| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.74 | 54.06 | 17.50 | 58.32 | 16.61 | 298.34 | 61.82 | 287.95 | 0.8890 | -158.5 | 35.7 | |
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back to the solar disc SDO HMI 2011-11-25 15:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.56 | 21.91 | 9.94 | 25.54 | 16.38 | 300.66 | 64.14 | 287.37 | 0.9064 | -546.3 | -76.7 | |
| 2.91 | 5.65 | 3.29 | 6.37 | 15.69 | 299.91 | 63.38 | 286.69 | 0.9004 | -339.1 | -265.0 | |
| 0.00 | 1.28 | 0.00 | 1.36 | 15.39 | 298.07 | 61.55 | 286.58 | 0.8864 | -224.0 | -200.3 | |
| 0.00 | 0.94 | 0.00 | 1.01 | 16.19 | 298.23 | 61.70 | 287.45 | 0.8883 | 507.0 | 401.8 | |
| 0.00 | 1.11 | 0.00 | 1.17 | 16.24 | 297.54 | 61.02 | 287.60 | 0.8831 | -340.0 | -385.9 | |
| 0.00 | 1.11 | 0.00 | 1.13 | 15.83 | 296.70 | 60.17 | 287.25 | 0.8759 | -527.0 | -387.2 | |
| 1.28 | 2.05 | 1.33 | 2.13 | 16.86 | 297.11 | 60.59 | 288.36 | 0.8803 | -477.4 | -437.3 | |
| 0.00 | 2.57 | 0.00 | 2.58 | 16.67 | 296.07 | 59.55 | 288.30 | 0.8718 | 150.0 | 114.0 | |
| 0.00 | 0.34 | 0.00 | 0.34 | 16.77 | 295.88 | 59.35 | 288.44 | 0.8703 | 272.0 | 269.8 | |
| 0.00 | 1.71 | 0.00 | 1.68 | 16.84 | 295.25 | 58.72 | 288.62 | 0.8653 | 461.0 | 381.1 | |
| 0.00 | 2.22 | 0.00 | 2.21 | 17.61 | 295.59 | 59.06 | 289.44 | 0.8690 | 336.0 | 197.2 | |
| 0.00 | 1.11 | 0.00 | 1.09 | 17.53 | 295.12 | 58.59 | 289.43 | 0.8651 | 509.0 | 382.7 | |
| 2.99 | 3.51 | 2.94 | 3.45 | 17.77 | 295.19 | 58.66 | 289.70 | 0.8660 | 555.5 | 482.5 | |
| 0.00 | 6.16 | 0.00 | 5.99 | 17.32 | 294.89 | 58.37 | 289.22 | 0.8629 | 677.0 | 549.8 | |
| 0.00 | 1.45 | 0.00 | 1.39 | 17.86 | 294.11 | 57.58 | 289.98 | 0.8570 | -348.0 | -294.0 | |
| 0.00 | 0.94 | 0.00 | 0.88 | 17.72 | 293.40 | 56.88 | 289.95 | 0.8508 | -600.0 | -491.4 | |
| 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. | |