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Transmission Body:
Operatives utilizing manual German Equatorial Mounts (GEM) often suffer from “Star Smear” during long-duration intercepts. When your polar scope is obscured or misaligned, you must execute Protocol 04-A: The Drift Method.

Objective:
Achieve sub-arcsecond tracking accuracy by observing and correcting star drift.

Methodology:

  1. Azimuth Calibration: Point your optics at a star near the Celestial Equator and the Meridian (South). If the star drifts North in your eyepiece, your mount is pointing too far East. Rotate the mount’s base accordingly.
  2. Altitude Calibration: Target a star low on the Eastern horizon. If the star drifts North, your polar axis is pointing too Low. Adjust the altitude bolts to raise the mount.
  3. Refinement: Repeat these steps using a high-power illuminated reticle eyepiece for maximum precision.

Technician’s Note:
“Do not rush the correction. Small, incremental rotations are the only way to lock the signal. A drift of 1 pixel over 5 minutes is the threshold for a successful deep-space capture.”

Required Arsenal:

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