SDO HMI 2011-08-28 07:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.49 | 21.92 | 1.75 | 11.05 | 7.75 | 345.31 | 10.18 | 274.39 | 0.1774 | 0.4 | 98.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.56 | 7.44 | 351.88 | 16.74 | 272.20 | 0.2871 | -680.0 | -561.9 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 7.29 | 351.01 | 15.88 | 271.64 | 0.2727 | -837.0 | -716.8 | |
| 0.00 | 1.97 | 0.00 | 1.01 | 7.77 | 350.40 | 15.26 | 273.45 | 0.2624 | -980.0 | -755.4 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 8.61 | 350.37 | 15.23 | 276.70 | 0.2627 | -763.0 | -577.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 7.97 | 346.26 | 11.12 | 275.18 | 0.1927 | -977.0 | -721.6 | |
| 1.79 | 2.42 | 0.90 | 1.22 | 8.31 | 345.86 | 10.72 | 277.15 | 0.1864 | -1062.8 | -986.9 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 7.42 | 345.37 | 10.24 | 272.36 | 0.1772 | -853.0 | -651.5 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 8.09 | 343.34 | 8.21 | 277.40 | 0.1432 | 812.0 | 639.4 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 7.67 | 343.21 | 8.07 | 274.50 | 0.1403 | 915.0 | 655.7 | |
| 0.00 | 1.97 | 0.00 | 0.99 | 7.16 | 343.08 | 7.94 | 270.82 | 0.1377 | 974.0 | 808.0 | |
| 1.70 | 4.22 | 0.85 | 2.11 | 6.68 | 342.45 | 7.32 | 267.07 | 0.1273 | 1101.9 | 921.0 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 7.65 | 342.44 | 7.30 | 274.73 | 0.1270 | 801.0 | 642.5 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 7.12 | 341.88 | 6.74 | 270.45 | 0.1170 | 733.0 | 545.5 | |
| 0.00 | 1.17 | 0.00 | 0.58 | 11.73 | 341.75 | 6.61 | 305.77 | 0.1396 | 880.0 | 755.2 | |
| 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. | |