| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 112.05 | 519.10 | 138.60 | 635.41 | 15.58 | 9.67 | -66.28 | 74.66 | 0.9139 | 46.5 | 182.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.39 | 147.61 | 32.53 | 148.09 | 15.12 | 15.52 | -60.43 | 74.84 | 0.8719 | -666.4 | -248.5 | |
| 0.00 | 0.26 | 0.00 | 0.29 | 18.83 | 12.52 | -63.43 | 70.90 | 0.8977 | -275.0 | -247.3 | |
| 1.30 | -1.00 | 1.33 | -1.00 | 14.61 | 14.68 | -61.27 | 75.48 | 0.8785 | -250.8 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.33 | 14.24 | 14.72 | -61.23 | 75.89 | 0.8780 | -503.0 | -410.8 | |
| 0.00 | 1.64 | 0.00 | 1.70 | 14.11 | 14.53 | -61.42 | 76.06 | 0.8795 | -227.0 | -170.3 | |
| 0.00 | 1.12 | 0.00 | 1.17 | 14.64 | 14.14 | -61.80 | 75.48 | 0.8828 | 251.0 | 224.6 | |
| 0.00 | 1.55 | 0.00 | 1.63 | 14.85 | 14.04 | -61.91 | 75.25 | 0.8837 | 274.0 | 236.9 | |
| 0.00 | 2.42 | 0.00 | 2.53 | 14.43 | 14.18 | -61.77 | 75.72 | 0.8824 | 370.0 | 295.5 | |
| 1.21 | 2.76 | 1.32 | 3.02 | 14.60 | 12.89 | -63.05 | 75.61 | 0.8925 | -409.8 | -212.9 | |
| 0.00 | 1.47 | 0.00 | 1.82 | 18.54 | 9.59 | -66.35 | 71.47 | 0.9177 | 520.0 | 558.5 | |
| 2.42 | 5.27 | 2.79 | 6.08 | 15.97 | 11.28 | -64.67 | 74.17 | 0.9050 | 401.2 | 417.0 | |
| 0.00 | 1.99 | 0.00 | 2.23 | 14.48 | 12.05 | -63.90 | 75.78 | 0.8988 | 383.0 | 345.7 | |
| 0.00 | 1.12 | 0.00 | 1.38 | 18.16 | 9.56 | -66.38 | 71.88 | 0.9178 | 585.0 | 479.4 | |
| 4.23 | 252.90 | 5.00 | 316.03 | 15.07 | 10.56 | -65.39 | 75.21 | 0.9098 | 868.0 | 330.3 | |
| 8.90 | -14.00 | 10.34 | -14.00 | 14.36 | 10.97 | -64.98 | 75.97 | 0.9067 | -107.8 | 999999 | |
| 11.57 | -14.00 | 14.06 | -14.00 | 15.18 | 9.81 | -66.13 | 75.12 | 0.9150 | 667.5 | 999999 | |
| 0.00 | 0.95 | 0.00 | 1.22 | 16.98 | 8.52 | -67.43 | 73.23 | 0.9241 | 418.0 | 462.6 | |
| 0.00 | 0.95 | 0.00 | 1.24 | 17.08 | 8.11 | -67.84 | 73.14 | 0.9267 | 266.0 | 271.4 | |
| 5.53 | -14.00 | 6.82 | -14.00 | 14.72 | 9.39 | -66.55 | 75.64 | 0.9177 | -248.3 | 999999 | |
| 5.79 | -14.00 | 7.63 | -14.00 | 16.66 | 7.84 | -68.11 | 73.61 | 0.9282 | 699.4 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.06 | 14.11 | 9.44 | -66.50 | 76.30 | 0.9172 | -193.0 | -199.6 | |
| 3.63 | -14.00 | 4.57 | -14.00 | 14.75 | 8.90 | -67.05 | 75.62 | 0.9209 | -149.5 | 999999 | |
| 1.99 | -14.00 | 2.69 | -14.00 | 17.05 | 7.19 | -68.75 | 73.21 | 0.9323 | 253.6 | 999999 | |
| 7.95 | -14.00 | 10.77 | -14.00 | 16.21 | 7.15 | -68.80 | 74.11 | 0.9324 | -109.8 | 999999 | |
| 0.00 | 1.04 | 0.00 | 1.35 | 14.36 | 7.93 | -68.02 | 76.09 | 0.9271 | 375.0 | 330.3 | |
| 0.00 | 0.95 | 0.00 | 1.39 | 17.10 | 5.53 | -70.42 | 73.22 | 0.9420 | 476.0 | 448.1 | |
| 1.99 | 10.62 | 2.68 | 14.26 | 14.89 | 7.15 | -68.79 | 75.53 | 0.9321 | 411.5 | 230.8 | |
| 0.00 | 0.60 | 0.00 | 0.94 | 17.98 | 4.22 | -71.73 | 72.34 | 0.9493 | 159.0 | 107.6 | |
| 5.27 | 9.33 | 7.66 | 13.59 | 15.93 | 5.57 | -70.38 | 74.47 | 0.9416 | -206.4 | 42.9 | |
| 2.42 | 13.39 | 3.44 | 18.95 | 15.13 | 6.01 | -69.94 | 75.31 | 0.9389 | 500.8 | 392.7 | |
| 0.00 | 1.04 | 0.00 | 1.65 | 17.67 | 3.71 | -72.24 | 72.68 | 0.9519 | 258.0 | 206.8 | |
| 0.00 | 0.43 | 0.00 | 0.59 | 13.38 | 7.02 | -68.93 | 77.16 | 0.9327 | -264.0 | -213.6 | |
| 0.00 | 1.47 | 0.00 | 2.14 | 15.43 | 5.41 | -70.54 | 75.01 | 0.9424 | -179.0 | -132.6 | |
| 13.21 | 51.74 | 21.21 | 82.50 | 17.14 | 3.61 | -72.33 | 73.24 | 0.9523 | 479.3 | 394.3 | |
| 0.00 | 1.21 | 0.00 | 2.02 | 17.71 | 2.82 | -73.13 | 72.66 | 0.9563 | -385.0 | -323.1 | |
| 0.00 | 3.11 | 0.00 | 5.21 | 17.46 | 2.76 | -73.19 | 72.93 | 0.9566 | -437.0 | -357.3 | |
| 2.25 | -34.00 | 3.76 | -34.00 | 16.99 | 2.80 | -73.15 | 73.41 | 0.9563 | 121.1 | 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. | |