| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89 | 488 | 55 | 303 | -22.92 | 305.17 | 27.00 | 222.99 | 0.6147 | -957.3 | -493.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 4 | -24.11 | 312.02 | 33.84 | 227.74 | 0.6892 | -459.0 | -351.7 | |
| 0 | 4 | 0 | 2 | -20.67 | 310.68 | 32.51 | 230.90 | 0.6504 | -489.0 | -400.5 | |
| 18 | 100 | 11 | 64 | -22.51 | 307.49 | 29.32 | 225.82 | 0.6331 | -1403.4 | -627.3 | |
| 0 | 8 | 0 | 5 | -22.75 | 305.93 | 27.76 | 224.03 | 0.6203 | -700.0 | -672.1 | |
| 17 | 205 | 11 | 130 | -23.96 | 305.83 | 27.66 | 222.49 | 0.6303 | -1144.9 | -459.1 | |
| 24 | -5 | 15 | -5 | -23.86 | 305.43 | 27.25 | 222.21 | 0.6257 | -1294.7 | 999999 | |
| 0 | 9 | 0 | 5 | -22.03 | 304.98 | 26.81 | 223.96 | 0.6046 | -640.0 | -410.8 | |
| -6 | -5 | -6 | -5 | -23.62 | 304.95 | 26.78 | 222.00 | 0.6191 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | -21.74 | 303.95 | 25.78 | 223.25 | 0.5919 | 374.0 | 263.3 | |
| 5 | 53 | 3 | 33 | -22.59 | 303.80 | 25.62 | 222.03 | 0.5986 | -1165.0 | -822.1 | |
| 0 | 4 | 0 | 2 | -20.23 | 303.26 | 25.09 | 224.43 | 0.5706 | -668.0 | -616.2 | |
| 0 | 8 | 0 | 5 | -24.46 | 303.91 | 25.74 | 219.95 | 0.6178 | -288.0 | -200.2 | |
| 14 | 52 | 8 | 31 | -20.89 | 302.74 | 24.57 | 223.00 | 0.5719 | -1167.7 | -798.0 | |
| 0 | 6 | 0 | 3 | -23.08 | 302.83 | 24.66 | 220.40 | 0.5944 | 444.0 | 318.7 | |
| 5 | 27 | 3 | 16 | -22.17 | 299.99 | 21.81 | 218.15 | 0.5593 | 855.1 | 635.4 | |
| 6 | -15 | 4 | -15 | -22.17 | 299.67 | 21.50 | 217.76 | 0.5564 | 1005.6 | 999999 | |
| 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. | |