| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.92 | 0.00 | 10.13 | 17.24 | 323.39 | 3.56 | 343.07 | 0.2234 | 891.5 | 681.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.09 | 0.00 | 1.05 | 13.14 | 325.96 | 6.13 | 322.87 | 0.1731 | 964.0 | 813.3 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 14.26 | 325.83 | 6.00 | 327.08 | 0.1874 | 863.0 | 745.4 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 13.87 | 325.39 | 5.56 | 327.87 | 0.1777 | 924.0 | 622.7 | |
| 0.00 | 4.35 | 0.00 | 2.22 | 17.82 | 324.94 | 5.11 | 338.71 | 0.2345 | 924.0 | 693.9 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 17.67 | 324.71 | 4.88 | 339.33 | 0.2307 | 869.0 | 643.7 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 17.94 | 324.53 | 4.70 | 340.45 | 0.2341 | 848.0 | 613.2 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 19.11 | 324.53 | 4.70 | 342.07 | 0.2527 | 676.0 | 375.5 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 18.92 | 324.30 | 4.47 | 342.65 | 0.2486 | 1051.0 | 802.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 18.04 | 324.12 | 4.29 | 342.15 | 0.2334 | 802.0 | 636.8 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 18.80 | 324.11 | 4.28 | 343.20 | 0.2457 | 947.0 | 760.7 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 12.39 | 321.53 | 1.70 | 346.80 | 0.1278 | 799.0 | 535.5 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 21.38 | 320.85 | 1.02 | 356.58 | 0.2791 | 930.0 | 653.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 19.89 | 320.05 | 0.22 | 359.20 | 0.2535 | 878.0 | 756.0 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 23.09 | 316.87 | -2.96 | 8.82 | 0.3110 | 842.0 | 659.4 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 15.76 | 315.95 | -3.88 | 19.69 | 0.1943 | 1056.0 | 807.9 | |
| 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. | |