1.9 KiB
1.9 KiB
Phase 0 Sample Stack Selection
Updated: 2026-04-03
Selected baseline sample
Current baseline sample stack:
- group key:
LT1A|STRIP1|HH|DESCENDING|E123.3_N46.1
- manifest:
experiments/isce2_sbas_timeseries/configs/sample_stack_e123p3_n46p1.json
Sample summary
- satellite:
LT1A
- mode:
STRIP1
- polarization:
HH
- orbit direction:
DESCENDING
- scene count:
5
- dates:
2025011820250315202505102025070520250830
- recommended reference date:
20250510
- receiving stations observed:
SYCKSC
Why this sample is useful
- It already satisfies a minimal SBAS smoke-test stack size.
- All scenes share the same:
- satellite
- imaging mode
- polarization
- orbit direction
- tile key
- The dates are evenly spaced enough to act as a first time-series experiment set.
Important adjacent-tile signal
This sample is not isolated.
The same date sequence also appears in multiple neighboring descending tiles, including:
E123.5_N46.6E123.6_N47.0E123.8_N47.5E123.9_N48.0E124.5_N49.9E124.7_N50.3E124.8_N50.8E125.0_N51.3E125.1_N51.8E125.3_N52.2E125.5_N52.7
These neighboring tiles share the same 5 acquisition dates:
2025011820250315202505102025070520250830
Implication
This strongly suggests the data pool contains a larger repeated strip-family, not just isolated scenes.
Recommended experiment order:
- Start with one tile-level stack smoke test using
E123.3_N46.1. - If stack-prep works, expand to multiple adjacent tiles with the same date family.
- Only after that, test a wider strip or mosaic strategy.
Current risk judgment
The main remaining uncertainty is still not scene selection.
The main uncertainty is:
- how to convert LT-1 per-scene
tiff + meta.xmlfolders - into a stack layout and sensor input form acceptable to the ISCE2 stripmap stack workflow