| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.97 | 27.41 | 5.58 | 25.61 | -19.59 | 109.78 | 55.55 | 246.38 | 0.8495 | 124.7 | 235.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 1.12 | -20.79 | 112.50 | 58.28 | 245.71 | 0.8744 | 198.0 | 167.0 | |
| 2.30 | 4.78 | 2.27 | 4.72 | -20.21 | 111.68 | 57.45 | 246.16 | 0.8669 | 361.0 | 200.7 | |
| 1.11 | 3.07 | 1.08 | 2.99 | -20.02 | 111.28 | 57.05 | 246.28 | 0.8632 | 519.8 | 449.1 | |
| 0.00 | 2.65 | 0.00 | 2.55 | -20.42 | 110.75 | 56.53 | 245.69 | 0.8598 | 504.0 | 464.1 | |
| 0.00 | 2.48 | 0.00 | 2.28 | -18.15 | 109.52 | 55.29 | 247.98 | 0.8447 | 81.0 | 134.5 | |
| 0.00 | 1.45 | 0.00 | 1.38 | -20.01 | 110.41 | 56.18 | 246.07 | 0.8561 | 575.0 | 526.4 | |
| 0.00 | 1.96 | 0.00 | 1.78 | -17.83 | 108.99 | 54.76 | 248.22 | 0.8394 | 520.0 | 320.4 | |
| 0.00 | 0.85 | 0.00 | 0.81 | -20.35 | 110.20 | 55.97 | 245.63 | 0.8552 | 455.0 | 483.8 | |
| 0.00 | 1.20 | 0.00 | 1.14 | -20.99 | 110.10 | 55.87 | 244.88 | 0.8557 | 470.0 | 417.4 | |
| 0.68 | 2.39 | 0.61 | 2.15 | -18.33 | 108.57 | 54.34 | 247.54 | 0.8368 | 627.6 | 504.0 | |
| 0.00 | 1.11 | 0.00 | 0.96 | -17.91 | 107.27 | 53.05 | 247.68 | 0.8242 | -514.0 | -367.3 | |
| 1.88 | 3.33 | 1.62 | 2.88 | -19.75 | 106.49 | 52.27 | 245.28 | 0.8216 | -474.2 | -327.8 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -19.75 | 106.24 | 52.01 | 245.21 | 0.8192 | -737.0 | -655.0 | |
| 0.00 | 0.77 | 0.00 | 0.63 | -19.11 | 104.40 | 50.17 | 245.40 | 0.8003 | -605.0 | -540.6 | |
| 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. | |