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
This commit is contained in:
Claude
+4
-3
@@ -253,12 +253,13 @@ def _make_atmosphere_layer(
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it reads as "clouds between the observer and the moon" — which is
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physically correct.
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blur_radius=0 → auto: output_width // 10, which smooths pixel-level
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detail but keeps cloud-scale gradients visible.
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blur_radius=0 → auto: output_width // 20 (96 px at 1920 wide).
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This smooths pixel-level RTSP noise and OSD text while keeping
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recognisable cloud shapes and sky-colour gradients intact.
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"""
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src = Image.open(east_frame_path).convert('RGB')
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layer = src.resize(output_size, LANCZOS)
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r = blur_radius if blur_radius > 0 else output_size[0] // 10
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r = blur_radius if blur_radius > 0 else output_size[0] // 20
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return layer.filter(ImageFilter.GaussianBlur(radius=r))
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+75
-98
@@ -88,6 +88,11 @@ REQUIRE_EAST_VERIFY = CONF.get('MOON_REQUIRE_EAST_VERIFY', 'true').lower() != 'f
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ATMOSPHERE_BLUR = int(CONF.get('MOON_ATMOSPHERE_BLUR', 0))
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CLOUDY_POST_ENABLED = CONF.get('MOON_CLOUDY_POST_ENABLED', 'true').lower() != 'false'
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_obs_parts = CONF.get('MOON_OBS_TIME_LOCAL', '22:30').split(':')
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OBS_TIME_H = int(_obs_parts[0])
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OBS_TIME_M = int(_obs_parts[1]) if len(_obs_parts) > 1 else 0
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OBS_WINDOW_MIN = int(CONF.get('MOON_OBS_WINDOW_MIN', 30))
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def _atmosphere_opacity_from_quality(quality: float | None) -> float:
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"""Map moon detection quality to atmospheric overlay opacity.
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@@ -115,39 +120,21 @@ PHASE_SPEC = {
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'index': 2,
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'label': 'Full Moon',
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'emoji': '🌕',
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# ±4% of target (100%): accept 96–100% illumination
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'illum_min': float(CONF.get('MOON_FULL_MIN_ILLUMINATION', 0.96)),
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'illum_max': 1.01,
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'waxing': None,
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'window_before': int(CONF.get('MOON_FULL_WINDOW_BEFORE_DAYS', 1)),
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'window_after': int(CONF.get('MOON_FULL_WINDOW_AFTER_DAYS', 2)),
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'post_delay': int(CONF.get('MOON_FULL_POST_DELAY_DAYS', 3)),
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'post_delay': int(CONF.get('MOON_FULL_POST_DELAY_DAYS', 1)),
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'enabled_key': 'MOON_FULL_ENABLED',
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},
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'first-quarter': {
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'index': 1,
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'label': 'First Quarter (Waxing Half)',
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'emoji': '🌓',
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# ±4% of target (50%): accept 46–54% illumination, waxing only
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'illum_min': float(CONF.get('MOON_QUARTER_MIN_ILLUMINATION', 0.46)),
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'illum_max': float(CONF.get('MOON_QUARTER_MAX_ILLUMINATION', 0.54)),
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'waxing': True,
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'window_before': int(CONF.get('MOON_QUARTER_WINDOW_BEFORE_DAYS', 1)),
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'window_after': int(CONF.get('MOON_QUARTER_WINDOW_AFTER_DAYS', 1)),
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'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 2)),
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'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 1)),
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'enabled_key': 'MOON_FIRST_QUARTER_ENABLED',
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},
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'third-quarter': {
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'index': 3,
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'label': 'Third Quarter (Waning Half)',
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'emoji': '🌗',
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# ±4% of target (50%): accept 46–54% illumination, waning only
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'illum_min': float(CONF.get('MOON_QUARTER_MIN_ILLUMINATION', 0.46)),
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'illum_max': float(CONF.get('MOON_QUARTER_MAX_ILLUMINATION', 0.54)),
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'waxing': False,
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'window_before': int(CONF.get('MOON_QUARTER_WINDOW_BEFORE_DAYS', 1)),
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'window_after': int(CONF.get('MOON_QUARTER_WINDOW_AFTER_DAYS', 1)),
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'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 2)),
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'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 1)),
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'enabled_key': 'MOON_THIRD_QUARTER_ENABLED',
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},
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}
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@@ -280,99 +267,89 @@ def run_phase(phase: str, target_utc: datetime | None, cam: str,
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cam, dry_run, no_upload, out_path,
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witness_text='not requiring east verification (set MOON_REQUIRE_EAST_VERIFY=true to require)')
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dates = []
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for i in range(-spec['window_before'], spec['window_after'] + 1):
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d = (target_local + timedelta(days=i)).date()
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dates.append(d.strftime('%Y-%m-%d'))
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print(f'scanning dates: {dates}')
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candidates = _candidate_frames(cam, dates)
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print(f'frame count in window: {len(candidates)}')
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if not candidates:
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msg = (
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f'No frames for {cam} in window {dates[0]}..{dates[-1]} '
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f'around {phase} {target_utc.strftime("%Y-%m-%d %H:%MZ")}.'
