| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 30.72 | 0.00 | 16.09 | 4.82 | 259.80 | -15.85 | 68.03 | 0.2923 | 177.4 | 199.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.35 | 0.00 | 1.17 | 5.33 | 273.76 | -1.89 | 19.66 | 0.0979 | -1043.0 | -816.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.18 | 273.46 | -2.19 | 23.15 | 0.0974 | -890.0 | -692.0 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 4.30 | 273.03 | -2.62 | 31.71 | 0.0871 | -956.0 | -780.1 | |
| 0.00 | 2.81 | 0.00 | 1.40 | 1.89 | 269.25 | -6.40 | 74.03 | 0.1164 | -958.0 | -801.5 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 2.87 | 269.06 | -6.59 | 66.90 | 0.1252 | -848.0 | -561.6 | |
| 0.00 | 1.27 | 0.00 | 0.63 | -3.00 | 268.99 | -6.66 | 114.83 | 0.1282 | -930.0 | -726.5 | |
| 0.00 | 2.44 | 0.00 | 1.27 | 8.04 | 260.30 | -15.35 | 62.10 | 0.2979 | 837.0 | 657.9 | |
| 0.00 | 4.80 | 0.00 | 2.48 | 5.65 | 259.65 | -16.00 | 70.46 | 0.2924 | 720.0 | 620.7 | |
| 0.00 | 2.44 | 0.00 | 1.27 | 5.62 | 259.04 | -16.61 | 71.19 | 0.3018 | 723.0 | 609.9 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 5.84 | 256.50 | -19.16 | 72.86 | 0.3431 | 543.0 | 589.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 9.65 | 255.89 | -19.76 | 63.45 | 0.3741 | 784.0 | 639.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -0.44 | 254.38 | -21.27 | 91.37 | 0.3643 | 858.0 | 786.5 | |
| 0.00 | 2.72 | 0.00 | 1.49 | 9.34 | 252.09 | -23.56 | 67.76 | 0.4279 | 768.0 | 589.6 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 9.19 | 249.35 | -26.30 | 70.06 | 0.4672 | 699.0 | 538.9 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 8.76 | 249.38 | -26.27 | 70.92 | 0.4647 | 764.0 | 588.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -0.46 | 249.63 | -26.02 | 91.19 | 0.4406 | 693.0 | 553.8 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 1.15 | 248.09 | -27.56 | 87.64 | 0.4648 | 656.0 | 423.5 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -0.19 | 246.33 | -29.32 | 90.50 | 0.4917 | 774.0 | 647.2 | |
| 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. | |