| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.80 | 287.79 | 64.41 | 299.73 | 3.39 | 162.44 | 61.56 | 273.38 | 0.8806 | -291.8 | -171.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.97 | 239.50 | 20.63 | 256.81 | 2.51 | 163.83 | 62.95 | 272.35 | 0.8924 | -588.1 | -237.4 | |
| 23.58 | -1.00 | 25.16 | -1.00 | 3.41 | 163.20 | 62.33 | 273.37 | 0.8875 | -607.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 1.16 | 4.19 | 162.41 | 61.54 | 274.27 | 0.8812 | -356.0 | -294.9 | |
| 2.99 | -1.00 | 3.09 | -1.00 | 3.78 | 162.23 | 61.36 | 273.80 | 0.8796 | -799.1 | 999999 | |
| 1.54 | -1.00 | 1.58 | -1.00 | 4.02 | 162.14 | 61.26 | 274.08 | 0.8789 | -558.8 | 999999 | |
| 0.00 | 1.28 | 0.00 | 1.23 | 3.64 | 159.70 | 58.82 | 273.69 | 0.8577 | -567.0 | -488.7 | |
| 3.84 | 6.15 | 3.66 | 5.86 | 4.50 | 159.52 | 58.64 | 274.71 | 0.8563 | 446.4 | 214.2 | |
| 0.00 | 2.65 | 0.00 | 2.48 | 3.80 | 158.92 | 58.04 | 273.90 | 0.8507 | -363.0 | -199.5 | |
| 0.00 | 0.60 | 0.00 | 0.55 | 4.34 | 158.53 | 57.66 | 274.55 | 0.8472 | 397.0 | 355.7 | |
| 0.77 | 2.99 | 0.71 | 2.75 | 4.08 | 158.28 | 57.40 | 274.24 | 0.8448 | 327.4 | 268.5 | |
| 1.79 | 4.19 | 1.58 | 3.67 | 5.53 | 156.46 | 55.59 | 276.06 | 0.8280 | 406.9 | 332.5 | |
| 0.00 | 1.20 | 0.00 | 1.04 | 3.69 | 156.14 | 55.26 | 273.85 | 0.8241 | 524.0 | 388.9 | |
| 0.00 | 0.60 | 0.00 | 0.52 | 3.93 | 155.90 | 55.02 | 274.15 | 0.8218 | 564.0 | 488.3 | |
| 1.54 | 3.76 | 1.34 | 3.27 | 5.68 | 156.06 | 55.19 | 276.27 | 0.8241 | 586.7 | 455.1 | |
| 0.00 | 1.03 | 0.00 | 0.89 | 6.76 | 155.71 | 54.84 | 277.60 | 0.8213 | 447.0 | 368.3 | |
| 6.24 | 18.97 | 5.36 | 16.32 | 6.19 | 155.57 | 54.69 | 276.93 | 0.8195 | 802.8 | 496.3 | |
| 1.54 | 2.99 | 1.30 | 2.54 | 4.03 | 155.08 | 54.21 | 274.30 | 0.8137 | 612.3 | 470.2 | |
| 0.00 | 0.77 | 0.00 | 0.64 | 4.25 | 154.20 | 53.32 | 274.61 | 0.8047 | 596.0 | 478.3 | |
| 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. | |