In the period from late autumn to early winter, the star patterns exhibit pronounced fluctuations. These variations necessitate a reevaluation of established navigation protocols.
| Time (UTC) | Star Identifier | Magnitude Deviation (dm) | Phase Angle (°) |
|---|---|---|---|
| 02:14 | Alpha Centauri | 0.0052 | 45 |
| 03:07 | Beta Orionis | -0.023 | 310 |
| 05:42 | Gamma Pegasi | 0.016 | 200 |
| 06:55 | Delta Pavonis | 0.018 | 90 |
The observed noise patterns are primarily caused by optical interferences. This warrants further examination through computerized models to mitigate impacts on navigation accuracy.