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Table 5
Comparison of the positions of the same spot in two different image plates.
| Date | Plate XLVI | Plate XLVII | |||||
| 1625 | CMD | λ | S | CMD | λ | S | δ |
|
|
|||||||
| Nov. 06 |
|
|
3 |
|
|
3 | 0.̊54 |
| Nov. 07 |
|
|
5 |
|
|
5 | 1.̊22 |
| Nov. 08 |
|
|
4 |
|
|
5 | 1.̊19 |
| Nov. 09 |
|
|
5 |
|
|
5 | 0.̊89 |
| Nov. 10 |
|
|
5 |
|
|
4 | 0.̊51 |
| Nov. 11 |
|
|
5 |
|
|
4 | 0.̊45 |
Notes. CMD is the central-meridian distance, λ is the heliographic latitude, S is the cursor size class according to Fig. 3, and δ contains the heliocentric distance between the two measurements.
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