| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.18 | 108.63 | 18.20 | 98.42 | -20.89 | 56.67 | -50.61 | 120.44 | 0.8393 | 400.7 | 142.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.55 | -21.44 | 58.33 | -48.95 | 121.79 | 0.8280 | 482.0 | 403.4 | |
| 0.00 | 2.25 | 0.00 | 2.06 | -22.26 | 56.87 | -50.41 | 122.01 | 0.8431 | -584.0 | -411.2 | |
| 11.44 | 89.18 | 10.22 | 79.98 | -20.89 | 57.32 | -49.96 | 120.72 | 0.8341 | 825.6 | 235.0 | |
| 0.00 | 2.07 | 0.00 | 1.92 | -22.44 | 56.47 | -50.81 | 122.02 | 0.8470 | -598.0 | -508.9 | |
| 0.00 | 1.26 | 0.00 | 1.16 | -22.09 | 56.49 | -50.79 | 121.65 | 0.8455 | -319.0 | -287.5 | |
| 5.77 | -3.00 | 5.22 | -3.00 | -21.02 | 56.75 | -50.53 | 120.60 | 0.8393 | 480.7 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.88 | -18.95 | 56.65 | -50.63 | 118.27 | 0.8323 | 431.0 | 445.2 | |
| 0.00 | 1.35 | 0.00 | 1.20 | -18.72 | 56.54 | -50.74 | 117.98 | 0.8324 | 397.0 | 395.4 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -19.91 | 56.02 | -51.25 | 119.06 | 0.8411 | 359.0 | 300.0 | |
| 1.44 | 1.53 | 1.30 | 1.38 | -19.36 | 56.17 | -51.11 | 118.52 | 0.8379 | 407.0 | 369.0 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -18.87 | 56.07 | -51.21 | 117.94 | 0.8369 | 355.0 | 296.1 | |
| 1.17 | 1.89 | 1.09 | 1.77 | -19.69 | 54.87 | -52.41 | 118.33 | 0.8497 | 307.8 | 300.6 | |
| 0.00 | 0.54 | 0.00 | 0.54 | -20.59 | 52.83 | -54.45 | 118.50 | 0.8686 | -319.0 | -318.8 | |
| 0.36 | 5.86 | 0.37 | 6.00 | -20.79 | 51.52 | -55.76 | 118.21 | 0.8789 | -522.0 | -541.7 | |
| 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. | |