Fix season dates, resolution, attribution, retention policies, montage trigger
season_info.py (new): - Computes actual equinox/solstice dates via Jean Meeus approximation - Converts to LOCAL timezone (pytz / zoneinfo) so the calendar date reflects what the camera sees on the ground, including DST transitions - Timezone defaults to America/New_York; override via $TIMEZONE env or 2nd arg - Divides each season into 3 equal movements; handles Winter's year boundary - Outputs IS_LAST_DAY=true on the final day of each movement 4-seasons.sh: - Uses season_info.py for all date/season logic (no hardcoded day-of-year) - Passes $yesterday to season_info.py so astronomical dates are correct - Removed forced 1280x720 scale; clips stay at native camera resolution - Auto-triggers montage-mvt.sh "$yesterday" on last day of movement so the correct movement (not the next day's) is compiled montage-mvt.sh: - Accepts optional YYYY-MM-DD argument (passed by 4-seasons.sh) so it resolves the correct season/movement when run the morning after last day - Detects source resolution from first daily clip via ffprobe; attribution card is generated at that exact resolution — no resizing of main video - Font sizes proportional to frame height so text looks right at any res - License corrected to CC BY-SA 3.0 (was CC BY-NC-SA 4.0) fullday-video.sh: - Removed 30-minute target; video length is natural (num_images / FPS) - Default FULLDAY_FPS=5 (configurable at top of script) - Retains RETENTION_DAYS=10 auto-delete for full-day videos only - Sunrise 10s uploads and montage videos are never auto-deleted https://claude.ai/code/session_01C4jbd3waXG3eKZYbGUjLUQ
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Claude
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#!/usr/bin/env python3
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"""
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season_info.py — output shell variables describing the current (or given) date's
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astronomical season and movement within that season.
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Season boundaries are the actual equinoxes/solstices computed via the Jean Meeus
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approximation (Astronomical Algorithms, Ch. 27 Table 27.a) and converted to the
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LOCAL timezone so the calendar date matches what the camera sees on the ground.
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DST transitions and year-to-year variation in the exact equinox moment are both
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handled correctly.
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Usage:
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eval "$(python3 season_info.py [YYYY-MM-DD] [Timezone])"
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Arguments (both optional):
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YYYY-MM-DD Date to evaluate; defaults to today.
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Timezone IANA timezone name, e.g. America/New_York.
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Can also be set via the TIMEZONE environment variable.
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Defaults to America/New_York (matches the sunrise scripts).
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Outputs (shell-sourceable):
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SEASON Spring | Summer | Autumn | Winter
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MVT_NUM 1 | 2 | 3
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DAY_OF_MVT day number within the movement (1-based)
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DAYS_IN_MVT total days in this movement
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MVT_START YYYY-MM-DD of movement start (local date)
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MVT_END YYYY-MM-DD of movement end (local date)
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SEASON_START YYYY-MM-DD of season start (local date)
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SEASON_END YYYY-MM-DD of season end (local date)
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IS_LAST_DAY true | false
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"""
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import sys
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import os
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import datetime
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DEFAULT_TZ = "America/New_York"
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# ---------------------------------------------------------------------------
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# Timezone helpers — prefer pytz (already installed for sunrise.py),
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# fall back to zoneinfo (Python ≥ 3.9), then to UTC with a warning.
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# ---------------------------------------------------------------------------
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def _load_tz(name: str):
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try:
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import pytz
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return pytz.timezone(name)
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except ImportError:
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pass
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try:
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from zoneinfo import ZoneInfo
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return ZoneInfo(name)
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except ImportError:
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pass
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print(f"WARNING: neither pytz nor zoneinfo available; using UTC instead of {name}", file=sys.stderr)
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return datetime.timezone.utc
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def _utc_datetime_from_jde(jde: float) -> datetime.datetime:
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"""Convert Julian Day Number to a UTC datetime (including time of day)."""
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jde_s = jde + 0.5 # shift so integer part = calendar day
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Z = int(jde_s)
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F = jde_s - Z # fractional day = fraction of 24 h after midnight
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if Z >= 2299161:
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alpha = int((Z - 1867216.25) / 36524.25)
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A = Z + 1 + alpha - alpha // 4
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else:
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A = Z
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B = A + 1524
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C = int((B - 122.1) / 365.25)
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D = int(365.25 * C)
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E = int((B - D) / 30.6001)
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day_frac = B - D - int(30.6001 * E) + F
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day = int(day_frac)
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frac_hours = (day_frac - day) * 24
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hour = int(frac_hours)
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frac_mins = (frac_hours - hour) * 60
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minute = int(frac_mins)
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second = int((frac_mins - minute) * 60)
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month = E - 1 if E < 14 else E - 13
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year = C - 4716 if month > 2 else C - 4715
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return datetime.datetime(year, month, day, hour, minute, second,
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tzinfo=datetime.timezone.utc)
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def _season_starts_local(year: int, tz) -> dict:
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"""
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Return the LOCAL calendar date (not UTC date) of each equinox/solstice
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for the given year. 'tz' is a pytz/zoneinfo timezone object.
