| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.28 | 111.99 | 33.33 | 69.19 | -12.40 | 177.31 | -31.52 | 121.21 | 0.5988 | 437.8 | -195.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.66 | 74.95 | 27.87 | 45.80 | -12.28 | 178.30 | -30.53 | 121.82 | 0.5863 | 976.4 | 221.9 | |
| 1.41 | -1.00 | 0.86 | -1.00 | -12.80 | 178.05 | -30.78 | 122.37 | 0.5930 | 473.6 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -13.03 | 177.98 | -30.84 | 122.64 | 0.5954 | 484.0 | 293.5 | |
| 0.44 | -1.00 | 0.27 | -1.00 | -12.24 | 177.88 | -30.95 | 121.41 | 0.5911 | -157.2 | 999999 | |
| 0.79 | -1.00 | 0.49 | -1.00 | -12.00 | 177.76 | -31.06 | 120.95 | 0.5907 | 390.9 | 999999 | |
| 0.00 | 2.46 | 0.00 | 1.53 | -12.98 | 177.23 | -31.59 | 121.95 | 0.6039 | -739.0 | -611.8 | |
| 0.62 | 3.17 | 0.38 | 1.97 | -13.13 | 176.92 | -31.91 | 121.91 | 0.6086 | 566.9 | 188.5 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -11.98 | 177.05 | -31.78 | 120.35 | 0.5993 | -519.0 | -418.6 | |
| 0.00 | 3.08 | 0.00 | 1.92 | -12.13 | 176.26 | -32.56 | 119.95 | 0.6096 | -808.0 | -683.6 | |
| 0.00 | 7.74 | 0.00 | 4.82 | -11.39 | 176.00 | -32.83 | 118.68 | 0.6080 | -975.0 | -737.6 | |
| 0.00 | 1.23 | 0.00 | 0.77 | -11.49 | 175.80 | -33.03 | 118.69 | 0.6111 | -457.0 | -453.9 | |
| 0.00 | 2.20 | 0.00 | 1.41 | -13.62 | 174.78 | -34.04 | 120.95 | 0.6367 | -729.0 | -591.2 | |
| 0.00 | 1.32 | 0.00 | 0.84 | -12.51 | 174.81 | -34.02 | 119.42 | 0.6293 | -700.0 | -563.3 | |
| 3.34 | 7.74 | 2.16 | 4.99 | -13.78 | 174.27 | -34.56 | 120.80 | 0.6437 | -716.8 | -666.4 | |
| 2.02 | 3.69 | 1.30 | 2.37 | -12.70 | 174.33 | -34.49 | 119.35 | 0.6361 | -858.3 | -686.3 | |
| 0.00 | 1.06 | 0.00 | 0.67 | -11.51 | 174.10 | -34.73 | 117.51 | 0.6317 | -695.0 | -453.8 | |
| 0.00 | 1.32 | 0.00 | 0.85 | -12.27 | 173.57 | -35.25 | 118.23 | 0.6424 | -702.0 | -500.0 | |
| 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. | |