pray-calc-ml/research/fayum-egypt-2022.md
Aric Camarata ada08e7ec4 data: expand dataset from 5.9k to 91k records via 6 new SQM sources
Add 6 new data collection pipelines and their processed outputs:

Sources added:
- TESS/Stars4All photometer network: 37 months (Jun 2017-Aug 2020),
  ~40k raw events from 100+ European stations via Zenodo archives
- Globe at Night citizen science: 26k twilight observations (2006-2024),
  filtered from 308k total observations for solar depression 6-22 deg
- GaN-MN continuous monitoring: 45 months (Jan 2022-Sep 2025),
  ~12.5k twilight events from 88 stations across 20+ countries
- Galicia SQM network: 14 stations, 1-min resolution, 7.5k events
- Madrid/Majadahonda SQM: multi-year continuous monitoring, 3.1k events
- washetdonker.nl Netherlands: 7 stations, 3.3k morning events
- Academic papers: Jordan (Abed 2015), Fayum Egypt, India photometer

Pipeline changes:
- ingest.py: add all new files to APPROVED_RAW_CSVS allowlist,
  fix filter to use allowlist instead of hardcoded exclusions
- .gitignore: exclude bulk raw data directories (BSRN, TESS, GaN-MN,
  washetdonker, Globe at Night downloads)

Final dataset: 56,668 Fajr + 34,763 Isha = 91,431 total records
Previous: 5,871 Fajr + 46 Isha = 5,917 total records
2026-03-22 16:39:29 -04:00

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Markdown

# Determination of the True Dawn by Several Different Ways at Fayum in Egypt
**Authors:** M.G. Rashed, Yasser A. Abdel-Hadi, M.S. El-Nawawy, M.Y. Amin, U.A. Rahoma, M.A. Semeida, A. Abul-Wafa, G.A. Goma, M. Sedek, M.M. Hussien, A.A. Elminawy, M.A. Shahat, A.H. Ibrahim, A.R. Mouner, A.H. Hassan, and Hussein M. Farid
**Year:** 2022
**Journal:** International Journal of Mechanical Engineering and Technology (IJMET), 13(10): 8-24
**DOI:** https://doi.org/10.17605/OSF.IO/9K3MJ
**URL:** https://iaeme.com/Home/article_id/IJMET_13_10_002
**Sites studied:** Wadi al Hitan, Fayum, Egypt (29 17'N, 30 03'E, 50m elevation)
**Observation method:** SQM (LU-DL, Unihedron) in horizontal (H) and zenith (Z) directions, plus naked eye by groups of 9+ astronomers
**Date range:** December 9-11, 2018 (Group 1) and December 19, 2019 (Group 2)
**Records:** 4 nights of SQM data, 2 separate naked-eye group observations
**Mean angle (Fajr):** D0 = 14.0 to 14.8 depending on method
## Location Details
- Wadi al Hitan, Fayum desert, Egypt
- 29 17'N, 30 03'E, 50m elevation
- Desert area far from urban light pollution
- Chosen specifically for astronomical observation quality
## Summary
A multi-method study combining SQM photometry and naked-eye observations over 4 nights at Fayum desert. The paper applies four different criteria to determine true dawn:
1. Eye threshold method (0.83 mag from full night): D0 = 14.7 degrees
2. Naked eye group observation (9+ trained observers, tayakkun): D0 = 14.8 degrees
3. Kocifaj relation H = pi*Z: D0 = 14.0 degrees
4. Luminance threshold 0.015 cd/m2 (mesopic region): D0 = 13.75 degrees (clear), 10 degrees (cloudy)
Key SQM findings:
- Full night illuminance: 18.76 mag (east direction), 16.92 mag (zenith) for clear nights
- Full night illuminance: 22 mag for cloudy night
- The H/Z ratio equals pi at D0 = 14 degrees (Kocifaj criterion)
- Clear vs cloudy comparison shows clouds delay apparent dawn by ~4 degrees
Table 4 provides SQM readings at D0 = 6, 12, 14, 14.8, 18 degrees for Dec 19, 2019 in both east and zenith directions. This is valuable calibration data.
Clouds absorb 19% of the night sky energy during full night and 2.5% during twilight.
## Data Availability
**LIMITED PER-NIGHT DATA.** The paper presents:
- SQM curves as figures for 4 nights (Dec 9, 10, 11 2018 + Dec 19 2019)
- Table 4: SQM readings at specific D0 values for Dec 19, 2019
- Tables 2-3: Statistical values of twilight luminance energy per degree for Dec 10-11, 2018
- No per-minute time series data published
The SQM curves in the figures could be digitized to extract approximate readings at specific D0 values, but the paper does not provide raw time-stamped SQM data.
For ML training, the useful data points are:
- Dec 9, 2018: clear night, SQM threshold at D0 = 14.6 degrees
- Dec 10, 2018: clear night, mesopic threshold at D0 = 13.75 degrees
- Dec 11, 2018: cloudy night, threshold at D0 = 10 degrees (excluded from ML, clouds)
- Dec 19, 2019: clear night, D0 = 14.0 (H=piZ method), D0 = 14.8 (naked eye group)
## Comprehensive Literature Table
Table 1 (page 12) provides an excellent summary of all published twilight studies chronologically from 1909 to 2022, covering Egypt, Libya, Saudi Arabia, Yemen, Indonesia, and Malaysia. This is a useful cross-reference for the aggregate D0 database.
## For ML Training
Can extract 4 data points (one per clear night) with SQM-derived D0 values. The naked-eye group observation on Dec 19, 2019 gives D0 = 14.8 degrees. Only useful as aggregate/representative data since exact dawn times are not given (only D0 values derived from SQM threshold analysis).