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# ── Fixed observation time on the night of the phase event ──────────────
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# Instead of scanning a multi-day window for the best detection, we look
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# at a short window around a configured local time (default 22:30) on the
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# night of the exact phase. That single timestamp drives both the NASA
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# Dial-a-Moon fetch (rounded to the nearest hour) and the atmosphere check.
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obs_naive = datetime(
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target_local.year, target_local.month, target_local.day,
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OBS_TIME_H, OBS_TIME_M, 0,
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)
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_notify(f'{spec["emoji"]} {spec["label"]} — no frames available', msg)
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print(msg)
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return 0
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if hasattr(tz, 'localize'):
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obs_utc = tz.localize(obs_naive).astimezone(timezone.utc)
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else:
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obs_utc = obs_naive.replace(tzinfo=tz).astimezone(timezone.utc)
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print(f'obs time: {obs_utc.isoformat()} ({_format_local(obs_utc)})')
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qualifying = []
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above_horizon = [] # frames where moon is up but quality/illum check failed
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for path, utc_dt in candidates:
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# Check moon altitude at the observation time
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try:
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alt, _ = moon_phase.altaz(utc_dt)
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alt_at_obs, _ = moon_phase.altaz(obs_utc)
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except Exception as e:
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print(f'ERROR: moon_phase.altaz failed: {e}', file=sys.stderr)
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print(f'ERROR: moon_phase.altaz: {e}', file=sys.stderr)
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return 2
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if alt < MIN_ALTITUDE:
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continue
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det = detect_moon(path)
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if det is None or det.quality < MIN_QUALITY:
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above_horizon.append((path, utc_dt, det))
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continue
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illum = moon_phase.illumination(utc_dt)
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if illum < spec['illum_min'] or illum > spec['illum_max']:
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continue
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if spec['waxing'] is not None:
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if moon_phase.waxing(utc_dt) != spec['waxing']:
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continue
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qualifying.append((path, utc_dt, det, alt, illum))
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print(f'moon altitude at obs time: {alt_at_obs:.1f}°')
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print(f'qualifying frames: {len(qualifying)} above-horizon fallback pool: {len(above_horizon)}')
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# Gather east frames in the ±OBS_WINDOW_MIN window
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obs_start = obs_utc - timedelta(minutes=OBS_WINDOW_MIN)
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obs_end = obs_utc + timedelta(minutes=OBS_WINDOW_MIN)
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obs_dates: list[str] = []
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d = obs_start.astimezone(tz).date()
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while d <= obs_end.astimezone(tz).date():
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obs_dates.append(d.strftime('%Y-%m-%d'))
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d += timedelta(days=1)
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all_frames = _candidate_frames(cam, obs_dates)
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window_frames = [(p, dt) for p, dt in all_frames if obs_start <= dt <= obs_end]
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print(f'east frames in ±{OBS_WINDOW_MIN} min window: {len(window_frames)}')
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if not qualifying:
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# No frame met quality + illumination thresholds — likely overcast.
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# If MOON_CLOUDY_POST_ENABLED, use the above-horizon frame closest to
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# the exact phase moment as the atmosphere source and post with a
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# heavy cloud overlay so the month is still represented.
