| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.19 | 0.00 | 12.05 | 5.25 | 259.64 | -12.18 | 152.75 | 0.2574 | 55.1 | 37.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.39 | 274.08 | 2.27 | 336.87 | 0.1008 | -849.0 | -558.4 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 5.02 | 273.93 | 2.11 | 336.84 | 0.0938 | -874.0 | -642.2 | |
| 0.00 | 2.26 | 0.00 | 1.13 | 5.21 | 273.62 | 1.81 | 340.56 | 0.0949 | -906.0 | -719.2 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 4.23 | 273.25 | 1.44 | 340.84 | 0.0767 | -1034.0 | -823.7 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 1.98 | 269.26 | -2.55 | 53.55 | 0.0556 | -1123.0 | -961.6 | |
| 0.00 | 1.36 | 0.00 | 0.67 | 0.92 | 267.64 | -4.17 | 78.83 | 0.0744 | -933.0 | -655.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 4.03 | 259.78 | -12.04 | 71.73 | 0.2200 | 859.0 | 653.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 9.89 | 256.36 | -15.46 | 57.06 | 0.3143 | 743.0 | 610.6 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 8.85 | 252.66 | -19.15 | 64.86 | 0.3597 | 630.0 | 612.1 | |
| 0.00 | 2.35 | 0.00 | 1.25 | 9.31 | 252.41 | -19.41 | 63.97 | 0.3665 | 849.0 | 621.7 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 5.66 | 250.48 | -21.33 | 75.00 | 0.3764 | 769.0 | 526.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -0.37 | 249.80 | -22.02 | 91.24 | 0.3766 | 861.0 | 556.7 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 9.00 | 248.75 | -23.06 | 68.18 | 0.4185 | 397.0 | 279.3 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -0.28 | 246.44 | -25.38 | 90.86 | 0.4304 | 794.0 | 633.6 | |
| 0.00 | 1.72 | 0.00 | 0.99 | 6.89 | 241.45 | -30.36 | 76.72 | 0.5176 | 644.0 | 541.3 | |
| 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. | |