New Analysis — LunaScope

Workspace

New Lunar Analysis

Assemble 2 to 5 lunar observations. LunaScope selects the correspondence pipeline automatically — no algorithm configuration is required.

Datasets for correspondence analysis

Each input is one observation of the same region, captured by any supported instrument.

0 of 2 loaded · max 5

IMAGE 01

Sensor

Orbiter High Resolution Camera — 0.25 m/px panchromatic

Drop raster here or browse

GeoTIFF, PNG, JPEG, ISRO .img · up to 512 MB

Image name: Awaiting dataset metadata
Instrument: OHRC
Dataset type: Awaiting dataset metadata
Processing status: Awaiting dataset metadata

Acquisition metadata (optional — improves matching)

AcquiredGSDLatitudeLongitudeSun azimuthSun elevation

IMAGE 02

Sensor

Terrain Mapping Camera 2 — 5 m/px stereo

Drop raster here or browse

GeoTIFF, PNG, JPEG, ISRO .img · up to 512 MB

Image name: Awaiting dataset metadata
Instrument: TMC-2
Dataset type: Awaiting dataset metadata
Processing status: Awaiting dataset metadata

Acquisition metadata (optional — improves matching)

AcquiredGSDLatitudeLongitudeSun azimuthSun elevation

Analysis settings

Parameters forwarded verbatim to the correspondence engine.

Correspondence Engine

Automatic

LunaScope automatically selects and combines the available correspondence methods based on image characteristics, sensor combination, and processing requirements.

Pipeline optionsScale normalizationResample to a common ground-sample distance (0.25 m/px ↔ 80 m/px).Illumination normalizationCompensate Sun-angle / shadow differences between observations.Geometric verificationRANSAC inlier selection against the estimated transform.Sub-pixel refinementRefine correspondence locations below one pixel. Slower.

Correspondence engine

Automatic. The image set, instrument assignments, acquisition metadata and pipeline options are forwarded to the engine, which chooses the correspondence strategy.