| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 30.32 | 0.00 | 17.79 | -23.61 | 74.19 | 7.46 | 193.47 | 0.5374 | 91.2 | 72.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.78 | 0.00 | 1.04 | -21.00 | 82.16 | 15.43 | 207.91 | 0.5326 | 560.0 | 509.4 | |
| 0.00 | 4.00 | 0.00 | 2.30 | -19.40 | 81.90 | 15.17 | 209.06 | 0.5100 | 811.0 | 623.2 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -20.68 | 79.73 | 13.00 | 204.35 | 0.5124 | 749.0 | 685.9 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -20.54 | 79.62 | 12.89 | 204.28 | 0.5099 | 693.0 | 577.4 | |
| 0.00 | 1.42 | 0.00 | 0.84 | -23.13 | 79.69 | 12.96 | 202.31 | 0.5452 | 707.0 | 653.6 | |
| 0.00 | 1.25 | 0.00 | 0.73 | -23.12 | 79.21 | 12.48 | 201.59 | 0.5424 | 707.0 | 597.1 | |
| 0.00 | 1.33 | 0.00 | 0.78 | -22.20 | 78.83 | 12.10 | 201.66 | 0.5279 | 770.0 | 646.6 | |
| 0.00 | 2.76 | 0.00 | 1.63 | -23.78 | 78.97 | 12.24 | 200.74 | 0.5501 | 707.0 | 455.0 | |
| 0.00 | 2.31 | 0.00 | 1.35 | -23.46 | 76.50 | 9.77 | 197.01 | 0.5340 | 729.0 | 598.7 | |
| 0.00 | 0.98 | 0.00 | 0.58 | -25.09 | 74.97 | 8.24 | 193.67 | 0.5511 | 700.0 | 604.5 | |
| 0.00 | 1.42 | 0.00 | 0.83 | -24.01 | 68.89 | 2.16 | 183.80 | 0.5217 | -894.0 | -744.8 | |
| 0.00 | 2.31 | 0.00 | 1.36 | -25.08 | 68.78 | 2.05 | 183.46 | 0.5374 | -572.0 | -554.7 | |
| 0.00 | 2.76 | 0.00 | 1.60 | -24.40 | 68.30 | 1.57 | 182.73 | 0.5270 | -774.0 | -694.1 | |
| 0.00 | 1.07 | 0.00 | 0.63 | -26.08 | 68.32 | 1.59 | 182.60 | 0.5518 | -587.0 | -420.6 | |
| 0.00 | 0.71 | 0.00 | 0.42 | -25.43 | 68.28 | 1.55 | 182.59 | 0.5423 | -635.0 | -529.6 | |
| 0.00 | 1.33 | 0.00 | 0.76 | -22.92 | 66.68 | -0.05 | 179.91 | 0.5041 | -728.0 | -594.9 | |
| 0.00 | 1.25 | 0.00 | 0.74 | -26.37 | 66.48 | -0.26 | 179.58 | 0.5554 | -755.0 | -608.7 | |
| 0.00 | 2.22 | 0.00 | 1.38 | -29.67 | 63.27 | -3.47 | 175.00 | 0.6047 | -547.0 | -505.4 | |
| 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. | |