| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 244 | 20 | 127 | -8.46 | 144.87 | -8.70 | 149.30 | 0.2910 | 165.6 | 278.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 9 | 2 | 5 | -8.82 | 150.24 | -3.33 | 167.20 | 0.2603 | -1073.6 | -719.4 | |
| 0 | 5 | 0 | 2 | -8.82 | 149.80 | -3.77 | 165.57 | 0.2621 | -944.0 | -642.7 | |
| 0 | 4 | 0 | 2 | -7.40 | 148.69 | -4.88 | 159.75 | 0.2447 | 970.0 | 728.8 | |
| 0 | 6 | 0 | 3 | -7.85 | 148.37 | -5.20 | 159.17 | 0.2538 | 988.0 | 840.0 | |
| 0 | 6 | 0 | 3 | -7.08 | 148.26 | -5.32 | 157.60 | 0.2423 | 825.0 | 765.1 | |
| 0 | 17 | 0 | 9 | -7.45 | 148.17 | -5.40 | 157.86 | 0.2486 | 955.0 | 884.2 | |
| 4 | 43 | 2 | 22 | -8.03 | 146.80 | -6.77 | 153.95 | 0.2671 | -84.8 | -668.0 | |
| 6 | -7 | 3 | -7 | -8.08 | 146.56 | -7.01 | 153.22 | 0.2696 | -1515.0 | 999999 | |
| 6 | 26 | 3 | 13 | -8.54 | 145.86 | -7.71 | 151.78 | 0.2818 | -1181.2 | -644.1 | |
| 0 | 3 | 0 | 2 | -8.19 | 144.29 | -9.28 | 146.49 | 0.2903 | -348.0 | -279.8 | |
| 0 | 3 | 0 | 2 | -7.95 | 144.06 | -9.51 | 145.35 | 0.2892 | -274.0 | -182.3 | |
| 0 | 25 | 0 | 13 | -8.61 | 143.92 | -9.65 | 146.23 | 0.2996 | 655.0 | 345.3 | |
| 0 | 5 | 0 | 3 | -9.07 | 143.38 | -10.19 | 145.63 | 0.3109 | 325.0 | 213.6 | |
| 0 | 6 | 0 | 3 | -8.42 | 142.83 | -10.74 | 142.97 | 0.3076 | 1073.0 | 852.8 | |
| 3 | 81 | 1 | 42 | -9.41 | 142.55 | -11.02 | 144.16 | 0.3234 | 951.5 | 972.4 | |
| 6 | -15 | 3 | -15 | -9.21 | 142.31 | -11.26 | 143.20 | 0.3231 | 1561.5 | 999999 | |
| 6 | -15 | 3 | -15 | -8.56 | 142.09 | -11.48 | 141.40 | 0.3169 | 1317.6 | 999999 | |
| 0 | 5 | 0 | 3 | -7.54 | 142.12 | -11.45 | 139.35 | 0.3035 | 367.0 | 475.0 | |
| 6 | -15 | 3 | -15 | -9.14 | 141.99 | -11.58 | 142.27 | 0.3254 | 1191.8 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. | |