| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.95 | 209.70 | 46.44 | 207.06 | 7.74 | 129.56 | -59.72 | 81.72 | 0.8658 | -166.3 | -110.3 | |
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back to the solar disc SDO HMI 2011-11-29 05:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.74 | 0.00 | 2.54 | 9.17 | 131.71 | -57.57 | 79.88 | 0.8485 | 417.0 | 337.9 | |
| 2.31 | 108.35 | 2.14 | 100.19 | 8.63 | 131.79 | -57.49 | 80.51 | 0.8474 | 350.1 | -285.8 | |
| 20.87 | -2.00 | 19.32 | -2.00 | 7.53 | 131.76 | -57.52 | 81.82 | 0.8470 | -763.6 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.80 | 5.47 | 131.35 | -57.93 | 84.27 | 0.8499 | -403.0 | -419.5 | |
| 2.31 | 16.25 | 2.20 | 15.50 | 6.32 | 130.75 | -58.53 | 83.30 | 0.8557 | -537.8 | -443.3 | |
| 0.00 | 2.65 | 0.00 | 2.54 | 7.09 | 130.54 | -58.74 | 82.41 | 0.8579 | -490.0 | -376.3 | |
| 2.39 | -5.00 | 2.29 | -5.00 | 6.64 | 130.52 | -58.76 | 82.93 | 0.8579 | -384.8 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.91 | 7.74 | 130.17 | -59.11 | 81.68 | 0.8615 | -325.0 | -307.5 | |
| 1.97 | 4.10 | 1.91 | 3.98 | 7.11 | 130.13 | -59.15 | 82.41 | 0.8615 | -246.1 | -190.8 | |
| 1.54 | 5.30 | 1.51 | 5.19 | 7.43 | 129.71 | -59.57 | 82.06 | 0.8654 | -337.2 | -171.0 | |
| 0.00 | 0.86 | 0.00 | 0.85 | 7.37 | 129.48 | -59.80 | 82.15 | 0.8673 | 138.0 | 16.4 | |
| 1.88 | 4.10 | 1.87 | 4.08 | 6.95 | 129.21 | -60.07 | 82.65 | 0.8694 | -201.0 | -218.3 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 7.75 | 128.97 | -60.31 | 81.74 | 0.8718 | -359.0 | -311.7 | |
| 0.00 | 0.94 | 0.00 | 0.95 | 7.87 | 128.76 | -60.52 | 81.62 | 0.8737 | -92.0 | -145.1 | |
| 1.03 | 9.58 | 1.09 | 10.13 | 8.86 | 127.30 | -61.98 | 80.59 | 0.8861 | 600.2 | 487.2 | |
| 7.35 | 52.77 | 8.14 | 59.14 | 8.21 | 125.98 | -63.30 | 81.40 | 0.8962 | 806.5 | 170.7 | |
| 5.30 | -16.00 | 5.97 | -16.00 | 8.11 | 125.46 | -63.82 | 81.53 | 0.9001 | 407.6 | 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. | |