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Record W1508707436

Magneto-hydrodynamics Simulation in Astrophysics

2011· dissertation· en· W1508707436 on OpenAlexvenueno aff
Bijia Pang

Bibliographic record

VenueLibrary and Archives Canada (Government of Canada) · 2011
Typedissertation
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
Fundersnot available
KeywordsPhysicsMagnetohydrodynamicsMagnetic reconnectionAccretion (finance)AstrophysicsMagnetic fieldComputational physics
DOInot available

Abstract

fetched live from OpenAlex

Magnetohydrodynamics (MHD) studies the dynamics of an electrically conducting fluid under the influence of a magnetic field.\nMany astrophysical phenomena are related to MHD,\nand computer simulations are used to model these dynamics.\nIn this thesis,\nwe conduct MHD simulations of non-radiative black hole accretion as well as fast magnetic reconnection.\nBy performing large scale three dimensional parallel MHD simulations on supercomputers and using a deformed-mesh algorithm,\nwe were able to conduct very high dynamical range simulations of black hole accretion of Sgr A* at the Galactic Center.\nWe find a generic set of solutions,\nand make specific predictions for currently feasible observations of rotation measure (RM).\nThe magnetized accretion flow is subsonic and lacks outward convection flux,\nmaking the accretion rate very small and having a density slope of around $-1$.\nThere is no tendency for the flows to become rotationally supported,\nand the slow time variability of the RM is a key quantitative signature of this accretion flow.\n\nWe also provide a constructive numerical example of fast magnetic reconnection in a three-dimensional periodic box.\nReconnection is initiated by a strong,\nlocalized perturbation to the field lines and the solution is intrinsically three-dimensional.\nApproximately $30\\%$ of the magnetic energy is released in an event which lasts about one Alfv\\'en time,\nbut only after a delay during which the field lines evolve into a critical configuration.\nIn the co-moving frame of the reconnection regions,\nreconnection occurs through an X-like point,\nanalogous to the Petschek reconnection.\nThe dynamics appear to be driven by global flows rather than local processes.\n\nIn addition to issues pertaining to physics,\nwe present results on the acceleration of MHD simulations using heterogeneous computing systems \\cite{shan2006heterogeneous}.\nWe have implemented the MHD code on a variety of heterogeneous and multi-core architectures (multi-core x86, Cell, Nvidia and ATI GPU) using different languages (FORTRAN, C, Cell, CUDA and OpenCL).\nInitial performance results for these systems are presented,\nand we conclude that substantial gains in performance over traditional systems are possible.\nIn particular,\nit is possible to extract a greater percentage of peak theoretical performance from some heterogeneous systems when compared to x86 architectures.

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)0.001
metaresearch head score (Gemma)0.002
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: Other · Consensus signal: none
Teacher disagreement score0.011
Threshold uncertainty score0.038

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.001
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0010.002
Research integrity0.0020.002
Insufficient payload (model declined to judge)0.0110.004

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 head0.003
GPT teacher head0.153
Teacher spread0.149 · 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
GenreOther

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

Citations0
Published2011
Admission routes1
Has abstractyes

Explore more

Same venueLibrary and Archives Canada (Government of Canada)→Same topicAstrophysical Phenomena and Observations→French-language works237,207→