SDO HMI 2011-10-07 17:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.59 | 148.54 | 15.76 | 81.76 | -11.38 | 180.25 | 18.69 | 226.24 | 0.4367 | 368.5 | 268.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.59 | 133.04 | 15.76 | 73.38 | -11.22 | 180.84 | 19.28 | 227.53 | 0.4409 | 1154.8 | 386.9 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -11.17 | 180.09 | 18.53 | 226.50 | 0.4317 | 998.0 | 745.8 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -12.88 | 176.52 | 14.96 | 217.65 | 0.4138 | -763.0 | -611.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -13.16 | 176.54 | 14.98 | 217.26 | 0.4175 | -787.0 | -576.6 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -12.67 | 174.74 | 13.18 | 214.50 | 0.3943 | -678.0 | -558.3 | |
| 0.00 | 1.75 | 0.00 | 0.94 | -11.53 | 174.65 | 13.09 | 216.06 | 0.3786 | -952.0 | -756.7 | |
| 0.00 | 1.84 | 0.00 | 1.00 | -14.10 | 174.69 | 13.13 | 212.40 | 0.4129 | -710.0 | -587.2 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -13.33 | 174.65 | 13.09 | 213.37 | 0.4023 | -824.0 | -656.1 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -12.22 | 174.46 | 12.90 | 214.61 | 0.3859 | -851.0 | -715.1 | |
| 0.00 | 1.75 | 0.00 | 0.94 | -12.47 | 174.38 | 12.82 | 214.06 | 0.3885 | -844.0 | -570.0 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -14.27 | 173.97 | 12.41 | 210.74 | 0.4092 | -807.0 | -644.0 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -14.17 | 173.84 | 12.28 | 210.60 | 0.4068 | -866.0 | -665.9 | |
| 0.00 | 1.40 | 0.00 | 0.75 | -11.83 | 172.94 | 11.38 | 211.88 | 0.3672 | -885.0 | -721.1 | |
| 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. | |