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if above_horizon and CLOUDY_POST_ENABLED:
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best_cloudy = min(above_horizon, key=lambda t: abs(t[1] - target_utc))
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path, _when, det = best_cloudy
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# Determine atmosphere opacity from the frame closest to obs_utc
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east_frame: str | None = None
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opacity = 0.0
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if alt_at_obs < MIN_ALTITUDE:
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print('moon below horizon at obs time — posting clean NASA image')
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_notify(
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f'{spec["emoji"]} {spec["label"]} {target_utc.strftime("%B %Y")} '
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f'— moon below horizon at {OBS_TIME_H:02d}:{OBS_TIME_M:02d} local',
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f'Adjust MOON_OBS_TIME_LOCAL in sky-cam.conf. Posting clean NASA render.',
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)
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elif window_frames:
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best_f = min(window_frames, key=lambda t: abs(t[1] - obs_utc))
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east_frame, best_dt = best_f
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det = detect_moon(east_frame)
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quality = det.quality if det is not None else None
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opacity = _atmosphere_opacity_from_quality(quality)
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print(f'overcast fallback: {path} quality={quality} opacity={opacity:.2f}')
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witness = f'cloud cover — {target_utc.strftime("%Y-%m-%d")} — NASA SVS Dial-a-Moon'
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if dry_run:
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return 0
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return _render_and_post(
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phase, spec, target_utc, target_utc,
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target_utc.astimezone(tz),
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cam, dry_run, no_upload, out_path,
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witness_text=witness,
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east_frame_path=path,
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atmosphere_opacity=opacity,
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offset_min = (best_dt - obs_utc).total_seconds() / 60.0
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print(f'atmosphere frame: {east_frame}')
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print(f' quality={quality} opacity={opacity:.2f} '
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f'offset={offset_min:+.1f} min from obs time')
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else:
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print('no east frames in obs window — posting clean NASA image')
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# Label atmospheric conditions for the caption
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if opacity == 0.0:
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atm_label = 'clear sky'
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elif opacity < 0.15:
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atm_label = 'slight haze'
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elif opacity < 0.40:
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atm_label = 'cloud cover'
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else:
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atm_label = 'heavy overcast'
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obs_local_str = _format_local(obs_utc)
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witness_text = (
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f'sky-cam {cam} — {atm_label} at {obs_local_str} — NASA SVS Dial-a-Moon'
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)
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msg = (
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f'No {phase} frame in window {dates[0]}..{dates[-1]} '
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f'(quality≥{MIN_QUALITY}, altitude≥{MIN_ALTITUDE}°, '
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f'illumination {spec["illum_min"]:.2f}-{spec["illum_max"]:.2f}) '
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f'and no above-horizon frames for cloudy fallback.'
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)
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_notify(f'{spec["emoji"]} {spec["label"]} — skipped {target_utc.strftime("%B %Y")}', msg)
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print(msg)
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return 0
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best = min(qualifying, key=lambda t: abs(t[1] - target_utc))
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path, when_utc, det, alt, illum = best
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local_dt = when_utc.astimezone(tz)
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delta_min = (when_utc - target_utc).total_seconds() / 60.0
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opacity = _atmosphere_opacity_from_quality(det.quality)
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print(f'picked: {path}')
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print(f' when_utc={when_utc.isoformat()} local={local_dt} '
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f'altitude={alt:.1f} illum={illum:.4f} quality={det.quality:.3f} '
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f'opacity={opacity:.2f} delta={delta_min:+.1f} min')
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if dry_run:
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print(f'dry-run: would post with opacity={opacity:.2f} ({atm_label})')
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return 0
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return _render_and_post(
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phase, spec, target_utc, when_utc, local_dt,
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phase, spec, target_utc, obs_utc, obs_utc.astimezone(tz),
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cam, dry_run, no_upload, out_path,
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witness_text=f'witnessed at {local_dt.strftime("%Y-%m-%d %H:%M:%S %Z")} '
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f'({delta_min:+.0f} min from exact {phase})',
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east_frame_path=path,
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witness_text=witness_text,
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east_frame_path=east_frame,
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atmosphere_opacity=opacity,
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)
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+21
-8
@@ -491,15 +491,28 @@ MOON_TRACK_FPS=12 # output mp4 framerate
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MOON_TRACK_CRF=24 # output mp4 CRF
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MOON_TRACK_RETENTION_DAYS=90 # delete tracker mp4s older than this; 0 = forever
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# Full-moon monthly tuning ────────────────────────────────────────────────────
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# How many days after the exact full moon to post. 3 = waits for D-1..D+2
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# nights to be on disk, then runs the morning of D+3.
