Merge pull request #66 from outis1one/claude/add-moon-image-locations-ACdGH

Claude/add moon image locations a cd gh
This commit is contained in:
Outis
2026-05-02 08:13:39 -04:00
committed by GitHub
5 changed files with 261 additions and 302 deletions
+11 -45
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@@ -240,28 +240,6 @@ def composite_full_moon(
return out_path
def _make_atmosphere_layer(
east_frame_path: str,
output_size: tuple[int, int],
blur_radius: int = 0,
) -> Image.Image:
"""Scale the full east frame to output_size and blur to atmospheric haze.
The blur removes wide-angle camera detail (RTSP artefacts, OSD text,
pixel noise) while preserving real sky colour and large-scale cloud
structure. The resulting layer is applied OVER the NASA moon disk so
it reads as "clouds between the observer and the moon" — which is
physically correct.
blur_radius=0 → auto: output_width // 10, which smooths pixel-level
detail but keeps cloud-scale gradients visible.
"""
src = Image.open(east_frame_path).convert('RGB')
layer = src.resize(output_size, LANCZOS)
r = blur_radius if blur_radius > 0 else output_size[0] // 10
return layer.filter(ImageFilter.GaussianBlur(radius=r))
def render_phase_closeup(
nasa_render_path: str,
out_path: str,
@@ -269,28 +247,16 @@ def render_phase_closeup(
moon_height_pct: float = 0.92,
caption: str | None = None,
background: tuple[int, int, int] = (0, 0, 0),
east_frame_path: str | None = None,
atmosphere_opacity: float = 0.0,
atmosphere_blur: int = 0,
when_utc: datetime | None = None,
):
"""Full-screen close-up rendering using a NASA SVS Dial-a-Moon image.
Rendering pipeline:
1. Black background (outer space).
2. NASA moon disk — correct phase, libration, crater shadows — centred
and scaled to moon_height_pct of frame height.
3. Atmospheric layer (optional): east's camera frame, scaled to output
size and blurred, composited OVER the moon at atmosphere_opacity.
This is physically correct — clouds are between the observer and the
moon so they occlude the disk, not sit behind it.
atmosphere_opacity controls what the viewer sees through east's sky:
0.00 — perfectly clear: pure NASA render, no overlay
0.10 — slight haze: moon is sharp but slightly softened
0.35 — noticeable cloud cover: moon partially obscured
0.65 — heavy overcast: moon a faint glow through thick cloud
Renders the NASA moon disk centred on a black background, rotated by
the parallactic angle so its orientation matches what east's camera sees
from its geographic location at the given UTC time.
"""
# ── Background + NASA moon ────────────────────────────────────────────
import moon_phase
bg = Image.new('RGB', output_size, background)
moon = Image.open(nasa_render_path).convert('RGB')
moon = _square_crop_to_disk(moon)
@@ -299,6 +265,11 @@ def render_phase_closeup(
target += target % 2
moon_resized = moon.resize((target, target), LANCZOS)
# Rotate by parallactic angle so "up" on the moon matches east's sky
if when_utc is not None:
par = moon_phase.parallactic_angle(when_utc)
moon_resized = moon_resized.rotate(-par, resample=BICUBIC, expand=False)
feather = max(3, target // 240)
mask = _disk_mask(target, feather_px=feather)
@@ -306,11 +277,6 @@ def render_phase_closeup(
py = (output_size[1] - target) // 2
bg.paste(moon_resized, (px, py), mask)
# ── Atmospheric layer from east frame — applied OVER the moon ─────────
if east_frame_path and atmosphere_opacity > 0.0:
atm = _make_atmosphere_layer(east_frame_path, output_size, atmosphere_blur)
bg = Image.blend(bg, atm, alpha=atmosphere_opacity)
if caption:
draw = ImageDraw.Draw(bg)
_draw_caption(draw, caption, (22, output_size[1] - 48), output_size[0])
+33
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@@ -179,6 +179,39 @@ def altaz(when: datetime, lat: float | None = None, lon: float | None = None):
return float(alt.degrees), float(az.degrees)
def sun_events_in_range(
search_start: datetime,
search_end: datetime,
) -> list[tuple[datetime, bool]]:
"""Return every sunrise/sunset transition between search_start and search_end.
Each item is (utc_datetime, is_rise): is_rise=True for sunrise, False for sunset.
Uses skyfield's almanac — accurate to within a minute at the configured location.
