SDO HMI 2011-11-25 18:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.27 | 48.96 | 22.76 | 54.58 | 16.63 | 297.72 | 62.85 | 287.83 | 0.8967 | -2.8 | -56.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.44 | 13.95 | 9.21 | 17.28 | 16.39 | 300.70 | 65.83 | 287.21 | 0.9180 | -520.3 | -235.8 | |
| 1.97 | 3.17 | 2.37 | 3.81 | 15.73 | 300.06 | 65.19 | 286.55 | 0.9132 | -251.0 | -219.4 | |
| 0.00 | 1.20 | 0.00 | 1.35 | 15.93 | 298.24 | 63.37 | 286.96 | 0.9006 | 448.0 | 319.4 | |
| 0.00 | 3.85 | 0.00 | 4.28 | 16.19 | 297.70 | 62.83 | 287.31 | 0.8968 | -534.0 | -326.9 | |
| 0.00 | 2.57 | 0.00 | 2.77 | 15.81 | 296.88 | 62.02 | 286.99 | 0.8904 | -353.0 | -324.5 | |
| 0.34 | 2.05 | 0.37 | 2.25 | 16.88 | 297.09 | 62.22 | 288.16 | 0.8929 | -505.0 | -482.8 | |
| 1.71 | 3.42 | 1.79 | 3.57 | 16.63 | 295.71 | 60.84 | 288.07 | 0.8821 | 242.0 | 53.1 | |
| 0.00 | 0.86 | 0.00 | 0.89 | 16.45 | 295.48 | 60.61 | 287.90 | 0.8801 | 286.0 | 188.5 | |
| 0.00 | 1.63 | 0.00 | 1.69 | 17.04 | 295.54 | 60.67 | 288.55 | 0.8812 | 260.0 | 167.2 | |
| 0.00 | 1.03 | 0.00 | 1.06 | 16.64 | 295.27 | 60.40 | 288.14 | 0.8786 | 189.0 | 194.3 | |
| 0.00 | 2.22 | 0.00 | 2.30 | 17.20 | 295.31 | 60.45 | 288.76 | 0.8796 | 420.0 | 374.6 | |
| 1.71 | 2.40 | 1.75 | 2.46 | 16.83 | 295.05 | 60.18 | 288.39 | 0.8771 | 363.4 | 385.2 | |
| 0.00 | 1.45 | 0.00 | 1.51 | 17.60 | 295.47 | 60.60 | 289.19 | 0.8813 | 251.0 | 174.8 | |
| 3.68 | 5.82 | 3.75 | 5.93 | 17.36 | 294.84 | 59.97 | 289.02 | 0.8760 | 576.9 | 474.7 | |
| 3.42 | 3.34 | 3.52 | 3.43 | 17.79 | 295.08 | 60.21 | 289.47 | 0.8784 | 508.4 | 0.0 | |
| 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. | |