| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.16 | 0.00 | 19.48 | 11.00 | 308.43 | 50.00 | 281.62 | 0.7691 | 115.9 | 29.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.91 | 0.00 | 2.55 | 11.21 | 314.03 | 55.60 | 281.29 | 0.8275 | -619.0 | -504.5 | |
| 0.00 | 1.63 | 0.00 | 1.38 | 11.31 | 312.38 | 53.95 | 281.56 | 0.8114 | -532.0 | -450.8 | |
| 0.00 | 0.64 | 0.00 | 0.51 | 9.09 | 310.50 | 52.07 | 278.92 | 0.7906 | -528.0 | -519.1 | |
| 0.00 | 0.54 | 0.00 | 0.43 | 6.48 | 309.84 | 51.41 | 275.62 | 0.7826 | -525.0 | -466.5 | |
| 0.00 | 1.09 | 0.00 | 0.87 | 9.08 | 309.99 | 51.56 | 278.94 | 0.7852 | -455.0 | -469.2 | |
| 0.00 | 1.54 | 0.00 | 1.22 | 8.11 | 309.71 | 51.28 | 277.72 | 0.7817 | -691.0 | -554.5 | |
| 0.00 | 2.18 | 0.00 | 1.72 | 10.08 | 309.61 | 51.18 | 280.25 | 0.7818 | -467.0 | -470.1 | |
| 0.00 | 0.91 | 0.00 | 0.68 | 10.22 | 307.22 | 48.79 | 280.66 | 0.7556 | 265.0 | 274.1 | |
| 0.00 | 0.82 | 0.00 | 0.61 | 10.35 | 307.01 | 48.58 | 280.85 | 0.7534 | 380.0 | 339.3 | |
| 0.00 | 1.82 | 0.00 | 1.36 | 10.49 | 306.81 | 48.38 | 281.05 | 0.7512 | 664.0 | 502.8 | |
| 0.00 | 1.18 | 0.00 | 0.88 | 10.35 | 306.45 | 48.02 | 280.91 | 0.7470 | 579.0 | 451.2 | |
| 0.00 | 2.00 | 0.00 | 1.48 | 10.66 | 306.33 | 47.90 | 281.34 | 0.7459 | 643.0 | 551.0 | |
| 0.00 | 1.63 | 0.00 | 1.21 | 11.62 | 306.31 | 47.88 | 282.63 | 0.7468 | 661.0 | 469.3 | |
| 0.00 | 1.45 | 0.00 | 1.07 | 11.74 | 305.69 | 47.26 | 282.87 | 0.7399 | 578.0 | 498.4 | |
| 0.00 | 0.91 | 0.00 | 0.67 | 12.08 | 305.77 | 47.33 | 283.32 | 0.7412 | 563.0 | 518.3 | |
| 0.00 | 1.91 | 0.00 | 1.39 | 13.68 | 305.24 | 46.81 | 285.57 | 0.7377 | 297.0 | 279.6 | |
| 0.00 | 0.82 | 0.00 | 0.60 | 14.98 | 304.82 | 46.39 | 287.40 | 0.7352 | 736.0 | 633.0 | |
| 0.00 | 1.18 | 0.00 | 0.85 | 14.61 | 303.98 | 45.55 | 287.08 | 0.7250 | 537.0 | 394.9 | |
| 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. | |