| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.79 | 36.50 | 5.38 | 20.03 | 8.95 | 3.16 | 25.02 | 284.38 | 0.4332 | -112.3 | 37.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.61 | 7.14 | 2.01 | 3.98 | 8.09 | 5.06 | 26.92 | 281.65 | 0.4596 | -955.4 | -714.3 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 8.33 | 4.77 | 26.64 | 282.28 | 0.4559 | -833.0 | -607.2 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 8.40 | 4.54 | 26.41 | 282.51 | 0.4526 | -626.0 | -618.0 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 8.74 | 4.17 | 26.03 | 283.39 | 0.4478 | -742.0 | -595.7 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 8.05 | 4.02 | 25.88 | 281.94 | 0.4436 | -779.0 | -640.9 | |
| 0.34 | 2.07 | 0.19 | 1.14 | 8.89 | 4.04 | 25.91 | 283.78 | 0.4464 | -739.8 | -652.2 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 8.35 | 4.00 | 25.87 | 282.61 | 0.4442 | -887.0 | -687.0 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 9.31 | 4.04 | 25.91 | 284.70 | 0.4477 | 412.0 | 299.5 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 9.35 | 3.58 | 25.44 | 285.01 | 0.4408 | -700.0 | -532.7 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 9.68 | 3.54 | 25.40 | 285.76 | 0.4413 | 511.0 | 396.5 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 8.80 | 2.74 | 24.61 | 284.16 | 0.4262 | 512.0 | 323.9 | |
| 1.03 | 18.33 | 0.56 | 9.98 | 9.26 | 2.08 | 23.95 | 285.57 | 0.4176 | 920.0 | 545.8 | |
| 1.29 | -12.00 | 0.70 | -12.00 | 9.56 | 2.07 | 23.94 | 286.27 | 0.4186 | 712.9 | 999999 | |
| 2.75 | -12.00 | 1.50 | -12.00 | 9.39 | 1.99 | 23.86 | 285.90 | 0.4167 | 994.1 | 999999 | |
| 0.77 | -12.00 | 0.42 | -12.00 | 9.27 | 1.79 | 23.65 | 285.74 | 0.4131 | 1118.2 | 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. | |