"""
_lazy()
from skyfield.almanac import find_discrete, sunrise_sunset
t0 = _t(search_start)
t1 = _t(search_end)
times, values = find_discrete(t0, t1, sunrise_sunset(_eph, _observer))
return [(t.utc_datetime(), bool(v)) for t, v in zip(times, values)]
def sun_altaz(when: datetime, lat: float | None = None, lon: float | None = None):
"""Apparent altitude/azimuth of the sun in degrees as seen from (lat, lon)."""
_lazy()
from skyfield.api import wgs84
if lat is None and lon is None:
obs = _observer
else:
obs = _eph['earth'] + wgs84.latlon(
LATITUDE if lat is None else lat,
LONGITUDE if lon is None else lon,
)
t = _t(when)
alt, az, _ = obs.at(t).observe(_eph['sun']).apparent().altaz()
return float(alt.degrees), float(az.degrees)
def parallactic_angle(when: datetime, lat: float | None = None, lon: float | None = None) -> float:
"""Parallactic angle in degrees — rotates a moon image so celestial north is up.
+129 -141
View File
@@ -85,29 +85,7 @@ OUT_H = int(CONF.get('MOON_OUTPUT_H', CONF.get('MOON_FULL_OUTPUT_H', 1080)))
MOON_PCT = float(CONF.get('MOON_HEIGHT_PCT', 0.92))
REQUIRE_EAST_VERIFY = CONF.get('MOON_REQUIRE_EAST_VERIFY', 'true').lower() != 'false'
ATMOSPHERE_BLUR = int(CONF.get('MOON_ATMOSPHERE_BLUR', 0))
CLOUDY_POST_ENABLED = CONF.get('MOON_CLOUDY_POST_ENABLED', 'true').lower() != 'false'
def _atmosphere_opacity_from_quality(quality: float | None) -> float:
"""Map moon detection quality to atmospheric overlay opacity.
quality >= 0.85 → 0.00 clear sky, no overlay
quality 0.70 → 0.20 light haze
quality 0.55 → 0.40 noticeable cloud, moon still detected
quality < 0.55 → up to 0.65 (overcast fallback frames)
quality is None → 0.68 no detection at all, heavy overcast
The overlay is applied OVER the NASA moon disk, so higher opacity means
more of the disk is obscured — physically correct for clouds above us.
"""
if quality is None:
return 0.68
if quality >= 0.85:
return 0.0
# Linear: 0.0 at quality=0.85, 0.40 at quality=0.55
raw = (0.85 - quality) / 0.30 * 0.40
return min(0.65, raw)
DARK_START_MIN = int(CONF.get('MOON_DARK_START_MIN', 30))
PHASE_SPEC = {
@@ -115,39 +93,21 @@ PHASE_SPEC = {
'index': 2,
'label': 'Full Moon',
'emoji': '🌕',
# ±4% of target (100%): accept 96100% illumination
'illum_min': float(CONF.get('MOON_FULL_MIN_ILLUMINATION', 0.96)),
'illum_max': 1.01,
'waxing': None,
'window_before': int(CONF.get('MOON_FULL_WINDOW_BEFORE_DAYS', 1)),
'window_after': int(CONF.get('MOON_FULL_WINDOW_AFTER_DAYS', 2)),
'post_delay': int(CONF.get('MOON_FULL_POST_DELAY_DAYS', 3)),
'post_delay': int(CONF.get('MOON_FULL_POST_DELAY_DAYS', 1)),
'enabled_key': 'MOON_FULL_ENABLED',
},
'first-quarter': {
'index': 1,
'label': 'First Quarter (Waxing Half)',
'emoji': '🌓',
# ±4% of target (50%): accept 4654% illumination, waxing only
'illum_min': float(CONF.get('MOON_QUARTER_MIN_ILLUMINATION', 0.46)),
'illum_max': float(CONF.get('MOON_QUARTER_MAX_ILLUMINATION', 0.54)),
'waxing': True,
'window_before': int(CONF.get('MOON_QUARTER_WINDOW_BEFORE_DAYS', 1)),
'window_after': int(CONF.get('MOON_QUARTER_WINDOW_AFTER_DAYS', 1)),
'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 2)),
'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 1)),
'enabled_key': 'MOON_FIRST_QUARTER_ENABLED',
},
'third-quarter': {
'index': 3,
'label': 'Third Quarter (Waning Half)',
'emoji': '🌗',
# ±4% of target (50%): accept 4654% illumination, waning only
'illum_min': float(CONF.get('MOON_QUARTER_MIN_ILLUMINATION', 0.46)),
'illum_max': float(CONF.get('MOON_QUARTER_MAX_ILLUMINATION', 0.54)),
'waxing': False,
'window_before': int(CONF.get('MOON_QUARTER_WINDOW_BEFORE_DAYS', 1)),
'window_after': int(CONF.get('MOON_QUARTER_WINDOW_AFTER_DAYS', 1)),
'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 2)),
'post_delay': int(CONF.get('MOON_QUARTER_POST_DELAY_DAYS', 1)),
'enabled_key': 'MOON_THIRD_QUARTER_ENABLED',
},
}
@@ -247,6 +207,70 @@ def _output_filename(phase: str, target_utc: datetime) -> str:
return f"{target_utc.strftime('%Y-%m')}-{slug}.jpg"
def _dark_moon_intervals(
search_start: datetime,
search_end: datetime,
moon_phase_mod,
) -> list[tuple[datetime, datetime]]:
"""Return contiguous blocks where the sky is dark and the moon is visible.
