SDO HMI 2011-08-28 06:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.29 | 26.05 | 2.65 | 13.11 | 8.50 | 345.20 | 9.52 | 279.39 | 0.1718 | 173.4 | 178.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.60 | 7.37 | 351.85 | 16.17 | 271.93 | 0.2776 | -938.0 | -683.6 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 7.66 | 351.48 | 15.80 | 272.99 | 0.2714 | -796.0 | -663.8 | |
| 0.00 | 1.70 | 0.00 | 0.88 | 7.31 | 350.99 | 15.31 | 271.69 | 0.2632 | -845.0 | -705.6 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 8.07 | 350.74 | 15.05 | 274.66 | 0.2591 | -788.0 | -557.5 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 7.13 | 346.63 | 10.95 | 270.75 | 0.1893 | -943.0 | -720.2 | |
| 2.24 | 3.50 | 1.13 | 1.76 | 8.36 | 345.88 | 10.20 | 277.67 | 0.1776 | -1057.0 | -833.5 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 8.73 | 344.03 | 8.35 | 281.58 | 0.1471 | 789.0 | 554.2 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 7.71 | 343.24 | 7.55 | 275.02 | 0.1314 | 964.0 | 788.6 | |
| 0.00 | 2.69 | 0.00 | 1.34 | 7.14 | 343.04 | 7.36 | 270.63 | 0.1277 | 1087.0 | 865.4 | |
| 0.00 | 2.96 | 0.00 | 1.49 | 14.18 | 343.18 | 7.50 | 314.42 | 0.1780 | 879.0 | 590.0 | |
| 3.05 | 4.13 | 1.52 | 2.06 | 6.72 | 342.45 | 6.77 | 267.07 | 0.1177 | 1129.9 | 897.3 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 7.60 | 342.43 | 6.75 | 274.58 | 0.1174 | 868.0 | 719.1 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 6.85 | 341.87 | 6.19 | 267.92 | 0.1076 | 853.0 | 673.6 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 11.77 | 341.55 | 5.87 | 309.22 | 0.1299 | 887.0 | 727.6 | |
| 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. | |