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Record W2776482757

Physical Properties Of Faint Meteors Through High-Resolution Observations

2017· article· en· W2776482757 on OpenAlexaboutno aff
Dilini Subasinghe

Bibliographic record

VenueScholarship@Western (Western University) · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
Fundersnot available
KeywordsMeteoroidPhysicsAstrobiology
DOInot available

Abstract

fetched live from OpenAlex

Small, faint meteors (with masses between 10-7 and 10-4 kg) were once part of an asteroid or comet, and collide with Earth's atmosphere daily. Studying meteors is an effective way to survey the physical properties of their parent bodies. Meteor light curves and orbital information is easily obtained from wide-field observations, from which meteoroid structure can be inferred through meteoroid ablation modelling. A high-resolution narrow-field camera can provide much more detail about the poorly understood ablation processes and physical properties of the meteoroid. The goal of this thesis is to better understand the physical properties of meteors using high-resolution optical observations.\nIn the first part of this work, wide-field and narrow-field optical observations of faint meteors were combined to determine what relationships, if any, exist between meteor light curve shapes, orbits, and fragmentation behaviour. Most meteors were found to have symmetric light curves, show fragmentation in the form of a long trail, and come from cometary bodies. More than 90% of meteors observed with the high-resolution camera system showed some form of fragmentation. Unexpectedly, the dynamically asteroidal meteoroids fragmented as often as the dynamically cometary meteoroids, suggestive of dynamical mixing or contamination.\nIn the second part of this work, the luminous efficiency (the fraction of kinetic energy used for visible light production) of meteors was investigated. It is crucial for determining meteoroid mass, and past results vary by up to two orders of magnitude. An attempt at determining luminous efficiency through the classical ablation equations was made, and verified on simulated meteor data, while quantifying the uncertainty in the method. This was then applied to fifteen real meteor events, observed with the Canadian Automated Meteor Observatory. This is the first study which compares photometric and dynamic meteoroid masses to determine luminous efficiency, with modern high-resolution observations. Twelve of the meteors had luminous efficiency values less than 1% (agreeing with the lower end results of past studies), and there was no obvious trend with speed. A weak negative trend was observed with meteoroid mass, implying that smaller meteoroids radiate more efficiently.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.002
Threshold uncertainty score0.003

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
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 head0.143
GPT teacher head0.296
Teacher spread0.153 · 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

Citations1
Published2017
Admission routes1
Has abstractyes

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