Switch monthly pipeline from render_phase_closeup (black background) to
composite_full_moon (east frame + NASA moon overlay) when an east frame
and detection are available. Falls back to render_phase_closeup when
east verification is disabled.
Changes:
- composite_full_moon: bilateral filter (d=9, σ=75) on upscaled background
to smooth pixelation artifacts before compositing the NASA moon
- composite_full_moon: caption now placed below the moon disk instead of
overlapping it (paste_y + target_size + 12)
- run_phase: keep detection result (best_det) alongside best_frame
- _render_and_post: accept east_frame + detection, route to the right renderer
- Monthly pipeline uses moon_height_pct=0.70 for the east-frame composite
https://claude.ai/code/session_01JieSeNQZ3X6fhsb11YyJrK
moon_phase.py: add sun_events_in_range() — returns actual sunset/sunrise
transitions via skyfield almanac, accurate to within a minute
moon_phase_monthly.py:
- _dark_moon_intervals(): replace sun-altitude threshold sampling with
actual sunset/sunrise times; dark window = sunset + DARK_START_MIN to
next sunrise; moon-above-horizon check still sampled every 10 min within
each night; polar fallback if no sun events found
- run_phase(): sort dark-window frames by proximity to exact phase moment
before scanning; first clear detection = the frame temporally closest to
the moon being precisely full/at quarter, not just the first in time order
- Replace DARK_SKY_SUN_ALT_DEG with DARK_START_MIN (default 30 min)
sky-cam.conf: replace MOON_DARK_SKY_SUN_ALT_DEG with MOON_DARK_START_MIN=30;
update comments to explain ±24h window, sunset+30 start, closest-frame logic,
and how the 01:30 and 23:55 edge cases are handled
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
moon_phase.py: add sun_altaz() to compute sun altitude for dark-sky check
moon_phase_monthly.py:
- Replace fixed 22:00-23:00 window with dynamic dark+moon intervals:
sample every 10 min across ±24h of the phase moment, keep blocks where
sun < DARK_SKY_SUN_ALT_DEG and moon > MIN_ALTITUDE — covers the full
night the moon is actually visible in a dark sky regardless of month
- First east frame with quality >= MIN_QUALITY in that window wins
- Illumination% computed at the detection time and shown in the image
caption and Mattermost message
- Remove OBS_TIME_H/M; add DARK_SKY_SUN_ALT_DEG config var
sky-cam.conf: replace MOON_OBS_TIME_LOCAL with MOON_DARK_SKY_SUN_ALT_DEG=-6
and explain the sun-altitude threshold options
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
- moon_composite.py: remove _make_atmosphere_layer() and all atmosphere
parameters from render_phase_closeup(); add when_utc parameter and apply
parallactic angle rotation so the NASA disk is oriented to match east's sky
- moon_phase_monthly.py: change obs time default to 22:00 (aligns with NASA
hourly renders); scan east frames in 22:00-23:00 window; binary go/no-go
(quality >= MIN_QUALITY = post, no clear shot = skip entirely); remove
_atmosphere_opacity_from_quality(), ATMOSPHERE_BLUR, CLOUDY_POST_ENABLED
- sky-cam.conf: update MOON_OBS_TIME_LOCAL to 22:00, remove
MOON_OBS_WINDOW_MIN, remove the atmospheric overlay and cloudy fallback
sections and their config variables
- test_moon_composite.py: single clean test — fetch NASA for 22:00 UTC on
2026-04-29, verify east frame quality, render with parallactic angle; no
procedural fallback
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
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
The core mental model was wrong: clouds are between the observer and
the moon, so they occlude the disk — they don't sit behind it.
moon_composite.py:
_make_east_sky_backdrop() → _make_atmosphere_layer()
render_phase_closeup() pipeline is now:
1. Black background
2. NASA moon disk centred (correct phase / libration / shadows)
3. East frame scaled + blurred → composited OVER the disk at
atmosphere_opacity (0.0 = clear, 0.68 = heavy overcast)
Parameters: east_sky_enabled/blur → atmosphere_opacity/blur
moon_phase_monthly.py:
_atmosphere_opacity_from_quality() maps detection quality to opacity:
quality >= 0.85 → 0.00 (clear)
quality 0.70 → 0.20 (light haze)
quality 0.55 → 0.40 (notable cloud, still detected)
quality None → 0.68 (no detection, heavy overcast)
Frame scan now tracks two lists:
qualifying — frames passing quality + illumination (existing)
above_horizon — frames where moon is up but detection failed
When qualifying is empty and MOON_CLOUDY_POST_ENABLED=true, the
above-horizon frame closest to the exact phase moment is used with
opacity 0.45–0.68. The month is always represented — full moon,
first quarter, and third quarter each get a post even in cloudy
months, showing the moon as a faint glow behind cloud.
sky-cam.conf:
MOON_EAST_SKY_ENABLED/BLUR → MOON_ATMOSPHERE_BLUR (opacity is
computed automatically from quality, not configured directly)
New: MOON_CLOUDY_POST_ENABLED=true
test_moon_composite.py:
Generates three outputs at opacity 0.00 / 0.20 / 0.65 so the
full opacity range is visible in one test run.
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
The annular-ring veil approach sampled too small a region (38 px moon
in 3840×2160 gives a tiny annulus) and was invisible in practice.
More fundamentally, using the whole east sky is what "relayed to where
it was taken" actually means.