'Dark' means after (sunset + DARK_START_MIN) and before the following
sunrise, based on actual computed sunset/sunrise times. Within each night
block we sample every 10 min and keep only the sub-intervals where the
moon is above MIN_ALTITUDE_DEG. Falls back to sampling sun altitude
directly if skyfield can't find sunrise/sunset events (e.g. polar summer).
"""
# Get actual sunset/sunrise events; widen the window a bit to catch events
# that fall right at the boundary.
events = moon_phase_mod.sun_events_in_range(
search_start - timedelta(hours=2),
search_end + timedelta(hours=2),
)
# Build night periods from real sunset/sunrise times.
night_periods: list[tuple[datetime, datetime]] = []
for i, (evt_t, is_rise) in enumerate(events):
if is_rise:
continue # only care about sunsets here
dark_start = evt_t + timedelta(minutes=DARK_START_MIN)
# The night ends at the next sunrise (or search_end if none found).
next_rise = next((t for t, r in events[i + 1:] if r), None)
dark_end = next_rise if next_rise is not None else search_end
if dark_start < dark_end:
night_periods.append((dark_start, dark_end))
# Polar fallback: no sunset/sunrise events found.
if not night_periods:
night_periods = [(search_start, search_end)]
# Within each night, sample every 10 min to find where moon is high enough.
step = timedelta(minutes=10)
intervals: list[tuple[datetime, datetime]] = []
for night_start, night_end in night_periods:
t = max(night_start, search_start)
end = min(night_end, search_end)
if t >= end:
continue
seg_start = None
while t <= end:
try:
moon_alt, _ = moon_phase_mod.altaz(t)
except Exception:
t += step
continue
ok = moon_alt >= MIN_ALTITUDE
if ok and seg_start is None:
seg_start = t
elif not ok and seg_start is not None:
intervals.append((seg_start, t))
seg_start = None
t += step
if seg_start is not None:
intervals.append((seg_start, end))
return intervals
def run_phase(phase: str, target_utc: datetime | None, cam: str,
dry_run: bool, no_upload: bool, out_path: str | None) -> int:
spec = PHASE_SPEC[phase]
@@ -269,128 +293,93 @@ def run_phase(phase: str, target_utc: datetime | None, cam: str,
print(f'target {phase}: {target_utc.isoformat()} ({_format_local(target_utc)})')
tz = _local_tz()
target_local = target_utc.astimezone(tz)
# If east-verification is disabled the user wants a post regardless of
# whether east could see the moon that night. Fetch dial-a-moon for the
# exact phase moment, render full-screen, post. Skips all east scanning.
if not REQUIRE_EAST_VERIFY:
print('MOON_REQUIRE_EAST_VERIFY=false — skipping east scan, using exact phase UTC')
return _render_and_post(phase, spec, target_utc, target_utc, target_local,
return _render_and_post(phase, spec, target_utc, target_utc,
cam, dry_run, no_upload, out_path,
witness_text='not requiring east verification (set MOON_REQUIRE_EAST_VERIFY=true to require)')
witness_text='east verification disabled')
dates = []
for i in range(-spec['window_before'], spec['window_after'] + 1):
d = (target_local + timedelta(days=i)).date()
dates.append(d.strftime('%Y-%m-%d'))
print(f'scanning dates: {dates}')