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"""
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y = (year - 2000) / 1000.0
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jdes = {
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"Spring": 2451623.80984 + 365242.37404*y + 0.05169*y**2 - 0.00411*y**3 - 0.00057*y**4,
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"Summer": 2451716.56767 + 365241.62603*y + 0.00325*y**2 + 0.00888*y**3 - 0.00030*y**4,
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"Autumn": 2451810.21715 + 365242.01767*y - 0.11575*y**2 + 0.00337*y**3 + 0.00078*y**4,
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"Winter": 2451900.05952 + 365242.74049*y - 0.06223*y**2 - 0.00823*y**3 + 0.00032*y**4,
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}
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result = {}
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for name, jde in jdes.items():
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utc_dt = _utc_datetime_from_jde(jde)
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local_dt = utc_dt.astimezone(tz)
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result[name] = local_dt.date()
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return result
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def get_info(date: datetime.date, tz_name: str = DEFAULT_TZ) -> dict:
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tz = _load_tz(tz_name)
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year = date.year
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cur = _season_starts_local(year, tz)
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prev = _season_starts_local(year - 1, tz)
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nxt = _season_starts_local(year + 1, tz)
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# Determine season and its inclusive start/end dates.
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# Winter straddles the year boundary (Dec solstice → next Mar equinox).
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if date < cur["Spring"]:
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season, s_start, s_end = "Winter", prev["Winter"], cur["Spring"] - datetime.timedelta(days=1)
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elif date < cur["Summer"]:
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season, s_start, s_end = "Spring", cur["Spring"], cur["Summer"] - datetime.timedelta(days=1)
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elif date < cur["Autumn"]:
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season, s_start, s_end = "Summer", cur["Summer"], cur["Autumn"] - datetime.timedelta(days=1)
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elif date < cur["Winter"]:
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season, s_start, s_end = "Autumn", cur["Autumn"], cur["Winter"] - datetime.timedelta(days=1)
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else:
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season, s_start, s_end = "Winter", cur["Winter"], nxt["Spring"] - datetime.timedelta(days=1)
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days_in_season = (s_end - s_start).days + 1
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# Split season into 3 movements. Mvt 1 and 2 get floor(n/3) days;
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# Mvt 3 takes the remainder so no days are lost to integer rounding.
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m1 = days_in_season // 3
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m2 = days_in_season // 3
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m3 = days_in_season - m1 - m2
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m1_end = s_start + datetime.timedelta(days=m1 - 1)
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m2_end = m1_end + datetime.timedelta(days=m2)
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m3_end = s_end
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if date <= m1_end:
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mvt, mvt_start, mvt_end, days_in_mvt = 1, s_start, m1_end, m1
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elif date <= m2_end:
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mvt, mvt_start, mvt_end, days_in_mvt = 2, m1_end + datetime.timedelta(1), m2_end, m2
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else:
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mvt, mvt_start, mvt_end, days_in_mvt = 3, m2_end + datetime.timedelta(1), m3_end, m3
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return {
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"SEASON": season,
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"MVT_NUM": mvt,
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"DAY_OF_MVT": (date - mvt_start).days + 1,
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"DAYS_IN_MVT": days_in_mvt,
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"MVT_START": mvt_start.isoformat(),
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"MVT_END": mvt_end.isoformat(),
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"SEASON_START": s_start.isoformat(),
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"SEASON_END": s_end.isoformat(),
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"IS_LAST_DAY": str(date == mvt_end).lower(),
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}
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if __name__ == "__main__":
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args = [a for a in sys.argv[1:] if not a.startswith("-")]
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date_s = args[0] if len(args) > 0 else None
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tz_name = args[1] if len(args) > 1 else os.environ.get("TIMEZONE", DEFAULT_TZ)
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date = datetime.date.fromisoformat(date_s) if date_s else datetime.date.today()
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for k, v in get_info(date, tz_name).items():
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print(f'{k}="{v}"')
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