Files
sky-cam/test_moon_composite.py
T
Claude 9e2852fd73 Use fixed obs time for NASA fetch and atmosphere check
Previous approach: scan a 3-day window, find best moon detection,
use that timestamp.  Problems: fuzzy composite (multi-day scan could
pick a frame far from actual full moon), no clear tie between the
NASA render and a specific observable moment.

New approach — MOON_OBS_TIME_LOCAL (default 22:30 local):
  On the night of the exact phase event, look at east frames in a
  ±MOON_OBS_WINDOW_MIN (default 30 min) window around the configured
  time.  The frame closest to that time determines atmosphere opacity;
  the same time (rounded to hour) drives the NASA Dial-a-Moon fetch.
  This gives one definitive moment per phase per month.

moon_phase_monthly.py:
  - PHASE_SPEC stripped to just post_delay + enabled_key (all window/
    illumination filtering removed — obs time is the only selector)
  - run_phase() replaced with obs-time logic; opacity derived from
    detect_moon quality on that single frame
  - MOON_FULL_POST_DELAY_DAYS / MOON_QUARTER_POST_DELAY_DAYS default
    changed to 1 (post morning after the phase, frames already on disk)

moon_composite.py:
  - atmosphere blur default: output_width//10 (192px) → output_width//20
    (96px) so cloud shapes survive the blur

sky-cam.conf:
  - MOON_OBS_TIME_LOCAL=22:30, MOON_OBS_WINDOW_MIN=30
  - Post delay defaults updated to 1

test_moon_composite.py:
  - Tries real NASA SVS Dial-a-Moon API first; procedural disc only as
    fallback if API unreachable
  - Runs detect_moon on the east frame to compute real opacity
  - Single output (test_composite_out.jpg)

https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
2026-05-01 22:03:57 +00:00

