SDO HMI 2011-08-27 02:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.01 | 79.51 | 14.01 | 39.72 | 7.52 | 344.01 | -7.07 | 97.55 | 0.1241 | 442.8 | -7.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.96 | 0.00 | 1.47 | 7.33 | 351.49 | 0.41 | 300.22 | 0.0082 | -1042.0 | -975.7 | |
| 0.00 | 1.44 | 0.00 | 0.71 | 7.30 | 351.31 | 0.23 | 312.57 | 0.0053 | -870.0 | -693.4 | |
| 0.00 | 2.33 | 0.00 | 1.16 | 7.63 | 348.78 | -2.31 | 76.74 | 0.0412 | -910.0 | -748.3 | |
| 0.00 | 1.26 | 0.00 | 0.62 | 7.04 | 346.73 | -4.35 | 90.48 | 0.0757 | -678.0 | -579.9 | |
| 0.00 | 1.35 | 0.00 | 0.67 | 8.76 | 346.04 | -5.05 | 71.27 | 0.0923 | 847.0 | 588.9 | |
| 0.00 | 2.24 | 0.00 | 1.12 | 6.76 | 345.88 | -5.21 | 93.42 | 0.0907 | -815.0 | -767.8 | |
| 0.00 | 3.50 | 0.00 | 1.74 | 8.50 | 345.21 | -5.88 | 75.99 | 0.1048 | -1121.0 | -794.6 | |
| 1.17 | 12.83 | 0.58 | 6.40 | 8.68 | 344.62 | -6.46 | 75.66 | 0.1154 | -1089.7 | -823.8 | |
| 1.17 | -8.00 | 0.58 | -8.00 | 8.61 | 344.19 | -6.90 | 77.01 | 0.1224 | -682.2 | 999999 | |
| 7.45 | 49.98 | 3.73 | 25.02 | 7.14 | 343.01 | -8.07 | 89.17 | 0.1400 | 1284.0 | 701.4 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 7.77 | 343.00 | -8.08 | 84.62 | 0.1406 | 916.0 | 722.7 | |
| 3.59 | -10.00 | 1.80 | -10.00 | 7.35 | 342.95 | -8.14 | 87.67 | 0.1411 | 1030.7 | 999999 | |
| 3.32 | -10.00 | 1.66 | -10.00 | 7.32 | 342.73 | -8.35 | 87.94 | 0.1448 | 1009.1 | 999999 | |
| 11.31 | -10.00 | 5.66 | -10.00 | 7.10 | 342.61 | -8.47 | 89.42 | 0.1469 | 1082.3 | 999999 | |
| 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. | |