| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.71 | 309.55 | 79.53 | 466.28 | 15.47 | 60.43 | -71.64 | 75.87 | 0.9426 | -102.2 | 20.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.12 | 148.26 | 21.17 | 186.26 | 16.00 | 64.81 | -67.26 | 75.43 | 0.9177 | -717.5 | -91.3 | |
| 0.81 | -1.00 | 1.03 | -1.00 | 15.68 | 64.19 | -67.87 | 75.77 | 0.9218 | 74.7 | 999999 | |
| 6.40 | -1.00 | 8.14 | -1.00 | 15.51 | 64.06 | -68.01 | 75.95 | 0.9227 | -233.9 | 999999 | |
| 0.00 | 2.25 | 0.00 | 3.07 | 15.08 | 62.42 | -69.65 | 76.38 | 0.9330 | -8.0 | -63.1 | |
| 6.40 | 34.34 | 9.41 | 51.00 | 16.59 | 60.62 | -71.45 | 74.73 | 0.9433 | -398.3 | 123.2 | |
| 0.81 | -5.00 | 1.20 | -5.00 | 16.40 | 60.59 | -71.48 | 74.93 | 0.9435 | 219.2 | 999999 | |
| 0.00 | 1.71 | 0.00 | 2.63 | 17.26 | 59.78 | -72.28 | 74.00 | 0.9477 | -290.0 | -162.3 | |
| 6.04 | 8.74 | 8.62 | 12.46 | 15.00 | 61.36 | -70.71 | 76.44 | 0.9393 | 562.7 | 387.0 | |
| 0.00 | 15.77 | 0.00 | 23.72 | 14.91 | 60.24 | -71.83 | 76.50 | 0.9457 | 711.0 | 510.5 | |
| 0.00 | 3.06 | 0.00 | 4.88 | 15.35 | 59.11 | -72.95 | 75.99 | 0.9516 | 564.0 | 507.1 | |
| 0.00 | 1.17 | 0.00 | 1.94 | 16.05 | 58.33 | -73.74 | 75.22 | 0.9554 | 521.0 | 440.9 | |
| 0.00 | 3.06 | 0.00 | 6.15 | 18.76 | 54.88 | -77.19 | 72.28 | 0.9704 | 402.0 | 249.5 | |
| 1.26 | 3.33 | 2.07 | 5.45 | 15.47 | 58.45 | -73.62 | 75.84 | 0.9549 | 509.6 | 540.4 | |
| 0.90 | 10.54 | 1.81 | 20.96 | 18.03 | 54.94 | -77.13 | 73.04 | 0.9703 | -203.1 | 323.6 | |
| 1.53 | 2.88 | 2.58 | 4.86 | 15.51 | 57.95 | -74.12 | 75.78 | 0.9574 | 203.4 | 177.9 | |
| 0.00 | 1.53 | 0.00 | 3.15 | 17.74 | 54.62 | -77.45 | 73.32 | 0.9716 | -352.0 | -310.2 | |
| 8.38 | 72.91 | 15.71 | 139.75 | 14.07 | 56.31 | -75.76 | 77.20 | 0.9654 | 415.2 | -70.4 | |
| 4.06 | -17.00 | 7.79 | -17.00 | 14.11 | 55.86 | -76.20 | 77.13 | 0.9673 | -317.3 | 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. | |