| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 500 | 86 | 591 | -7.76 | 149.47 | 63.82 | 258.44 | 0.9074 | -65.1 | -107.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 148 | 23 | 205 | -8.09 | 153.93 | 68.28 | 258.97 | 0.9386 | -304.7 | -53.7 | |
| 13 | -1 | 17 | -1 | -7.66 | 152.93 | 67.28 | 259.24 | 0.9321 | -367.7 | 999999 | |
| 0 | 6 | 0 | 8 | -6.40 | 152.45 | 66.80 | 260.49 | 0.9277 | -491.0 | -386.5 | |
| 0 | 14 | 0 | 18 | -8.40 | 152.25 | 66.60 | 258.33 | 0.9287 | -176.0 | -192.6 | |
| 0 | 5 | 0 | 6 | -8.21 | 150.33 | 64.67 | 258.16 | 0.9158 | -168.0 | -229.1 | |
| 0 | 4 | 0 | 5 | -9.28 | 150.02 | 64.37 | 256.95 | 0.9151 | -274.0 | -235.0 | |
| 12 | 151 | 14 | 177 | -7.38 | 149.35 | 63.70 | 258.86 | 0.9079 | -932.2 | -426.2 | |
| 0 | 3 | 0 | 4 | -8.97 | 149.36 | 63.71 | 257.15 | 0.9101 | -230.0 | -353.9 | |
| 2 | 18 | 2 | 20 | -9.64 | 147.54 | 61.89 | 256.02 | 0.8980 | 315.0 | 25.9 | |
| 1 | 7 | 1 | 7 | -6.44 | 145.40 | 59.75 | 259.10 | 0.8761 | -213.5 | -198.2 | |
| 0 | 5 | 0 | 5 | -7.17 | 144.99 | 59.34 | 258.19 | 0.8739 | -77.0 | -21.2 | |
| 7 | 25 | 7 | 25 | -8.48 | 144.36 | 58.71 | 256.56 | 0.8710 | 289.0 | -25.9 | |
| 5 | 94 | 5 | 91 | -6.95 | 143.56 | 57.91 | 258.11 | 0.8614 | 834.5 | 322.2 | |
| 8 | -13 | 8 | -13 | -7.23 | 143.47 | 57.81 | 257.78 | 0.8611 | 871.7 | 999999 | |
| 8 | -13 | 7 | -13 | -7.46 | 143.36 | 57.71 | 257.49 | 0.8606 | 838.9 | 999999 | |
| 2 | 9 | 2 | 9 | -8.83 | 143.68 | 58.03 | 256.01 | 0.8659 | 643.9 | 502.9 | |
| 0 | 3 | 0 | 3 | -9.27 | 143.64 | 57.99 | 255.50 | 0.8664 | 503.0 | 403.8 | |
| 0 | 5 | 0 | 5 | -10.07 | 143.48 | 57.83 | 254.55 | 0.8666 | -245.0 | -148.5 | |
| 0 | 3 | 0 | 3 | -7.41 | 141.95 | 56.30 | 257.20 | 0.8481 | 383.0 | 344.1 | |
| 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. | |