# Find every interval within ±24h of the phase moment where the sky is
# dark (sun below civil twilight) and the moon is above the horizon.
search_start = target_utc - timedelta(hours=24)
search_end = target_utc + timedelta(hours=24)
intervals = _dark_moon_intervals(search_start, search_end, moon_phase)
candidates = _candidate_frames(cam, dates)
print(f'frame count in window: {len(candidates)}')
if not candidates:
msg = (
f'No frames for {cam} in window {dates[0]}..{dates[-1]} '
f'around {phase} {target_utc.strftime("%Y-%m-%d %H:%MZ")}.'
if not intervals:
print('no dark-sky + moon window in ±24h of phase — skipping')
_notify(
f'{spec["emoji"]} {spec["label"]} {target_utc.strftime("%B %Y")} — skipped',
'No dark-sky + moon-above-horizon window found near the phase moment.',
)
_notify(f'{spec["emoji"]} {spec["label"]} — no frames available', msg)
print(msg)
return 0
qualifying = []
above_horizon = [] # frames where moon is up but quality/illum check failed
for path, utc_dt in candidates:
try:
alt, _ = moon_phase.altaz(utc_dt)
except Exception as e:
print(f'ERROR: moon_phase.altaz failed: {e}', file=sys.stderr)
return 2
if alt < MIN_ALTITUDE:
continue
det = detect_moon(path)
if det is None or det.quality < MIN_QUALITY:
above_horizon.append((path, utc_dt, det))
continue
illum = moon_phase.illumination(utc_dt)
if illum < spec['illum_min'] or illum > spec['illum_max']:
continue
if spec['waxing'] is not None:
if moon_phase.waxing(utc_dt) != spec['waxing']:
continue
qualifying.append((path, utc_dt, det, alt, illum))
total_h = sum((e - s).total_seconds() / 3600 for s, e in intervals)
print(f'dark+moon window: {len(intervals)} segment(s), {total_h:.1f}h total')
for s, e in intervals:
print(f' {_format_local(s)} -> {_format_local(e)}')
print(f'qualifying frames: {len(qualifying)} above-horizon fallback pool: {len(above_horizon)}')
# Collect east frames that fall inside those intervals
search_dates: list[str] = []
d = search_start.astimezone(tz).date()
while d <= search_end.astimezone(tz).date():
search_dates.append(d.strftime('%Y-%m-%d'))
d += timedelta(days=1)
all_frames = _candidate_frames(cam, search_dates)
dark_frames = [
(p, dt) for p, dt in all_frames
if any(s <= dt <= e for s, e in intervals)
]
print(f'east frames in dark+moon window: {len(dark_frames)}')
if not qualifying:
# No frame met quality + illumination thresholds — likely overcast.
# If MOON_CLOUDY_POST_ENABLED, use the above-horizon frame closest to
# the exact phase moment as the atmosphere source and post with a
# heavy cloud overlay so the month is still represented.
if above_horizon and CLOUDY_POST_ENABLED:
best_cloudy = min(above_horizon, key=lambda t: abs(t[1] - target_utc))
path, _when, det = best_cloudy
quality = det.quality if det is not None else None
opacity = _atmosphere_opacity_from_quality(quality)
print(f'overcast fallback: {path} quality={quality} opacity={opacity:.2f}')
witness = f'cloud cover — {target_utc.strftime("%Y-%m-%d")} — NASA SVS Dial-a-Moon'
if dry_run:
return 0
return _render_and_post(
phase, spec, target_utc, target_utc,
target_utc.astimezone(tz),
cam, dry_run, no_upload, out_path,
witness_text=witness,
east_frame_path=path,
atmosphere_opacity=opacity,
)
# Sort by proximity to exact phase moment so the first clear frame we find
# is the one temporally closest to the moon being precisely full/quarter.
dark_frames.sort(key=lambda x: abs(x[1] - target_utc))
msg = (
f'No {phase} frame in window {dates[0]}..{dates[-1]} '
f'(quality≥{MIN_QUALITY}, altitude≥{MIN_ALTITUDE}°, '
f'illumination {spec["illum_min"]:.2f}-{spec["illum_max"]:.2f}) '
f'and no above-horizon frames for cloudy fallback.'
