| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.40 | 190.12 | 43.19 | 193.42 | 7.72 | 129.68 | -60.70 | 81.80 | 0.8742 | -73.7 | -116.5 | |
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back to the solar disc SDO HMI 2011-11-29 03:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.96 | 8.88 | 132.60 | -57.78 | 80.25 | 0.8502 | 557.0 | 522.5 | |
| 0.00 | 2.05 | 0.00 | 1.97 | 9.16 | 131.60 | -58.77 | 80.01 | 0.8593 | 401.0 | 340.2 | |
| 14.71 | 103.31 | 14.05 | 98.63 | 7.46 | 131.73 | -58.65 | 81.98 | 0.8572 | -825.5 | -268.3 | |
| 1.97 | -3.00 | 1.89 | -3.00 | 7.94 | 131.62 | -58.75 | 81.43 | 0.8584 | -557.2 | 999999 | |
| 0.00 | 2.39 | 0.00 | 2.32 | 8.65 | 131.27 | -59.10 | 80.63 | 0.8619 | 169.0 | 81.6 | |
| 0.00 | 2.14 | 0.00 | 2.10 | 6.82 | 130.69 | -59.68 | 82.79 | 0.8660 | -570.0 | -463.7 | |
| 0.00 | 2.48 | 0.00 | 2.45 | 7.11 | 130.51 | -59.86 | 82.46 | 0.8677 | -440.0 | -363.8 | |
| 3.51 | 5.64 | 3.45 | 5.56 | 6.34 | 130.61 | -59.77 | 83.35 | 0.8666 | -443.0 | -539.9 | |
| 0.00 | 3.34 | 0.00 | 3.32 | 6.78 | 130.34 | -60.03 | 82.85 | 0.8690 | -317.0 | -233.9 | |
| 1.97 | 10.95 | 2.00 | 11.13 | 7.51 | 129.57 | -60.81 | 82.05 | 0.8759 | -367.6 | -181.2 | |
| 0.94 | -10.00 | 0.97 | -10.00 | 7.45 | 129.33 | -61.04 | 82.14 | 0.8778 | 366.5 | 999999 | |
| 1.88 | 3.08 | 1.94 | 3.17 | 6.97 | 129.19 | -61.18 | 82.69 | 0.8788 | -197.2 | -139.9 | |
| 0.00 | 0.86 | 0.00 | 0.89 | 7.80 | 128.87 | -61.50 | 81.76 | 0.8817 | -242.0 | -195.2 | |
| 1.20 | 7.01 | 1.31 | 7.67 | 8.91 | 127.39 | -62.98 | 80.60 | 0.8940 | 521.5 | 432.7 | |
| 0.00 | 1.03 | 0.00 | 1.13 | 8.58 | 127.23 | -63.15 | 80.98 | 0.8951 | 296.0 | 258.8 | |
| 11.12 | 44.81 | 12.77 | 52.12 | 8.20 | 126.04 | -64.33 | 81.47 | 0.9039 | 693.0 | 170.3 | |
| 4.10 | -16.00 | 4.81 | -16.00 | 8.10 | 125.44 | -64.93 | 81.61 | 0.9083 | 370.2 | 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. | |