| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65 | 267 | 37 | 151 | -5.60 | 81.11 | -25.72 | 115.77 | 0.4810 | -499.0 | -86.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19 | 82 | 10 | 45 | -5.91 | 84.13 | -22.71 | 119.21 | 0.4417 | -1411.1 | -733.4 | |
| 7 | -1 | 4 | -1 | -5.44 | 83.90 | -22.94 | 118.02 | 0.4414 | -1056.9 | 999999 | |
| 0 | 4 | 0 | 2 | -5.92 | 83.19 | -23.64 | 118.21 | 0.4546 | -875.0 | -744.2 | |
| 18 | 33 | 10 | 19 | -6.02 | 82.76 | -24.08 | 117.96 | 0.4613 | -1138.3 | -642.0 | |
| -4 | -4 | -4 | -4 | -6.11 | 82.49 | -24.34 | 117.87 | 0.4655 | 999999 | 999999 | |
| 3 | 21 | 2 | 12 | -6.62 | 82.08 | -24.76 | 118.40 | 0.4748 | -649.1 | -444.9 | |
| 0 | 3 | 0 | 2 | -5.02 | 81.98 | -24.85 | 115.27 | 0.4649 | -583.0 | -495.2 | |
| 0 | 4 | 0 | 2 | -6.28 | 81.66 | -25.17 | 117.36 | 0.4780 | -141.0 | -227.6 | |
| 0 | 7 | 0 | 4 | -3.76 | 80.99 | -25.85 | 111.93 | 0.4709 | 746.0 | 706.3 | |
| 0 | 4 | 0 | 2 | -4.60 | 79.47 | -27.37 | 112.32 | 0.4973 | 830.0 | 606.1 | |
| 0 | 4 | 0 | 2 | -5.39 | 78.99 | -27.85 | 113.38 | 0.5087 | 847.0 | 849.5 | |
| 0 | 4 | 0 | 3 | -5.76 | 78.88 | -27.95 | 113.95 | 0.5124 | 829.0 | 685.9 | |
| 0 | 2 | 0 | 1 | -5.77 | 78.61 | -28.22 | 113.77 | 0.5162 | 666.0 | 581.4 | |
| 6 | 99 | 4 | 57 | -5.06 | 78.47 | -28.36 | 112.39 | 0.5139 | 1283.0 | 563.2 | |
| 5 | -14 | 3 | -14 | -5.55 | 78.22 | -28.61 | 113.08 | 0.5202 | 770.4 | 999999 | |
| 7 | -14 | 4 | -14 | -5.17 | 78.07 | -28.77 | 112.27 | 0.5201 | 963.0 | 999999 | |
| 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. | |