| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.08 | 0.00 | 11.25 | 19.45 | 354.79 | -31.00 | 63.95 | 0.5368 | -199.0 | -134.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.38 | 15.14 | 6.10 | -19.69 | 65.46 | 0.3591 | -680.0 | -548.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 16.84 | 4.16 | -21.63 | 63.07 | 0.3973 | -781.0 | -571.7 | |
| 0.00 | 2.43 | 0.00 | 1.34 | 18.40 | 1.15 | -24.64 | 62.23 | 0.4490 | -981.0 | -747.4 | |
| 0.00 | 2.16 | 0.00 | 1.21 | 19.84 | 0.56 | -25.23 | 59.82 | 0.4657 | -714.0 | -561.8 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 19.13 | 0.21 | -25.57 | 61.49 | 0.4660 | -790.0 | -608.8 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 18.63 | 0.01 | -25.77 | 62.66 | 0.4658 | -700.0 | -537.4 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 18.55 | 359.74 | -26.05 | 63.01 | 0.4691 | -648.0 | -518.3 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 16.61 | 359.44 | -26.35 | 67.15 | 0.4634 | -574.0 | -522.8 | |
| 0.00 | 1.71 | 0.00 | 1.09 | 21.79 | 348.17 | -37.62 | 63.81 | 0.6340 | 179.0 | 250.4 | |
| 0.00 | 0.81 | 0.00 | 0.52 | 21.79 | 347.71 | -38.08 | 64.00 | 0.6394 | 709.0 | 529.0 | |
| 0.00 | 1.98 | 0.00 | 1.28 | 21.99 | 347.40 | -38.39 | 63.82 | 0.6439 | 485.0 | 407.9 | |
| 0.00 | 0.81 | 0.00 | 0.52 | 19.62 | 346.58 | -39.21 | 67.68 | 0.6459 | 524.0 | 449.9 | |
| 0.00 | 1.35 | 0.00 | 0.87 | 19.50 | 346.57 | -39.22 | 67.88 | 0.6456 | 613.0 | 548.8 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 19.33 | 346.50 | -39.29 | 68.15 | 0.6461 | 572.0 | 461.6 | |
| 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. | |