best_frame: str | None = None
best_dt: datetime | None = None
for fpath, fdt in dark_frames:
det = detect_moon(fpath)
if det is not None and det.quality >= MIN_QUALITY:
best_frame = fpath
best_dt = fdt
offset_min = int((fdt - target_utc).total_seconds() / 60)
print(f'best frame: {pathlib.Path(fpath).name} quality={det.quality:.3f} '
f'time={_format_local(fdt)} offset={offset_min:+d} min from exact phase')
break
if best_frame is None:
checked = len(dark_frames)
print(f'no clear moon in {checked} dark-window frame(s) — skipping (overcast)')
_notify(
f'{spec["emoji"]} {spec["label"]} {target_utc.strftime("%B %Y")} — skipped',
f'No clear moon detection in {checked} frame(s) during the dark+moon window.',
)
_notify(f'{spec["emoji"]} {spec["label"]} — skipped {target_utc.strftime("%B %Y")}', msg)
print(msg)
return 0
best = min(qualifying, key=lambda t: abs(t[1] - target_utc))
path, when_utc, det, alt, illum = best
local_dt = when_utc.astimezone(tz)
delta_min = (when_utc - target_utc).total_seconds() / 60.0
opacity = _atmosphere_opacity_from_quality(det.quality)
print(f'picked: {path}')
print(f' when_utc={when_utc.isoformat()} local={local_dt} '
f'altitude={alt:.1f} illum={illum:.4f} quality={det.quality:.3f} '
f'opacity={opacity:.2f} delta={delta_min:+.1f} min')
illum_pct = round(moon_phase.illumination(best_dt) * 100)
print(f'illumination at detection: {illum_pct}%')
if dry_run:
print(f'dry-run: would post NASA image for {best_dt.isoformat()} ({illum_pct}% lit)')
return 0
return _render_and_post(
phase, spec, target_utc, when_utc, local_dt,
phase, spec, target_utc, best_dt,
cam, dry_run, no_upload, out_path,
witness_text=f'witnessed at {local_dt.strftime("%Y-%m-%d %H:%M:%S %Z")} '
f'({delta_min:+.0f} min from exact {phase})',
east_frame_path=path,
atmosphere_opacity=opacity,
witness_text=f'sky-cam {cam}{illum_pct}% lit — {_format_local(best_dt)}',
)
def _render_and_post(phase, spec, target_utc, when_utc, local_dt, cam,
dry_run, no_upload, out_path, witness_text,
east_frame_path=None, atmosphere_opacity=0.0):
def _render_and_post(phase, spec, target_utc, when_utc, cam,
dry_run, no_upload, out_path, witness_text):
if out_path is None:
out_dir = pathlib.Path(MOVIES_DIR) / cam / _output_subdir(phase)
out_dir.mkdir(parents=True, exist_ok=True)
out_path = str(out_dir / _output_filename(phase, target_utc))
# Fetch the NASA SVS Dial-a-Moon render for the hour east captured the
# moon (or the exact phase moment if east-verification is off). The
# render carries the correct phase, libration and crater shadows for
# that UTC moment — the strongest possible match for what east "saw,"
# and free of the white-blob limitation.
import moon_dialamoon
import moon_phase as _mp
try:
nasa_path = moon_dialamoon.fetch_for_time(when_utc)
except Exception as e:
@@ -403,18 +392,17 @@ def _render_and_post(phase, spec, target_utc, when_utc, local_dt, cam,
return 4
print(f'dial-a-moon: {nasa_path}')
illum_pct = round(_mp.illumination(when_utc) * 100)
from moon_composite import render_phase_closeup
caption = (
f"{spec['label']}{target_utc.strftime('%B %Y')}"
f"sky-cam {cam} {witness_text} render: NASA SVS Dial-a-Moon"
f"{spec['label']}{illum_pct}% lit — {target_utc.strftime('%B %Y')}"
f"{witness_text} — NASA SVS Dial-a-Moon"
)
render_phase_closeup(
str(nasa_path), out_path,
output_size=(OUT_W, OUT_H), moon_height_pct=MOON_PCT,
caption=caption,
east_frame_path=east_frame_path,
atmosphere_opacity=atmosphere_opacity,
atmosphere_blur=ATMOSPHERE_BLUR,
when_utc=when_utc,
)
print(f'wrote {out_path}')