New approach — _make_east_sky_backdrop():
Scale the full east camera frame to output size, apply GaussianBlur
r = output_width // 6 (≈ 320 px at 1920 wide). The blur erases RTSP
artefacts, OSD overlays, and the wide-angle look while preserving real
sky colour, cloud / haze gradients, and the dark ground silhouette.
The NASA moon disk is pasted sharp on top. The result reads as east
photographed the moon through a telephoto with its actual sky that night.
Clear dark sky → nearly black backdrop (same feel as before).
Thin cloud cover → soft grey-blue haze behind the sharp moon.
Heavy overcast → the moon detection would not qualify, so this case
never reaches rendering.
Config rename: MOON_CLOUD_OVERLAY_* → MOON_EAST_SKY_ENABLED / _BLUR.
moon_phase_monthly.py: CLOUD_OVERLAY_* → EAST_SKY_*.
render_phase_closeup(): cloud_overlay_* params → east_sky_*.
test_moon_composite.py: replace full_moon_closeup.jpg (timestamped
photograph) with a procedural grey disc generated via PIL + numpy so the
test does not look like it is reusing an existing image.
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
Three changes driven by the same goal: make each monthly moon post
look like east captured it at that exact moment.
Tighter illumination windows (±4% of target phase):
Full moon: 95% → 96–100% (was a 5-point band; now hugs exact full)
Quarters: 40–65% → 46–54% (was a 25-point band; now ±4% of 50%)
This ensures the NASA Dial-a-Moon render timestamp is pulled within
4 percentage points of the true phase, making the fetched image
genuinely represent that night's moon. One fresh fetch per event,
~3/month, cached by hour — never reused across months.
Atmospheric cloud veil from east's surrounding sky:
_extract_cloud_veil() samples the annular sky region just outside
east's moon disk (2×–5× radius), scales it to the output frame,
blurs heavily (GaussianBlur r≈output_width/10) so it reads as haze
rather than an upscaled photo, then blends it over the NASA composite
at an opacity proportional to sky brightness:
sky < 5% mean brightness → no veil (clear dark night)
sky ~10% → ~17% veil (thin haze / airglow)
sky ≥ 20% → 40% veil (max, MOON_CLOUD_OVERLAY_MAX_OPACITY)
After the veil pass the NASA moon disk is re-pasted sharply so the
haze sits naturally behind the crisp lunar surface.
This is the honest answer to "east can't capture high-res clouds":
east's real atmospheric fingerprint becomes the veil texture.
New sky-cam.conf keys:
MOON_CLOUD_OVERLAY_ENABLED=true
MOON_CLOUD_OVERLAY_MAX_OPACITY=0.40
#MOON_CLOUD_OVERLAY_BLUR=0 (0 = auto)
https://claude.ai/code/session_01HkTxpNSTWtViZzxbrbKytR
The previous east-flavored composite (tight-crop east region + lunar
texture overlay) was honest but visually limited: 38-px source moon, no
real terminator shadows on quarters, and a faint upscaled-halo
background that was less compelling than just a clean lunar render.
New flow:
- East stays the witness (verifies the moon was visible during the
collection window) and supplies the timestamp.
- moon_dialamoon.py fetches the NASA SVS Dial-a-Moon render for that
exact UTC hour. Free, public-domain, real-physics: correct phase,
libration, and crater shadows for any timestamp.
- moon_composite.render_phase_closeup() places that render at ~92% of
frame height on a 1920x1080 black background -- the long-telephoto
look the user asked for.
- One API call per phase event (~36/year), cached forever in
moon-ref/dialamoon/.
Quarter moons now show real 3D crater shadows along the terminator,
which the prior algorithmic phase-shadow couldn't simulate from a
full-moon reference.
Adds MOON_REQUIRE_EAST_VERIFY=true|false toggle so the user can choose
"only post when east saw it" (default, current behavior) vs "post every
cycle regardless of weather over east."
Drops the install-time lunar reference download (no longer needed) and
the now-unused per-phase phase-shadow path stays in moon_composite.py
for reference / future reuse.
https://claude.ai/code/session_015PBVDESC3KLMbq1LpA6qLn
Two new jobs operate on the SUNRISE_CAM, sharing three Python helpers
(moon_phase, moon_detect, moon_composite) and one cached lunar texture:
- moon-track.sh: nightly batch detects the moon in each east frame,
crops a 480x480 box around it, stitches into an mp4 that holds the
moon roughly centred while clouds and stars drift past.
- moon-phase-monthly.sh: daily check that runs whichever phase composite
is due that day. Handles full moon (posts D+3), first quarter (D+2,
best-effort due to daytime-only geometry from east), and third quarter
(D+2). Picks the frame closest in time to the exact phase moment that
meets quality / altitude / illumination thresholds, then composites
the cached lunar texture into it -- sky/halo/parallactic-angle/timing
real from east, surface detail borrowed from the reference image.
Honest-by-design: a 38-px white blob from a wide-field IP camera cannot
be enhanced into crater detail by software. The composite makes the
borrowing explicit and constrains everything else (when, where, sky,
orientation) to match what east actually saw.
install.sh now downloads the skyfield ephemeris (de421.bsp) and the
default lunar reference (Wikipedia CC BY-SA full-moon photo) on first
run. Both can be overridden via .env.
https://claude.ai/code/session_015PBVDESC3KLMbq1LpA6qLn
Claude