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Record W155729965

Formation of Interdigitate Patterns on Martian Alluvial Fans

2007· article· en· W155729965 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

Bibliographic record

VenueLPI · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversity of Calgary
Fundersnot available
KeywordsAlluvial fanGeologyMars Exploration ProgramMartianGeomorphologyImpact craterDebris flowAlluviumAlluvial plainDebrisPaleontologySedimentary rockAstrobiology
DOInot available

Abstract

fetched live from OpenAlex

Introduction: Alluvial fans are semi-conical accumulations of sediment that develop at the base of slopes where channelized flows decelerate and spread laterally due to a change in gradient. Flow deceleration triggers sediment deposition, gradually building up a mounded or semi-conical fan shape. Terrestrial alluvial fans are constructed by a multitude of processes that range between two end-members: (i) low-density fluidal flows (riverine flows) and (ii) high-density sediment-gravitydriven flows (debris flows). As a key component of landscape evolution modeling and natural hazard research, terrestrial alluvial fans have been widely investigated from both academic and engineering research contexts. Several recent investigations have documented alluvial fan-like deposits on Mars [1, 2]. Collectively, these studies have documented fan characteristics consistent with fluid and gravity-driven alluvial sedimentation. However, many aspects of Martian fan formation remain poorly understood including the source and amount of fluid involved in mobilizing the flows. In this study we describe interdigitate patterns of lobate deposits on Martian alluvial fans and propose that they result from high-density, sediment-laden flows (debris flows). We compare the interdigitate fans with terrestrial analogs and draw implications for Martian alluvial fan development. Interdigitate fans on Mars: Using two MOC narrow angle images (R13-02920 and E11-04033), we have identified interdigitate patterns on fans at the base of south-facing crater walls (Figs. 1 and 2). In the first image (R13-02920; Fig. 1), the crater rim is characterized by a series of closely-spaced alcoves with feeder channels that extend partway down the slope. The upper feeder channels are broader and consist of multiple gullies that merge downslope to form a single channel above the fan apex. The feeder channels are up to 250 m wide and between 400-700 m long. The boundary between the lower portion of the feeder channels and the apex of the alluvial fans is diffuse. In some cases levees extend a short distance from the feeder channels onto the proximal fan. The fan surface is comprised of an overlapping (interdigitate) pattern of lobate deposits and largely devoid of channels, suggesting that the most recent phase of fan development involved upslope aggradation and backfilling. Lobate deposits on the proximal fan are much smaller than those along the medial and distal portions. Consequently, the proximal fan has a higher density of these deposits. The size of the lobate deposits range between 2-80 m wide and between 10200 m long. The second MOC image (E11-04033; Fig. 2) shows an alcove with a fan branching out onto the crater floor. The arcuate ridges at the base of the crater (inset; Fig. 2) resemble protalus ramparts [3]. The fan has an interdigitate pattern of lobate deposits. Similar to their counterparts in Fig. 1, the lobes decrease in size towards the fan apex. The size of the lobes ranges between 4-25 m wide and 15-60 m long. Like Fig. 1, the fan surface is not dissected by channels, suggesting upslope aggradation.

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.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.533
Threshold uncertainty score0.232

Codex and Gemma teacher scores by category

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

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 head0.014
GPT teacher head0.230
Teacher spread0.217 · 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