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MOON_FULL_POST_DELAY_DAYS=3
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# Observation time ────────────────────────────────────────────────────────────
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# Local time used to select the east camera frame and the NASA Dial-a-Moon
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# render for each phase post. The script looks at east frames within
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# ±MOON_OBS_WINDOW_MIN of this time on the night of the exact phase event,
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# picks the one closest to the target time, and uses it to:
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# 1. Determine atmospheric conditions (clear / hazy / overcast)
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# 2. Set the atmosphere overlay opacity on the NASA moon image
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# 3. Round to the nearest hour for the NASA API call
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#
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# 22:30 works well for full moon and first quarter (both visible after dark).
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# For third quarter (rises after midnight), consider 02:30 or leave at 22:30
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# and accept that the moon may be below the horizon — the script will warn
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# and post a clean NASA render instead.
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MOON_OBS_TIME_LOCAL=22:30
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MOON_OBS_WINDOW_MIN=30 # ±minutes around obs time to check east frames
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# Quarter (half-moon) tuning ──────────────────────────────────────────────────
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# 2 = waits for D-1, D, D+1 nights, runs the morning of D+2.
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MOON_QUARTER_POST_DELAY_DAYS=2
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MOON_QUARTER_MIN_ILLUMINATION=0.46 # ±4% of 50%: waxing/waning within 4% of exact quarter
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# Post delay ──────────────────────────────────────────────────────────────────
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# How many days after the exact phase to run the post. The post delay gives
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# time for the obs-night frames to land on disk before the job runs.
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MOON_FULL_POST_DELAY_DAYS=1 # post the morning after the full moon
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MOON_QUARTER_POST_DELAY_DAYS=1 # post the morning after each quarter
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MOON_QUARTER_MIN_ILLUMINATION=0.46
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MOON_QUARTER_MAX_ILLUMINATION=0.54
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# Frame-acceptance thresholds — a candidate must beat all three to qualify.
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+92
-45
@@ -1,41 +1,54 @@
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#!/usr/bin/env python3
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"""test_moon_composite.py — smoke-test atmospheric overlay at three opacity levels.
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"""test_moon_composite.py — render a phase composite using real NASA data.
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Generates three output images from the same east camera frame (21-07-00.jpg)
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to show how the atmospheric overlay looks across the quality spectrum:
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Simulates what moon_phase_monthly.py does on the night of a full moon:
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test_composite_clear.jpg — opacity 0.00 (quality ≥ 0.85, clear sky)
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test_composite_hazy.jpg — opacity 0.20 (quality ~ 0.70, light haze)
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test_composite_cloudy.jpg — opacity 0.65 (overcast fallback)
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The moon disk in each image is procedurally generated (clean grey sphere,
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no camera timestamp). In production it is replaced by the NASA SVS
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Dial-a-Moon render for the exact UTC hour east captured the moon.
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1. Round the obs time (22:30 local on 2026-04-29) to the nearest hour.
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2. Fetch the NASA SVS Dial-a-Moon render for that UTC hour.
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3. Load the east camera frame (21-07-00.jpg, captured at 21:07 UTC that night).
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4. Detect atmospheric conditions → compute overlay opacity.
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5. Render: NASA moon + east atmosphere overlay → test_composite_out.jpg.
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Run from the sky-cam directory:
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python3 test_moon_composite.py
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Requires internet access to reach svs.gsfc.nasa.gov.
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If the API is unreachable a procedural moon disc is used as a fallback
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so the atmospheric overlay is still visible and testable.
