| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.28 | 37.44 | 6.90 | 30.22 | 15.70 | 54.18 | 52.44 | 284.64 | 0.7894 | -15.9 | -48.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.54 | 0.00 | 0.49 | 15.22 | 59.46 | 57.73 | 283.69 | 0.8418 | -249.0 | -345.2 | |
| 0.00 | 1.35 | 0.00 | 1.23 | 15.53 | 59.48 | 57.75 | 284.06 | 0.8420 | -420.0 | -337.5 | |
| 4.95 | 7.38 | 4.41 | 6.58 | 14.72 | 58.61 | 56.87 | 283.11 | 0.8338 | -629.3 | -395.2 | |
| 0.00 | 1.53 | 0.00 | 1.36 | 14.27 | 58.43 | 56.69 | 282.58 | 0.8320 | -636.0 | -494.9 | |
| 0.00 | 1.17 | 0.00 | 0.96 | 14.05 | 55.21 | 53.47 | 282.42 | 0.8004 | 337.0 | 228.6 | |
| 0.00 | 0.99 | 0.00 | 0.81 | 16.09 | 54.74 | 53.00 | 285.00 | 0.7967 | -548.0 | -483.4 | |
| 0.00 | 6.66 | 0.00 | 5.40 | 16.02 | 54.50 | 52.76 | 284.93 | 0.7942 | -856.0 | -628.3 | |
| 0.00 | 0.63 | 0.00 | 0.54 | 21.48 | 56.17 | 54.44 | 291.52 | 0.8159 | -355.0 | -370.6 | |
| 0.00 | 1.26 | 0.00 | 0.95 | 14.62 | 51.15 | 49.41 | 283.39 | 0.7576 | 605.0 | 502.5 | |
| 0.00 | 2.52 | 0.00 | 1.92 | 15.92 | 51.57 | 49.83 | 285.06 | 0.7633 | 303.0 | 277.3 | |
| 1.89 | 3.42 | 1.43 | 2.60 | 15.85 | 51.30 | 49.56 | 284.99 | 0.7603 | 631.0 | 465.5 | |
| 0.00 | 1.08 | 0.00 | 0.82 | 16.18 | 51.41 | 49.68 | 285.42 | 0.7618 | 409.0 | 356.8 | |
| 0.00 | 1.44 | 0.00 | 1.07 | 15.00 | 50.40 | 48.66 | 283.95 | 0.7496 | 657.0 | 495.5 | |
| 0.00 | 0.90 | 0.00 | 0.67 | 16.42 | 50.09 | 48.36 | 285.89 | 0.7476 | 529.0 | 430.5 | |
| 0.72 | 5.31 | 0.53 | 3.92 | 16.14 | 49.76 | 48.02 | 285.55 | 0.7436 | 760.8 | 616.8 | |
| 0.72 | -15.00 | 0.53 | -15.00 | 16.22 | 49.60 | 47.86 | 285.67 | 0.7418 | 738.6 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.34 | 19.23 | 50.55 | 48.81 | 289.55 | 0.7563 | 454.0 | 373.6 | |
| 0.00 | 0.81 | 0.00 | 0.56 | 19.70 | 45.04 | 43.30 | 291.34 | 0.6955 | 517.0 | 369.3 | |
| 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. | |