| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.40 | 51.10 | 15.45 | 38.13 | -12.34 | 116.89 | -47.89 | 103.73 | 0.7470 | 452.6 | 129.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.57 | -15.31 | 123.94 | -40.84 | 109.45 | 0.6713 | 615.0 | 458.8 | |
| 0.00 | 0.76 | 0.00 | 0.52 | -8.50 | 121.99 | -42.79 | 99.04 | 0.6827 | 653.0 | 518.9 | |
| 0.00 | 1.19 | 0.00 | 0.87 | -17.89 | 118.78 | -46.00 | 111.50 | 0.7381 | 497.0 | 358.5 | |
| 0.00 | 1.27 | 0.00 | 0.92 | -15.08 | 118.63 | -46.15 | 107.70 | 0.7333 | 369.0 | 398.6 | |
| 0.00 | 0.59 | 0.00 | 0.43 | -14.42 | 118.68 | -46.10 | 106.82 | 0.7314 | 571.0 | 538.1 | |
| 9.34 | 20.81 | 6.63 | 14.80 | -11.35 | 119.33 | -45.46 | 102.73 | 0.7188 | 925.5 | 569.8 | |
| 2.46 | -6.00 | 1.76 | -6.00 | -11.34 | 119.03 | -45.76 | 102.67 | 0.7223 | 543.7 | 999999 | |
| 0.00 | 1.10 | 0.00 | 0.79 | -11.69 | 118.95 | -45.83 | 103.15 | 0.7237 | 257.0 | 267.3 | |
| 0.00 | 1.10 | 0.00 | 0.81 | -14.36 | 117.94 | -46.84 | 106.58 | 0.7397 | 408.0 | 358.3 | |
| 9.60 | 12.99 | 7.06 | 9.56 | -12.32 | 117.49 | -47.30 | 103.77 | 0.7415 | 700.1 | 398.8 | |
| 0.00 | 0.93 | 0.00 | 0.74 | -13.39 | 113.62 | -51.17 | 104.57 | 0.7853 | 549.0 | 466.7 | |
| 0.00 | 0.25 | 0.00 | 0.21 | -12.00 | 112.74 | -52.04 | 102.70 | 0.7928 | 230.0 | 220.0 | |
| 0.00 | 3.74 | 0.00 | 3.14 | -13.92 | 111.30 | -53.48 | 104.92 | 0.8096 | -732.0 | -581.7 | |
| 0.00 | 2.55 | 0.00 | 2.12 | -12.36 | 111.39 | -53.39 | 103.00 | 0.8070 | -710.0 | -549.5 | |
| 0.00 | 1.44 | 0.00 | 1.22 | -11.77 | 110.95 | -53.84 | 102.23 | 0.8109 | -502.0 | -435.5 | |
| 0.00 | 0.85 | 0.00 | 0.79 | -12.98 | 107.15 | -57.63 | 103.33 | 0.8480 | -475.0 | -372.9 | |
| 0.00 | 0.68 | 0.00 | 0.64 | -13.02 | 106.79 | -57.99 | 103.35 | 0.8512 | -437.0 | -377.0 | |
| 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. | |