| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.34 | 217.41 | 49.60 | 189.17 | -11.36 | 79.11 | -54.89 | 102.51 | 0.8227 | -183.4 | -66.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.86 | 62.54 | 3.83 | 49.23 | -10.43 | 83.29 | -50.71 | 101.87 | 0.7801 | 841.4 | 348.0 | |
| 6.30 | -1.00 | 4.96 | -1.00 | -10.12 | 83.31 | -50.69 | 101.48 | 0.7795 | 866.3 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.72 | -11.28 | 82.74 | -51.26 | 102.87 | 0.7869 | 615.0 | 443.2 | |
| 0.00 | 1.98 | 0.00 | 1.58 | -10.72 | 82.78 | -51.23 | 102.18 | 0.7859 | 498.0 | 358.5 | |
| 0.00 | 1.17 | 0.00 | 0.98 | -12.09 | 80.63 | -53.37 | 103.59 | 0.8095 | 520.0 | 551.6 | |
| 0.00 | 1.26 | 0.00 | 1.05 | -11.19 | 80.73 | -53.27 | 102.50 | 0.8075 | 551.0 | 498.1 | |
| 0.00 | 0.54 | 0.00 | 0.45 | -11.93 | 80.52 | -53.48 | 103.38 | 0.8104 | 524.0 | 415.2 | |
| 3.42 | 5.31 | 2.90 | 4.50 | -12.36 | 80.24 | -53.76 | 103.86 | 0.8137 | 380.4 | 225.8 | |
| 0.00 | 1.26 | 0.00 | 1.11 | -12.87 | 78.78 | -55.22 | 104.29 | 0.8284 | 298.0 | 250.0 | |
| 0.00 | 0.72 | 0.00 | 0.63 | -12.32 | 78.90 | -55.10 | 103.64 | 0.8266 | 488.0 | 376.2 | |
| 1.17 | 1.98 | 1.02 | 1.72 | -10.84 | 79.13 | -54.88 | 101.88 | 0.8230 | -590.2 | -512.4 | |
| 3.15 | 65.51 | 2.79 | 60.00 | -12.49 | 78.41 | -55.59 | 103.79 | 0.8315 | 420.0 | -386.5 | |
| 3.42 | -12.00 | 3.05 | -12.00 | -12.42 | 78.15 | -55.85 | 103.67 | 0.8339 | -430.8 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.67 | -11.22 | 78.42 | -55.58 | 102.26 | 0.8302 | -257.0 | -360.0 | |
| 23.49 | 71.54 | 21.24 | 64.78 | -11.35 | 77.54 | -56.46 | 102.32 | 0.8386 | -785.0 | -182.4 | |
| 0.00 | 0.81 | 0.00 | 0.75 | -12.98 | 77.00 | -57.00 | 104.19 | 0.8451 | -456.0 | -486.6 | |
| 10.53 | -12.00 | 9.81 | -12.00 | -12.00 | 76.47 | -57.53 | 102.98 | 0.8489 | -482.8 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |