| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.78 | 387.25 | 50.26 | 300.63 | -19.18 | 254.42 | 45.62 | 241.19 | 0.7725 | 857.4 | 265.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.89 | -20.04 | 268.05 | 59.24 | 245.18 | 0.8913 | 133.0 | 109.9 | |
| 0.00 | 1.45 | 0.00 | 1.38 | -20.78 | 262.97 | 54.17 | 242.79 | 0.8544 | 496.0 | 430.6 | |
| 0.00 | 0.64 | 0.00 | 0.53 | -23.09 | 256.71 | 47.90 | 237.69 | 0.8098 | -513.0 | -495.6 | |
| 61.23 | 371.81 | 47.54 | 288.24 | -19.07 | 254.43 | 45.63 | 241.34 | 0.7722 | 1110.8 | 280.6 | |
| 1.64 | -4.00 | 1.25 | -4.00 | -19.06 | 253.65 | 44.84 | 240.98 | 0.7644 | 1154.4 | 999999 | |
| 1.91 | 3.63 | 1.47 | 2.81 | -21.39 | 253.12 | 44.32 | 237.93 | 0.7699 | 736.0 | 562.3 | |
| 0.00 | 0.91 | 0.00 | 0.70 | -21.63 | 253.12 | 44.31 | 237.65 | 0.7710 | 558.0 | 470.3 | |
| 0.00 | 1.36 | 0.00 | 1.05 | -22.31 | 252.75 | 43.94 | 236.65 | 0.7707 | -431.0 | -349.4 | |
| 0.00 | 1.18 | 0.00 | 0.91 | -22.43 | 252.29 | 43.48 | 236.28 | 0.7670 | -510.0 | -432.4 | |
| 0.00 | 1.00 | 0.00 | 0.76 | -22.20 | 251.70 | 42.89 | 236.23 | 0.7604 | -636.0 | -544.3 | |
| 0.00 | 0.91 | 0.00 | 0.67 | -20.39 | 251.01 | 42.20 | 238.02 | 0.7446 | -633.0 | -367.4 | |
| 0.00 | 1.00 | 0.00 | 0.74 | -20.75 | 250.96 | 42.15 | 237.55 | 0.7459 | -365.0 | -323.2 | |
| 0.00 | 1.18 | 0.00 | 0.87 | -20.59 | 250.33 | 41.52 | 237.41 | 0.7389 | -636.0 | -514.6 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -26.62 | 251.64 | 42.84 | 231.12 | 0.7830 | -271.0 | -208.4 | |
| 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. | |