+30 -35
View File
@@ -491,15 +491,37 @@ MOON_TRACK_FPS=12 # output mp4 framerate
MOON_TRACK_CRF=24 # output mp4 CRF
MOON_TRACK_RETENTION_DAYS=90 # delete tracker mp4s older than this; 0 = forever
# Full-moon monthly tuning ────────────────────────────────────────────────────
# How many days after the exact full moon to post. 3 = waits for D-1..D+2
# nights to be on disk, then runs the morning of D+3.
MOON_FULL_POST_DELAY_DAYS=3
# Dark-sky observation window ─────────────────────────────────────────────────
# The script searches ±24h around the exact phase moment using actual computed
# sunset and sunrise times for the configured location. The dark window for
# each night starts at (sunset + MOON_DARK_START_MIN) and ends at sunrise.
# Within that window, only frames where the moon is above MOON_MIN_ALTITUDE_DEG
# are considered.
#
# The east camera faces east, so the moon is visible to it from moonrise through
# roughly south — typically from dusk through midnight for a full moon.
# MOON_DARK_START_MIN=30 means the script starts looking 30 min after the sun
# sets, when the sky is dark enough for a clean moon shot but east can still
# catch the moon low on the eastern horizon.
#
# Of all qualifying frames, the one temporally closest to the exact phase moment
# is used (not the first one). This picks the frame when the moon was most
# precisely full / at quarter. Its timestamp drives the NASA Dial-a-Moon fetch
# and the parallactic angle rotation; the caption shows illumination% at that
# moment. If no clear frame is found, the month is skipped entirely.
#
# If the phase falls early in the day (e.g. 01:30 local), the ±24h window
# covers the previous evening through the following dusk — both nights where
# the moon is essentially full. If the phase falls just before midnight
# (e.g. 23:55), both the same evening and the next morning are included.
MOON_DARK_START_MIN=30
# Quarter (half-moon) tuning ──────────────────────────────────────────────────
# 2 = waits for D-1, D, D+1 nights, runs the morning of D+2.
MOON_QUARTER_POST_DELAY_DAYS=2
MOON_QUARTER_MIN_ILLUMINATION=0.46 # ±4% of 50%: waxing/waning within 4% of exact quarter
# Post delay ──────────────────────────────────────────────────────────────────
# How many days after the exact phase to run the post. The post delay gives
# time for the obs-night frames to land on disk before the job runs.
MOON_FULL_POST_DELAY_DAYS=1 # post the morning after the full moon
MOON_QUARTER_POST_DELAY_DAYS=1 # post the morning after each quarter
MOON_QUARTER_MIN_ILLUMINATION=0.46
MOON_QUARTER_MAX_ILLUMINATION=0.54
# Frame-acceptance thresholds — a candidate must beat all three to qualify.
@@ -524,33 +546,6 @@ MOON_HEIGHT_PCT=0.92 # moon disk fills this fraction of frame heig
MOON_DIALAMOON_TARGET_PX=2048 # cached PNG longest side; downsampled on save
MOON_DIALAMOON_TIMEOUT_SEC=30
# Atmospheric overlay ─────────────────────────────────────────────────────────
# East's camera frame is scaled to output size, blurred, and composited OVER
# the NASA moon disk. This is physically correct: clouds sit between the
# observer and the moon, so they occlude the disk rather than appear behind it.
#
# Opacity is derived from the moon detection quality in that frame:
# quality ≥ 0.85 → 0% (clear sky — pure NASA render)
# quality 0.70 → 20% (light haze)
# quality 0.55 → 40% (notable cloud, moon still detected)
# quality < 0.55 → 4065% (overcast fallback — see MOON_CLOUDY_POST_ENABLED)
# no detection → 68% (heavy overcast)
#
# blur radius: 0 = auto (output_width / 10); set in px to override.
#MOON_ATMOSPHERE_BLUR=0
#
# Cloudy-month fallback ───────────────────────────────────────────────────────
# If no frame in the collection window passes the quality + illumination
# thresholds, the script normally skips posting that month. With
# MOON_CLOUDY_POST_ENABLED=true it instead finds the above-horizon frame
# closest to the exact phase moment, applies a heavy atmospheric overlay
# (opacity 0.450.68), and posts the month anyway — the moon shows as a faint
# glow behind cloud rather than being absent entirely.
#
# This applies to all three phases: full, first-quarter, third-quarter.
# Caption will read "cloud cover — YYYY-MM-DD — NASA SVS Dial-a-Moon".
MOON_CLOUDY_POST_ENABLED=true
# ── Mattermost — daily sunrise upload ─────────────────────────────────────────
# mattermost_url, access_token, channel_id go in .env (see bottom of this file).
+58 -81
View File
@@ -1,64 +1,34 @@
#!/usr/bin/env python3
"""test_moon_composite.py — smoke-test atmospheric overlay at three opacity levels.
