| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.55 | 232.32 | 47.63 | 234.37 | -14.85 | 117.56 | -57.20 | 111.15 | 0.8718 | 180.2 | 95.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.84 | 127.40 | 6.35 | 119.26 | -15.20 | 120.72 | -54.04 | 112.53 | 0.8478 | 847.3 | 256.0 | |
| 0.00 | 2.19 | 0.00 | 2.02 | -13.66 | 120.58 | -54.18 | 110.74 | 0.8446 | -116.0 | -51.5 | |
| 19.04 | -1.00 | 17.95 | -1.00 | -14.91 | 120.02 | -54.73 | 111.97 | 0.8529 | 686.5 | 999999 | |
| 0.00 | 1.14 | 0.00 | 1.10 | -15.30 | 119.26 | -55.49 | 112.15 | 0.8602 | -368.0 | -339.8 | |
| 0.00 | 2.28 | 0.00 | 2.19 | -14.14 | 119.16 | -55.59 | 110.82 | 0.8580 | 662.0 | 423.0 | |
| 0.00 | 0.88 | 0.00 | 0.84 | -13.99 | 119.05 | -55.70 | 110.62 | 0.8585 | 549.0 | 387.9 | |
| 1.23 | 2.11 | 1.19 | 2.03 | -13.95 | 118.79 | -55.96 | 110.49 | 0.8606 | 444.0 | 379.1 | |
| 3.07 | 15.09 | 2.99 | 14.72 | -13.73 | 118.48 | -56.27 | 110.14 | 0.8626 | 540.6 | 98.0 | |
| 2.11 | -8.00 | 2.07 | -8.00 | -13.60 | 118.14 | -56.62 | 109.90 | 0.8651 | 316.2 | 999999 | |
| 0.00 | 1.05 | 0.00 | 1.04 | -13.37 | 117.66 | -57.10 | 109.49 | 0.8685 | -486.0 | -334.3 | |
| 4.30 | 9.91 | 4.52 | 10.44 | -15.13 | 116.18 | -58.58 | 110.97 | 0.8842 | -564.7 | -439.0 | |
| 0.00 | 1.14 | 0.00 | 1.24 | -15.46 | 115.11 | -59.64 | 111.01 | 0.8928 | -248.0 | -183.4 | |
| 0.00 | 1.32 | 0.00 | 1.48 | -15.62 | 114.15 | -60.60 | 110.91 | 0.9001 | -425.0 | -450.3 | |
| 0.00 | 1.05 | 0.00 | 1.20 | -15.52 | 113.88 | -60.87 | 110.72 | 0.9018 | -449.0 | -407.8 | |
| 0.00 | 5.26 | 0.00 | 6.06 | -15.47 | 113.45 | -61.30 | 110.55 | 0.9047 | 230.0 | -23.5 | |
| 1.75 | 61.50 | 1.99 | 70.75 | -14.59 | 113.62 | -61.13 | 109.66 | 0.9018 | -602.2 | -71.2 | |
| 9.21 | -16.00 | 10.57 | -16.00 | -14.90 | 113.41 | -61.34 | 109.93 | 0.9038 | -557.9 | 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. | |