| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.74 | 24.01 | 1.04 | 14.19 | -15.43 | 4.88 | 25.80 | 230.37 | 0.5464 | 55.5 | 240.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.63 | -15.57 | 7.15 | 28.06 | 232.56 | 0.5730 | 608.0 | 527.6 | |
| 0.00 | 0.78 | 0.00 | 0.47 | -15.36 | 6.73 | 27.65 | 232.45 | 0.5665 | 731.0 | 587.9 | |
| 1.74 | 6.96 | 1.04 | 4.16 | -14.88 | 6.49 | 27.40 | 232.93 | 0.5596 | 656.6 | 699.4 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -14.65 | 6.39 | 27.30 | 233.16 | 0.5566 | 537.0 | 533.4 | |
| 0.00 | 1.39 | 0.00 | 0.83 | -15.84 | 5.96 | 26.88 | 231.00 | 0.5618 | 591.0 | 565.8 | |
| 0.00 | 1.22 | 0.00 | 0.73 | -16.06 | 5.92 | 26.84 | 230.64 | 0.5633 | 797.0 | 695.4 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -16.34 | 5.62 | 26.53 | 229.93 | 0.5623 | 623.0 | 572.4 | |
| 0.00 | 2.87 | 0.00 | 1.69 | -15.25 | 4.77 | 25.69 | 230.62 | 0.5432 | 873.0 | 726.8 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -16.64 | 4.41 | 25.33 | 228.22 | 0.5518 | -537.0 | -458.1 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -15.66 | 3.22 | 24.14 | 228.27 | 0.5296 | -529.0 | -327.8 | |
| 0.00 | 1.39 | 0.00 | 0.81 | -15.94 | 3.12 | 24.04 | 227.74 | 0.5312 | -771.0 | -681.1 | |
| 0.00 | 1.57 | 0.00 | 0.90 | -15.26 | 1.85 | 22.77 | 227.23 | 0.5107 | -762.0 | -628.5 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -14.92 | 1.48 | 22.40 | 227.26 | 0.5033 | -695.0 | -585.1 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -15.74 | 1.07 | 21.99 | 225.53 | 0.5070 | -756.0 | -633.4 | |
| 0.00 | 1.22 | 0.00 | 0.70 | -16.23 | 0.66 | 21.58 | 224.28 | 0.5077 | -558.0 | -499.6 | |
| 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. | |