"""test_moon_composite.py — render a phase composite using real NASA data.
Generates three output images from the same east camera frame (21-07-00.jpg)
to show how the atmospheric overlay looks across the quality spectrum:
Simulates what moon_phase_monthly.py does on the night of a full moon:
test_composite_clear.jpg — opacity 0.00 (quality ≥ 0.85, clear sky)
test_composite_hazy.jpg — opacity 0.20 (quality ~ 0.70, light haze)
test_composite_cloudy.jpg — opacity 0.65 (overcast fallback)
The moon disk in each image is procedurally generated (clean grey sphere,
no camera timestamp). In production it is replaced by the NASA SVS
Dial-a-Moon render for the exact UTC hour east captured the moon.
1. Fetch the NASA SVS Dial-a-Moon render for 2026-04-29T22:00Z.
2. Load the east camera frame (21-07-00.jpg) and check for a clear moon.
3. If clear: render — NASA moon with parallactic angle rotation → test_composite_out.jpg.
4. If not clear: exit with a message (no fallback image).
Run from the sky-cam directory:
python3 test_moon_composite.py
Requires internet access to reach svs.gsfc.nasa.gov.
"""
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'
CASES = [
('test_composite_clear.jpg', 0.00, 'clear sky (quality >= 0.85)'),
('test_composite_hazy.jpg', 0.20, 'light haze (quality ~ 0.70)'),
('test_composite_cloudy.jpg', 0.65, 'heavy overcast fallback'),
]
# Obs time: 22:00 UTC on 2026-04-29 — aligns directly with NASA hourly renders.
NASA_FETCH_UTC = datetime(2026, 4, 29, 22, 0, tzinfo=timezone.utc)
def _make_procedural_moon(size: int = 2048) -> 'Image':
"""Clean grey disc with simplified lunar 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')
return Image.fromarray(arr)
MIN_QUALITY = 0.55
def main():
@@ -66,49 +36,56 @@ 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)
from moon_composite import render_phase_closeup
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. Check east frame for clear moon detection
print(f'checking moon in {EAST_FRAME.name} ...')
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}]'
)
print(f'rendering {filename} (opacity={opacity:.2f}) {label}')
render_phase_closeup(
nasa_render_path=tmp_moon,
out_path=str(out),
output_size=(1920, 1080),
moon_height_pct=0.88,
caption=caption,
east_frame_path=str(EAST_FRAME),
atmosphere_opacity=opacity,
atmosphere_blur=0,
)
print(f' -> {out}')
finally:
os.unlink(tmp_moon)
from moon_detect import detect_moon
det = detect_moon(str(EAST_FRAME))
quality = det.quality if det is not None else None
except Exception as e:
print(f' detection failed: {e}', file=sys.stderr)
sys.exit(2)
if quality is None or quality < MIN_QUALITY:
print(f' quality={quality} — no clear moon detection — skipping (no fallback)')
sys.exit(0)
print(f' quality={quality:.3f} — clear shot confirmed')
print()
print('done. Three outputs:')
for filename, opacity, label in CASES:
print(f' {filename:35s} opacity={opacity:.2f} {label}')
# 2. Fetch NASA Dial-a-Moon
print(f'fetching NASA Dial-a-Moon for {NASA_FETCH_UTC.strftime("%Y-%m-%dT%H:00Z")} ...')
try:
import moon_dialamoon
nasa_path = moon_dialamoon.fetch_for_time(NASA_FETCH_UTC)
print(f' cached at {nasa_path}')
except Exception as e:
print(f' NASA fetch failed: {e}', file=sys.stderr)
sys.exit(3)
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')
# 3. Render with parallactic angle rotation
from moon_composite import render_phase_closeup
caption = (
f'Full Moon — April 2026 — '
f'sky-cam east 2026-04-29 22:00 UTC — '
f'NASA SVS Dial-a-Moon'
)
print(f'rendering {OUT_PATH.name} ...')
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,
when_utc=NASA_FETCH_UTC,
)
print(f'done -> {OUT_PATH}')
if __name__ == '__main__':