodynamic (MHD) simulation model and the Tsyganenko 96 (T96_01) empirical model are presented and compared for three different interplanetary magnetic field (IMF) directions (north, south, and dusk directed). Field line configurations indicate a significantly larger magnetosphere in the T96_01 model compared to the MHD model for all IMF directions. In each of the models the polar cusp is identified by depressions in the magnetic field residual and by the boundary between dayside closed and open field lines. It is found that the MHD model exhibits a much stronger residual magnetic field depression in the cusp region than does the T96_01 model. The MHD field depression is associated with the presence of diamagnetic magnetosheath plasma that enters the cusp via the MHD merging process. In the northward IMF case, MHD merging above both poles results in an MHD open‐closed field line boundary located at 89° invariant latitude with MHD cusp plasma and field depressions centered on closed field lines near 81°. The T96_01 model is very different from this with its north IMF open‐closed boundary located at 79° invariant latitude. For the southward IMF case the T96_01 open‐closed boundary at 74° invariant latitude lies slightly poleward of the MHD open‐closed boundary at 73°. In this case the MHD cusp plasma is centered near 75° invariant latitude. In the dusk‐directed IMF case the MHD cusp plasma shifts ∼2 hours in magnetic local time (MLT) toward dusk and remains poleward of the MHD open‐closed boundary. In this case the MHD dayside open‐closed boundary extends from dawn to dusk, while the T96_01 dayside open‐closed boundary extends only from dawn to ∼13 MLT and near local noon is coincident with the MHD boundary at ∼74° invariant latitude. Differences between the two models are due in large part to differences in the form of their interconnectivity with the interplanetary magnetic field lines. For each IMF direction the MHD merging locations and T96_01 strongest interconnection regions are identified and are found to be very different. On the basis of comparisons with numerous case and statistical studies of the cusp it is concluded that the MHD model provides a fairly realistic representation of the cusp and dayside magnetic field configuration, while the T96_01 model is limited in its ability to model the cusp region.

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)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.017

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
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 head0.026
GPT teacher head0.315
Teacher spread0.289 · 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 designSimulation or modeling
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

Citations8
Published2001
Admission routes1
Has abstractyes

Explore more

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