| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.84 | 0.00 | 12.28 | 5.09 | 256.20 | 13.07 | 298.84 | 0.2476 | 580.9 | 498.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.68 | 5.53 | 274.35 | 31.22 | 280.03 | 0.5260 | -720.0 | -618.1 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 4.93 | 272.27 | 29.13 | 279.44 | 0.4937 | -261.0 | -266.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 6.80 | 270.70 | 27.57 | 283.83 | 0.4752 | -746.0 | -586.9 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 1.92 | 262.14 | 19.01 | 274.87 | 0.3281 | 906.0 | 653.2 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 4.35 | 262.06 | 18.93 | 282.25 | 0.3324 | 791.0 | 647.5 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 6.40 | 260.65 | 17.51 | 289.49 | 0.3186 | 716.0 | 605.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 0.95 | 260.43 | 17.30 | 272.08 | 0.2988 | 743.0 | 545.4 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 4.34 | 256.09 | 12.96 | 287.34 | 0.2353 | 777.0 | 635.1 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 7.34 | 256.07 | 12.94 | 298.75 | 0.2544 | 952.0 | 708.0 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 9.86 | 253.36 | 10.22 | 313.41 | 0.2418 | 697.0 | 539.2 | |
| 0.00 | 4.44 | 0.00 | 2.22 | 5.21 | 250.55 | 7.42 | 303.40 | 0.1547 | 1144.0 | 842.8 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 7.66 | 249.76 | 6.62 | 318.08 | 0.1718 | 982.0 | 703.1 | |
| 0.00 | 2.08 | 0.00 | 1.03 | 1.19 | 246.42 | 3.29 | 284.46 | 0.0595 | 891.0 | 726.1 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 6.53 | 244.67 | 1.54 | 346.10 | 0.1115 | 910.0 | 651.2 | |
| 0.00 | 1.00 | 0.00 | 0.49 | 1.35 | 243.17 | 0.03 | 358.23 | 0.0176 | 932.0 | 690.6 | |
| 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. | |