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"""
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import os
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import pathlib
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import sys
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import tempfile
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from datetime import datetime, timezone
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HERE = pathlib.Path(__file__).resolve().parent
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sys.path.insert(0, str(HERE))
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EAST_FRAME = HERE / '21-07-00.jpg'
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OUT_PATH = HERE / 'test_composite_out.jpg'
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CASES = [
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('test_composite_clear.jpg', 0.00, 'clear sky (quality >= 0.85)'),
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('test_composite_hazy.jpg', 0.20, 'light haze (quality ~ 0.70)'),
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('test_composite_cloudy.jpg', 0.65, 'heavy overcast fallback'),
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]
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# The east frame is 2026-04-29 21:07 UTC; obs time is 22:30 local → ~21:30 UTC
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# (assuming Eastern time UTC-4 in late April). Round to nearest hour → 22:00 UTC.
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NASA_FETCH_UTC = datetime(2026, 4, 29, 22, 0, tzinfo=timezone.utc)
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def _make_procedural_moon(size: int = 2048) -> 'Image':
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"""Clean grey disc with simplified lunar maria and limb darkening."""
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def _fetch_nasa(dt: datetime) -> 'pathlib.Path | None':
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try:
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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
|
||||
|
||||
@@ -58,7 +71,26 @@ def _make_procedural_moon(size: int = 2048) -> 'Image':
|
||||
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')
|
||||
return Image.fromarray(arr)
|
||||
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():
|
||||
@@ -66,27 +98,42 @@ def main():
|
||||
print(f'ERROR: missing {EAST_FRAME}', file=sys.stderr)
|
||||
sys.exit(1)
|
||||
|
||||
print('generating procedural moon disc …')
|
||||
moon_img = _make_procedural_moon(2048)
|
||||
tmp = tempfile.NamedTemporaryFile(suffix='.png', delete=False)
|
||||
tmp_moon = tmp.name
|
||||
tmp.close()
|
||||
moon_img.save(tmp_moon)
|
||||
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
|
||||
|
||||
try:
|
||||
for filename, opacity, label in CASES:
|
||||
out = HERE / filename
|
||||
caption = (
|
||||
f'Full Moon — April 2026 — '
|
||||
f'sky-cam east 2026-04-29 21:07 UTC — '
|
||||
f'NASA SVS Dial-a-Moon [{label}]'
|
||||
f'sky-cam east 2026-04-29 22:30 local — '
|
||||
f'NASA SVS Dial-a-Moon'
|
||||
)
|
||||
print(f'rendering {filename} (opacity={opacity:.2f}) {label} …')
|
||||
print(f'rendering {OUT_PATH.name} …')
|
||||
try:
|
||||
render_phase_closeup(
|
||||
nasa_render_path=tmp_moon,
|
||||
out_path=str(out),
|
||||
nasa_render_path=str(nasa_path),
|
||||
out_path=str(OUT_PATH),
|
||||
output_size=(1920, 1080),
|
||||
moon_height_pct=0.88,
|
||||
caption=caption,
|
||||
@@ -94,21 +141,21 @@ def main():
|
||||
atmosphere_opacity=opacity,
|
||||
atmosphere_blur=0,
|
||||
)
|
||||
print(f' -> {out}')
|
||||
finally:
|
||||
os.unlink(tmp_moon)
|
||||
if tmp_to_delete:
|
||||
os.unlink(tmp_to_delete)
|
||||
|
||||
print(f'done → {OUT_PATH}')
|
||||
print()
|
||||
print('done. Three outputs:')
|
||||
for filename, opacity, label in CASES:
|
||||
print(f' {filename:35s} opacity={opacity:.2f} {label}')
|
||||
print()
|
||||
print('What you should see in each:')
|
||||
print(' clear — NASA moon disk sharp and unobscured on black background')
|
||||
print(' hazy — same moon but with a soft grey-blue veil over the disk')
|
||||
print(' (from the thin cloud visible in 21-07-00.jpg)')
|
||||
print(' cloudy — moon mostly hidden; visible as a bright glow through')
|
||||
print(' the cloud texture from east\'s April 29 frame')
|
||||
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__':
|
||||
|
||||
Reference in New Issue
Block a user