AUSPICIOUS 8 · CCD / COUNTER LAB

Virtual Telescope → Future Physical Telescope · Core20

This browser bench models the observation record a future physical CCD / counter instrument can produce.

WHAT A REAL OBSERVER WOULD GIVE US

frameId
rawPulse       free-running arbitrary counter captured for the frame
moon           io | eu | ga
jupiterX       measured Jupiter center in CCD pixels
moonX          measured moon center in CCD pixels
visible        optional
uncertaintyX   optional

Only reduction: x = moonX − jupiterX.

No degree conversion is required for turn detection. Original images and counter logs remain the evidence.

Fake CCD generator

Generated data includes Jupiter detector drift, different moon starting phases, arbitrary counter values and centroid noise. Later, replace these rows with real measurements.

CCD / counter records

Observation-format preview

The reduced observation record keeps only rawPulse + moon + signed Jupiter-relative x. Exporting it here does not feed or alter Core20.

Placard for a future volunteer

1. Run one monotonic free-running counter.
2. Capture its value with each CCD frame.
3. Measure Jupiter center X in pixels.
4. Measure Io / Europa / Ganymede center X in the same frame.
5. Keep originals. Do not pre-convert pixels to degrees for A8.
6. Send CSV:
   frameId,rawPulse,moon,jupiterX,moonX,visible,uncertaintyX

The session does not need to start at WEST. It only needs enough observations around repeated extrema. For full 8:4:2 qualification, long coverage is needed; shorter data can still test early recovery.