| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.07 | 98.24 | 20.38 | 81.42 | -10.32 | 187.71 | 53.45 | 260.67 | 0.8026 | 74.6 | 173.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.77 | -10.70 | 189.82 | 55.55 | 260.30 | 0.8242 | 215.0 | 228.9 | |
| 5.96 | 48.27 | 5.11 | 41.45 | -10.10 | 189.28 | 55.01 | 261.02 | 0.8188 | 598.3 | 245.1 | |
| 2.58 | -2.00 | 2.20 | -2.00 | -10.15 | 188.97 | 54.70 | 260.95 | 0.8157 | 799.2 | 999999 | |
| 4.89 | 17.96 | 4.13 | 15.15 | -9.68 | 188.64 | 54.38 | 261.52 | 0.8123 | 909.5 | 455.2 | |
| 0.00 | 1.51 | 0.00 | 1.25 | -10.90 | 187.84 | 53.58 | 259.99 | 0.8046 | 566.0 | 537.3 | |
| 0.00 | 1.60 | 0.00 | 1.34 | -13.02 | 188.14 | 53.88 | 257.37 | 0.8087 | 354.0 | 364.0 | |
| 0.00 | 0.89 | 0.00 | 0.72 | -10.46 | 186.61 | 52.34 | 260.48 | 0.7916 | 156.0 | 233.3 | |
| 0.00 | 1.33 | 0.00 | 1.04 | -9.44 | 184.95 | 50.68 | 261.73 | 0.7735 | -302.0 | -349.4 | |
| 0.71 | 3.29 | 0.55 | 2.56 | -10.75 | 184.84 | 50.58 | 260.01 | 0.7729 | -547.5 | -498.5 | |
| 0.80 | 1.87 | 0.62 | 1.44 | -11.10 | 184.63 | 50.37 | 259.55 | 0.7708 | -338.3 | -267.1 | |
| 8.09 | 10.67 | 6.23 | 8.21 | -10.78 | 184.37 | 50.10 | 259.95 | 0.7677 | -811.3 | -459.7 | |
| 0.00 | 0.89 | 0.00 | 0.69 | -12.31 | 184.40 | 50.14 | 257.96 | 0.7691 | -476.0 | -449.8 | |
| 0.00 | 0.89 | 0.00 | 0.67 | -10.43 | 183.10 | 48.84 | 260.33 | 0.7534 | -488.0 | -509.0 | |
| 0.00 | 2.84 | 0.00 | 2.13 | -10.63 | 182.96 | 48.69 | 260.06 | 0.7518 | -709.0 | -562.7 | |
| 0.00 | 0.98 | 0.00 | 0.73 | -11.14 | 182.98 | 48.71 | 259.37 | 0.7524 | -426.0 | -464.2 | |
| 2.04 | 3.56 | 1.54 | 2.67 | -12.27 | 183.01 | 48.74 | 257.87 | 0.7536 | 426.3 | 466.3 | |
| 0.00 | 0.80 | 0.00 | 0.60 | -11.04 | 182.63 | 48.36 | 259.48 | 0.7484 | -286.0 | -286.4 | |
| 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. | |