| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.47 | 57.77 | 13.71 | 39.30 | -17.47 | 123.63 | 41.85 | 248.43 | 0.6860 | 5.0 | -297.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.27 | 18.40 | 10.96 | 13.21 | -16.96 | 127.18 | 45.40 | 250.24 | 0.7260 | 718.6 | 482.3 | |
| 0.00 | 3.57 | 0.00 | 2.46 | -16.35 | 124.88 | 43.10 | 250.48 | 0.6979 | 740.0 | 589.2 | |
| 0.00 | 1.25 | 0.00 | 0.86 | -16.11 | 124.60 | 42.82 | 250.73 | 0.6940 | 726.0 | 657.9 | |
| 0.00 | 1.25 | 0.00 | 0.84 | -17.85 | 122.78 | 40.99 | 247.69 | 0.6772 | 587.0 | 524.0 | |
| 0.00 | 9.02 | 0.00 | 6.02 | -17.11 | 122.53 | 40.75 | 248.68 | 0.6720 | -818.0 | -628.7 | |
| 0.00 | 2.05 | 0.00 | 1.35 | -17.10 | 121.33 | 39.54 | 248.28 | 0.6573 | -493.0 | -484.9 | |
| 4.20 | 8.84 | 2.75 | 5.79 | -17.26 | 121.16 | 39.38 | 247.98 | 0.6559 | -736.6 | -637.8 | |
| 0.00 | 1.43 | 0.00 | 0.94 | -18.89 | 121.15 | 39.37 | 245.57 | 0.6614 | -554.0 | -473.3 | |
| 0.00 | 0.71 | 0.00 | 0.47 | -18.49 | 120.95 | 39.17 | 246.08 | 0.6576 | -533.0 | -437.5 | |
| 0.00 | 1.07 | 0.00 | 0.70 | -18.80 | 121.00 | 39.22 | 245.64 | 0.6593 | -533.0 | -499.8 | |
| 0.00 | 1.43 | 0.00 | 0.94 | -19.46 | 121.14 | 39.36 | 244.75 | 0.6635 | -545.0 | -458.8 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -17.91 | 120.59 | 38.81 | 246.80 | 0.6511 | -731.0 | -534.0 | |
| 0.00 | 1.79 | 0.00 | 1.17 | -18.66 | 120.75 | 38.97 | 245.76 | 0.6558 | -749.0 | -674.7 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -19.34 | 120.90 | 39.12 | 244.82 | 0.6602 | -639.0 | -530.3 | |
| 0.00 | 1.88 | 0.00 | 1.22 | -18.45 | 120.49 | 38.71 | 245.96 | 0.6518 | -714.0 | -588.9 | |
| 0.00 | 1.16 | 0.00 | 0.75 | -17.83 | 120.25 | 38.46 | 246.78 | 0.6466 | -722.0 | -605.1 | |
| 0.00 | 2.14 | 0.00 | 1.41 | -21.25 | 120.06 | 38.28 | 241.69 | 0.6581 | -729.0 | -545.5 | |
| 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. | |