| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.43 | 0.00 | 11.28 | -18.81 | 77.48 | -36.34 | 125.91 | 0.6943 | 566.3 | 469.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.44 | 0.00 | 0.30 | -22.13 | 81.06 | -32.75 | 132.65 | 0.6837 | 662.0 | 602.8 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -21.65 | 81.19 | -32.63 | 132.20 | 0.6788 | 626.0 | 503.3 | |
| 0.00 | 0.44 | 0.00 | 0.29 | -20.07 | 80.17 | -33.65 | 129.47 | 0.6766 | 571.0 | 507.4 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -20.18 | 79.44 | -34.37 | 129.04 | 0.6846 | 641.0 | 530.6 | |
| 0.00 | 2.20 | 0.00 | 1.46 | -18.21 | 79.68 | -34.13 | 126.80 | 0.6680 | 786.0 | 668.0 | |
| 0.00 | 1.49 | 0.00 | 0.97 | -15.51 | 79.83 | -33.99 | 123.41 | 0.6476 | 753.0 | 572.5 | |
| 0.00 | 1.32 | 0.00 | 0.85 | -15.06 | 79.84 | -33.98 | 122.81 | 0.6444 | 785.0 | 617.6 | |
| 0.00 | 1.41 | 0.00 | 0.95 | -16.81 | 77.26 | -36.56 | 123.24 | 0.6840 | 828.0 | 722.8 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -19.58 | 75.64 | -38.18 | 125.55 | 0.7181 | 563.0 | 498.0 | |
| 0.00 | 1.23 | 0.00 | 0.92 | -23.37 | 74.43 | -39.39 | 129.12 | 0.7532 | 530.0 | 432.0 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -16.84 | 76.31 | -37.51 | 122.63 | 0.6943 | 645.0 | 558.8 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -16.65 | 76.31 | -37.50 | 122.39 | 0.6930 | 538.0 | 453.4 | |
| 0.00 | 1.05 | 0.00 | 0.75 | -19.43 | 74.95 | -38.87 | 124.91 | 0.7240 | 585.0 | 485.8 | |
| 0.00 | 1.41 | 0.00 | 1.06 | -20.57 | 72.25 | -41.57 | 124.54 | 0.7565 | -585.0 | -424.3 | |
| 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. | |