163 lines
5.6 KiB
Python

#!/usr/bin/env python3
"""test_moon_composite.py — render a phase composite using real NASA data.
Simulates what moon_phase_monthly.py does on the night of a full moon:
1. Round the obs time (22:30 local on 2026-04-29) to the nearest hour.
2. Fetch the NASA SVS Dial-a-Moon render for that UTC hour.
3. Load the east camera frame (21-07-00.jpg, captured at 21:07 UTC that night).
4. Detect atmospheric conditions → compute overlay opacity.
5. Render: NASA moon + east atmosphere overlay → test_composite_out.jpg.
Run from the sky-cam directory:
python3 test_moon_composite.py
Requires internet access to reach svs.gsfc.nasa.gov.
If the API is unreachable a procedural moon disc is used as a fallback
so the atmospheric overlay is still visible and testable.
"""
import os
import pathlib
import sys
import tempfile
from datetime import datetime, timezone
HERE = pathlib.Path(__file__).resolve().parent
sys.path.insert(0, str(HERE))
EAST_FRAME = HERE / '21-07-00.jpg'
OUT_PATH = HERE / 'test_composite_out.jpg'
# The east frame is 2026-04-29 21:07 UTC; obs time is 22:30 local → ~21:30 UTC
# (assuming Eastern time UTC-4 in late April). Round to nearest hour → 22:00 UTC.
NASA_FETCH_UTC = datetime(2026, 4, 29, 22, 0, tzinfo=timezone.utc)
def _fetch_nasa(dt: datetime) -> 'pathlib.Path | None':
try:
import moon_dialamoon
print(f'fetching NASA Dial-a-Moon for {dt.strftime("%Y-%m-%dT%H:00Z")} …')
path = moon_dialamoon.fetch_for_time(dt)
print(f' cached at {path}')
return path
except Exception as e:
print(f' NASA fetch failed: {e}')
return None
def _make_procedural_moon(size: int = 2048) -> 'pathlib.Path':
"""Fallback: clean grey disc with maria and limb darkening."""
from PIL import Image, ImageDraw, ImageFilter
import numpy as np
img = Image.new('RGB', (size, size), (0, 0, 0))
draw = ImageDraw.Draw(img)
cx = cy = size // 2
r = int(size * 0.47)
draw.ellipse([cx - r, cy - r, cx + r, cy + r], fill=(218, 214, 200))
draw.ellipse([cx - r//3, cy - r//3, cx + r//6, cy + r//5], fill=(170, 167, 154))
draw.ellipse([cx + r//8, cy - r//5, cx + r//3, cy + r//8], fill=(182, 179, 166))
draw.ellipse([cx - r//4, cy + r//6, cx + r//8, cy + r//3], fill=(175, 172, 159))
draw.ellipse([cx - r//2, cy - r//10, cx - r//5, cy + r//4], fill=(185, 182, 169))
img = img.filter(ImageFilter.GaussianBlur(radius=size // 80))
vignette = Image.new('L', (size, size), 0)
vd = ImageDraw.Draw(vignette)
vd.ellipse([cx - r, cy - r, cx + r, cy + r], fill=255)
vignette = vignette.filter(ImageFilter.GaussianBlur(radius=size // 30))
arr = np.asarray(img).astype(float)
vig = np.asarray(vignette).astype(float) / 255.0
arr = np.clip(arr * (0.75 + 0.25 * vig)[..., None], 0, 255).astype('uint8')
img = Image.fromarray(arr)
tmp = tempfile.NamedTemporaryFile(suffix='.png', delete=False)
tmp.close()
img.save(tmp.name)
return pathlib.Path(tmp.name)
def _detect_atmosphere(frame_path: str) -> tuple[float | None, float]:
"""Run moon_detect and return (quality, opacity)."""
try:
from moon_detect import detect_moon
from moon_phase_monthly import _atmosphere_opacity_from_quality
det = detect_moon(frame_path)
quality = det.quality if det is not None else None
opacity = _atmosphere_opacity_from_quality(quality)
return quality, opacity
except Exception as e:
print(f' detection failed: {e}')
return None, 0.0
def main():
if not EAST_FRAME.exists():
print(f'ERROR: missing {EAST_FRAME}', file=sys.stderr)
sys.exit(1)
print('=== moon composite test ===')
print(f'east frame : {EAST_FRAME.name} (2026-04-29 21:07 UTC)')
print(f'NASA time : {NASA_FETCH_UTC.strftime("%Y-%m-%dT%H:00Z")}')
print()
# 1. Try real NASA image
tmp_to_delete = None
nasa_path = _fetch_nasa(NASA_FETCH_UTC)
if nasa_path is None:
print('falling back to procedural moon disc …')
nasa_path = _make_procedural_moon()
tmp_to_delete = str(nasa_path)
print(f' disc saved to {nasa_path}')
print()
# 2. Atmosphere from east frame
print(f'checking atmosphere in {EAST_FRAME.name} …')
quality, opacity = _detect_atmosphere(str(EAST_FRAME))
if quality is not None:
print(f' moon quality: {quality:.3f} → atmosphere opacity: {opacity:.2f}')
else:
print(f' no moon detected (overcast) → opacity: {opacity:.2f}')
print()
# 3. Render
from moon_composite import render_phase_closeup
caption = (
f'Full Moon — April 2026 — '
f'sky-cam east 2026-04-29 22:30 local — '
f'NASA SVS Dial-a-Moon'
)
print(f'rendering {OUT_PATH.name} …')
try:
render_phase_closeup(
nasa_render_path=str(nasa_path),
out_path=str(OUT_PATH),
output_size=(1920, 1080),
moon_height_pct=0.88,
caption=caption,
east_frame_path=str(EAST_FRAME),
atmosphere_opacity=opacity,
atmosphere_blur=0,
)
finally:
if tmp_to_delete:
os.unlink(tmp_to_delete)
print(f'done → {OUT_PATH}')
print()
print(f'opacity={opacity:.2f}:', end=' ')
if opacity == 0.0:
print('clear sky — pure NASA moon on black background')
elif opacity < 0.15:
print('slight haze — moon visible, softly veiled')
elif opacity < 0.40:
print('cloud cover — moon partially obscured')
else:
print('heavy overcast — moon a glow through cloud')
if __name__ == '__main__':
main()