SDO HMI 2011-06-25 08:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.82 | 51.86 | 8.41 | 62.67 | 16.99 | 166.30 | 65.20 | 287.68 | 0.9127 | -91.7 | -250.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 1.60 | 15.78 | 167.69 | 66.58 | 286.23 | 0.9214 | -291.0 | -260.2 | |
| 5.09 | 9.72 | 6.40 | 12.22 | 16.22 | 167.58 | 66.48 | 286.72 | 0.9209 | -584.6 | -417.4 | |
| 0.00 | 7.08 | 0.00 | 8.88 | 16.77 | 167.47 | 66.37 | 287.32 | 0.9205 | -605.0 | -523.8 | |
| 0.00 | 0.91 | 0.00 | 1.27 | 19.83 | 169.78 | 68.68 | 290.40 | 0.9364 | 207.0 | 237.6 | |
| 0.00 | 1.36 | 0.00 | 1.71 | 17.25 | 167.41 | 66.31 | 287.85 | 0.9204 | -394.0 | -366.9 | |
| 0.00 | 1.63 | 0.00 | 1.94 | 15.99 | 165.96 | 64.85 | 286.62 | 0.9098 | 195.0 | 21.5 | |
| 0.00 | 1.45 | 0.00 | 1.69 | 16.74 | 165.38 | 64.27 | 287.50 | 0.9063 | 242.0 | 137.8 | |
| 1.73 | 24.25 | 2.01 | 28.60 | 17.22 | 165.46 | 64.35 | 288.01 | 0.9072 | 445.8 | -277.0 | |
| 0.00 | 0.82 | 0.00 | 0.96 | 17.53 | 165.52 | 64.41 | 288.35 | 0.9079 | 242.0 | 224.2 | |
| 0.00 | 1.00 | 0.00 | 1.17 | 17.38 | 165.41 | 64.31 | 288.19 | 0.9070 | 397.0 | 322.3 | |
| 0.00 | 0.82 | 0.00 | 0.96 | 17.70 | 165.47 | 64.37 | 288.53 | 0.9077 | 351.0 | 266.7 | |
| 0.00 | 0.73 | 0.00 | 0.87 | 18.57 | 166.09 | 64.98 | 289.42 | 0.9126 | 177.0 | 118.9 | |
| 0.00 | 0.82 | 0.00 | 0.80 | 19.20 | 159.50 | 58.39 | 291.06 | 0.8638 | 544.0 | 451.8 | |
| 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. | |