| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.12 | 71.88 | 11.62 | 39.60 | 8.35 | 195.24 | -23.63 | 64.69 | 0.4401 | -109.6 | 49.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.58 | 7.29 | 197.21 | -21.65 | 65.18 | 0.4049 | -702.0 | -561.6 | |
| 0.00 | 2.34 | 0.00 | 1.27 | 8.49 | 197.08 | -21.78 | 62.64 | 0.4150 | -674.0 | -613.5 | |
| 9.88 | 25.51 | 5.37 | 13.87 | 8.06 | 197.04 | -21.82 | 63.63 | 0.4126 | -1127.9 | -730.7 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 7.44 | 196.94 | -21.92 | 65.09 | 0.4099 | -876.0 | -794.0 | |
| 2.25 | -3.00 | 1.22 | -3.00 | 7.78 | 196.82 | -22.04 | 64.45 | 0.4138 | -938.4 | 999999 | |
| 0.00 | 3.41 | 0.00 | 1.87 | 8.47 | 196.29 | -22.58 | 63.49 | 0.4261 | -904.0 | -573.4 | |
| 0.00 | 1.89 | 0.00 | 1.03 | 8.72 | 196.21 | -22.66 | 63.05 | 0.4290 | -570.0 | -427.7 | |
| 0.00 | 1.44 | 0.00 | 0.79 | 7.67 | 195.04 | -23.83 | 66.38 | 0.4388 | -680.0 | -460.9 | |
| 0.00 | 1.35 | 0.00 | 0.75 | 9.75 | 194.22 | -24.64 | 62.87 | 0.4637 | 657.0 | 579.5 | |
| 0.00 | 1.35 | 0.00 | 0.75 | 9.51 | 194.17 | -24.69 | 63.40 | 0.4627 | 834.0 | 695.4 | |
| 0.00 | 4.85 | 0.00 | 2.70 | 8.98 | 194.18 | -24.69 | 64.43 | 0.4592 | 885.0 | 889.6 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 9.10 | 194.10 | -24.76 | 64.25 | 0.4611 | 809.0 | 657.3 | |
| 1.80 | 3.95 | 1.00 | 2.21 | 9.02 | 193.73 | -25.13 | 64.74 | 0.4657 | 903.0 | 723.4 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 8.72 | 193.52 | -25.35 | 65.52 | 0.4668 | 722.0 | 598.5 | |
| 2.16 | 19.76 | 1.21 | 11.06 | 8.32 | 193.41 | -25.45 | 66.41 | 0.4660 | 1017.6 | 749.2 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 8.13 | 193.25 | -25.61 | 66.89 | 0.4671 | 549.0 | 493.3 | |
| 2.87 | -15.00 | 1.61 | -15.00 | 8.32 | 193.21 | -25.66 | 66.56 | 0.4689 | 955.9 | 999999 | |
| 2.16 | -15.00 | 1.21 | -15.00 | 8.57 | 193.16 | -25.71 | 66.11 | 0.4711 | 736.3 | 999999 | |
| 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. | |