| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.97 | 359.69 | 96.60 | 615.40 | -20.23 | 258.71 | -70.86 | 112.14 | 0.9578 | 92.8 | -96.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.09 | 22.26 | 8.37 | 30.61 | -21.17 | 263.49 | -66.08 | 113.97 | 0.9344 | 580.4 | 302.1 | |
| 1.00 | 126.47 | 1.44 | 198.22 | -21.35 | 262.50 | -67.07 | 113.96 | 0.9402 | 349.9 | -354.0 | |
| 3.73 | -2.00 | 5.43 | -2.00 | -21.23 | 262.09 | -67.48 | 113.76 | 0.9422 | 270.7 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.76 | -22.38 | 260.28 | -69.29 | 114.61 | 0.9527 | -387.0 | -406.6 | |
| 0.00 | 1.45 | 0.00 | 2.37 | -22.26 | 259.94 | -69.63 | 114.43 | 0.9542 | -468.0 | -487.8 | |
| 0.00 | 1.54 | 0.00 | 2.52 | -21.97 | 259.88 | -69.69 | 114.11 | 0.9542 | -509.0 | -484.5 | |
| 0.00 | 4.45 | 0.00 | 6.63 | -20.31 | 261.48 | -68.09 | 112.68 | 0.9445 | -249.0 | -187.5 | |
| 0.00 | 1.73 | 0.00 | 2.31 | -17.90 | 263.49 | -66.08 | 110.53 | 0.9304 | -96.0 | -110.2 | |
| 9.90 | -2.00 | 15.89 | -2.00 | -21.49 | 260.12 | -69.46 | 113.66 | 0.9526 | -535.5 | 999999 | |
| 3.09 | 5.09 | 5.20 | 8.55 | -22.16 | 259.38 | -70.19 | 114.22 | 0.9567 | -271.4 | -301.6 | |
| 0.00 | 1.00 | 0.00 | 1.84 | -23.13 | 257.87 | -71.70 | 114.96 | 0.9642 | 93.0 | 63.5 | |
| 0.00 | 8.72 | 0.00 | 15.68 | -22.32 | 258.17 | -71.40 | 114.18 | 0.9623 | 189.0 | 60.6 | |
| 3.00 | -2.00 | 5.23 | -2.00 | -21.67 | 258.54 | -71.03 | 113.57 | 0.9601 | -305.7 | 999999 | |
| 0.00 | 1.45 | 0.00 | 2.69 | -20.90 | 257.36 | -72.21 | 112.59 | 0.9647 | 248.0 | 193.9 | |
| 30.16 | 179.90 | 55.04 | 332.16 | -19.22 | 257.35 | -72.22 | 110.87 | 0.9635 | 292.6 | 34.7 | |
| 0.00 | 3.54 | 0.00 | 8.13 | -20.18 | 253.88 | -75.69 | 111.36 | 0.9776 | -159.0 | -189.8 | |
| 0.00 | 1.00 | 0.00 | 1.93 | -18.04 | 256.23 | -73.34 | 109.50 | 0.9675 | -190.0 | -164.5 | |
| 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. | |