| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.68 | 248.66 | 26.58 | 172.31 | -23.84 | 193.88 | -40.40 | 121.98 | 0.7006 | 527.7 | 280.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.36 | 0.00 | 0.24 | -26.58 | 198.33 | -35.95 | 128.09 | 0.6694 | -574.0 | -469.8 | |
| 2.24 | 234.35 | 1.53 | 161.10 | -23.84 | 194.93 | -39.36 | 122.48 | 0.6899 | 989.7 | 338.2 | |
| 0.27 | -2.00 | 0.18 | -2.00 | -23.48 | 194.88 | -39.40 | 121.97 | 0.6886 | 1078.7 | 999999 | |
| 35.18 | -2.00 | 24.19 | -2.00 | -23.72 | 194.32 | -39.96 | 122.01 | 0.6958 | 994.2 | 999999 | |
| 0.99 | -2.00 | 0.68 | -2.00 | -23.38 | 193.71 | -40.57 | 121.25 | 0.7007 | 414.5 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -21.03 | 193.20 | -41.08 | 117.86 | 0.6961 | -543.0 | -439.2 | |
| 0.00 | 0.81 | 0.00 | 0.57 | -23.04 | 192.25 | -42.03 | 120.13 | 0.7147 | 510.0 | 341.0 | |
| 0.00 | 1.80 | 0.00 | 1.33 | -23.39 | 189.23 | -45.05 | 119.33 | 0.7474 | -537.0 | -383.0 | |
| 0.00 | 0.63 | 0.00 | 0.49 | -25.77 | 187.47 | -46.81 | 121.62 | 0.7733 | -735.0 | -616.6 | |
| 0.00 | 0.99 | 0.00 | 0.78 | -26.44 | 186.71 | -47.57 | 122.15 | 0.7828 | -603.0 | -546.2 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -26.03 | 186.43 | -47.85 | 121.55 | 0.7840 | -605.0 | -547.4 | |
| 0.00 | 1.44 | 0.00 | 1.16 | -26.31 | 185.67 | -48.61 | 121.60 | 0.7919 | -522.0 | -470.8 | |
| 0.00 | 1.26 | 0.00 | 1.01 | -25.88 | 185.76 | -48.53 | 121.11 | 0.7897 | -301.0 | -374.9 | |
| 0.00 | 1.71 | 0.00 | 1.42 | -27.91 | 184.55 | -49.73 | 123.11 | 0.8072 | -616.0 | -550.3 | |
| 0.00 | 0.72 | 0.00 | 0.58 | -26.13 | 185.51 | -48.77 | 121.34 | 0.7928 | -463.0 | -407.8 | |
| 0.00 | 0.81 | 0.00 | 0.70 | -29.14 | 183.53 | -50.76 | 124.18 | 0.8199 | -347.0 | -350.6 | |
| 0.00 | 1.62 | 0.00 | 1.32 | -26.38 | 185.06 | -49.23 | 121.48 | 0.7977 | -367.0 | -358.5 | |
| 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. | |