| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.34 | 0.00 | 11.59 | 4.90 | 267.47 | -22.51 | 76.97 | 0.3897 | -304.4 | -371.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.26 | 0.00 | 1.17 | 4.27 | 273.44 | -16.54 | 75.08 | 0.2951 | -1075.0 | -857.5 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 6.07 | 273.40 | -16.59 | 69.35 | 0.3047 | -869.0 | -691.1 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 6.23 | 273.20 | -16.78 | 69.09 | 0.3086 | -792.0 | -662.1 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 3.97 | 273.16 | -16.82 | 76.30 | 0.2984 | -969.0 | -727.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 5.92 | 273.05 | -16.93 | 70.19 | 0.3093 | -790.0 | -689.2 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 3.15 | 272.80 | -17.19 | 79.25 | 0.3016 | -828.0 | -747.3 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 4.03 | 272.75 | -17.24 | 76.41 | 0.3054 | -841.0 | -692.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 3.70 | 271.02 | -18.96 | 78.56 | 0.3323 | -677.0 | -507.4 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 3.00 | 270.32 | -19.66 | 80.96 | 0.3416 | -933.0 | -602.9 | |
| 0.00 | 1.99 | 0.00 | 1.05 | 2.48 | 270.04 | -19.94 | 82.57 | 0.3451 | -918.0 | -700.4 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 3.09 | 268.07 | -21.91 | 81.59 | 0.3783 | -820.0 | -644.5 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 8.74 | 259.66 | -30.32 | 72.96 | 0.5240 | 642.0 | 521.6 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 4.27 | 258.85 | -31.13 | 81.67 | 0.5231 | 701.0 | 570.5 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 5.58 | 258.50 | -31.48 | 79.29 | 0.5311 | 599.0 | 396.5 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 8.81 | 255.60 | -34.38 | 74.56 | 0.5811 | 306.0 | 343.5 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 6.29 | 255.27 | -34.72 | 78.95 | 0.5789 | 665.0 | 480.6 | |
| 0.00 | 0.54 | 0.00 | 0.35 | 9.99 | 251.50 | -38.48 | 74.11 | 0.6395 | 540.0 | 473.3 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 9.47 | 248.58 | -41.40 | 75.77 | 0.6752 | 579.0 | 609.0 | |
| 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. | |