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Record W237885010

Using HiRISE Digital Elevation Models to Investigate the Peripheral Peak Ring Morphology in the Martian Impact Crater Tooting

2010· article· en· W237885010 on OpenAlexaff
Jason Nycz, A. R. Hildebrand

Bibliographic record

VenueLPI · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversity of Calgary
Fundersnot available
KeywordsImpact craterGeologySlumpingDigital elevation modelMartianElevation (ballistics)EjectaMars Exploration ProgramGeomorphologyAstrobiologyGeometryRemote sensing
DOInot available

Abstract

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Introduction: Examination of MOC, MOLA HRSC, THEMIS, and most recently HiRISE data reveal the presence of partial or completely collapsed rims in some Martian impact craters. These collapse features have been named Peripheral Peak Rings (PPR) [1]. The 29km diameter impact crater Tooting is an excellent example of a young, largely uneroded complex impact crater which contains a PPR. By generating digital elevation models (DEM’s) from HiRISE stereo data, detailed topographical information was obtained about the PPR in this crater. These data assisted in reconstructing the original rim of the Tooting crater before PPR formation, and allowed for the development of a robust PPR formation model. Peripheral Peak Ring Formation: PPR are blocks from the crater rim that separated and slid downwards across the terraced zone until stopping near the crater floor. PPR form when the crater rim wall, after conventional slumping to form the terraced zone overlying the slump blocks (in the case of a complex crater), fails. PPR can be differentiated from the outermost terrace zone based on morphology. Whereas the slump blocks that form the terraces show downward displacement consistent with normal faulting, PPR undergo displacement that is mostly lateral, across the tops of the terraces (in the case of complex craters). This causes the tops of some PPR to be higher in elevation than the resulting crater rim, a phenomenon not seen in terraces. Examples of well developed PPR have been observed in simple craters as well, and most PPR have shapes that fit back into the depletion zone which once held them. Impact Crater Tooting: The Tooting Impact crater is located at 23.4oN, 207.5°E (Figure 1). MouginisMark and Garbiel determined the age of Tooting to be between 0.4 and 1.7Myr [2]. Figure 1 shows the well developed monolithic PPR in the NW portion of the crater. Tooting has recently been almost completely covered by HiRISE stereo pairs which allow for the generation of Digital Elevation Models having sub meter resolution. DEM Generation: DEM’s were generated from stereo pairs having a maximum resolution of 25cm/pixel using stereo workstations and BAE’s SOCET SET® photogrammetry software (see Acknowledgements). Using the USGS processing sequence, generated HiRISE DEM’s were controlled to the MOLA DEM and groundtracks for absolute orientation. This results in an absolute error of the DEM’s overall position in the X and Y direction of 50-100m. The absolute error in the Z direction for an entire DEM would be limited to the error in MOLA measurements, which in the case of steep topography, can be on the order of 10% of the elevation change within the 160m MOLA sample window (≈9m on a slope of 30°). [3].

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.042
Threshold uncertainty score0.084

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.000
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.001

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 head0.047
GPT teacher head0.272
Teacher spread0.226 · 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".

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Citations0
Published2010
Admission routes1
Has abstractyes

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