SDO HMI 2011-11-26 03:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.54 | 39.13 | 23.62 | 51.89 | 16.85 | 297.40 | 67.48 | 287.60 | 0.9280 | 57.6 | 80.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.28 | 12.07 | 2.02 | 18.73 | 16.40 | 301.19 | 71.28 | 286.77 | 0.9503 | 156.7 | -92.4 | |
| 0.00 | 0.86 | 0.00 | 1.29 | 15.83 | 300.42 | 70.51 | 286.23 | 0.9461 | -171.0 | -177.5 | |
| 5.99 | -1.00 | 9.24 | -1.00 | 16.47 | 300.86 | 70.95 | 286.87 | 0.9487 | -375.3 | 999999 | |
| 0.00 | 0.94 | 0.00 | 1.42 | 16.08 | 300.44 | 70.53 | 286.49 | 0.9462 | -438.0 | -364.5 | |
| 0.00 | 0.77 | 0.00 | 1.03 | 16.33 | 297.57 | 67.66 | 286.99 | 0.9297 | -586.0 | -508.0 | |
| 1.20 | 5.14 | 1.44 | 6.19 | 16.14 | 295.10 | 65.19 | 287.03 | 0.9137 | 189.1 | 97.6 | |
| 0.00 | 1.28 | 0.00 | 1.56 | 16.66 | 295.29 | 65.38 | 287.57 | 0.9153 | 27.0 | -29.7 | |
| 1.37 | -6.00 | 1.64 | -6.00 | 16.33 | 294.92 | 65.01 | 287.25 | 0.9126 | 297.5 | 999999 | |
| 4.28 | 6.34 | 5.20 | 7.70 | 17.44 | 295.14 | 65.23 | 288.44 | 0.9149 | 372.6 | 203.2 | |
| 0.00 | 1.80 | 0.00 | 2.14 | 17.20 | 294.68 | 64.77 | 288.23 | 0.9116 | 425.0 | 347.8 | |
| 0.00 | 0.94 | 0.00 | 1.14 | 17.78 | 295.00 | 65.09 | 288.83 | 0.9142 | 376.0 | 334.0 | |
| 0.00 | 1.20 | 0.00 | 1.41 | 16.84 | 294.23 | 64.32 | 287.89 | 0.9082 | -268.0 | -323.4 | |
| 3.42 | 6.25 | 4.08 | 7.43 | 17.67 | 294.55 | 64.64 | 288.76 | 0.9111 | 577.3 | 548.1 | |
| 0.00 | 1.54 | 0.00 | 1.85 | 18.00 | 294.79 | 64.87 | 289.09 | 0.9129 | 553.0 | 514.5 | |
| 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. | |