SDO HMI 2011-06-07 23:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.54 | 60.56 | 18.12 | 47.95 | 17.42 | 20.10 | 49.03 | 292.52 | 0.7816 | -245.5 | -124.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.79 | 23.44 | 4.72 | 19.03 | 17.07 | 21.65 | 50.58 | 291.60 | 0.7964 | -448.9 | -290.7 | |
| 0.00 | 0.91 | 0.00 | 0.75 | 18.42 | 21.87 | 50.80 | 293.17 | 0.8020 | -263.0 | -252.9 | |
| 4.53 | -1.00 | 3.66 | -1.00 | 17.14 | 21.22 | 50.15 | 291.80 | 0.7924 | -526.0 | 999999 | |
| 3.89 | 17.56 | 3.11 | 13.96 | 16.69 | 20.81 | 49.74 | 291.36 | 0.7871 | -557.2 | -485.6 | |
| 4.71 | -4.00 | 3.73 | -4.00 | 16.66 | 20.41 | 49.34 | 291.44 | 0.7830 | -790.5 | 999999 | |
| 2.44 | 5.79 | 2.01 | 4.77 | 19.41 | 21.38 | 50.31 | 294.53 | 0.7999 | 508.3 | 225.4 | |
| 0.00 | 0.63 | 0.00 | 0.52 | 19.87 | 21.57 | 50.50 | 295.01 | 0.8030 | -382.0 | -374.3 | |
| 1.18 | 1.27 | 0.89 | 0.96 | 16.79 | 17.78 | 46.71 | 292.42 | 0.7561 | -568.1 | -570.0 | |
| 0.00 | 1.72 | 0.00 | 1.28 | 17.01 | 17.11 | 46.04 | 292.93 | 0.7496 | -712.0 | -578.1 | |
| 0.00 | 3.44 | 0.00 | 2.49 | 17.59 | 15.16 | 44.09 | 294.39 | 0.7305 | 742.0 | 537.2 | |
| 0.00 | 1.54 | 0.00 | 1.11 | 17.84 | 15.10 | 44.03 | 294.75 | 0.7308 | 614.0 | 488.1 | |
| 0.00 | 1.36 | 0.00 | 0.99 | 18.52 | 15.27 | 44.20 | 295.56 | 0.7351 | 514.0 | 435.2 | |
| 0.00 | 1.00 | 0.00 | 0.73 | 18.90 | 15.22 | 44.15 | 296.08 | 0.7360 | 612.0 | 506.9 | |
| 0.00 | 1.90 | 0.00 | 1.36 | 19.58 | 13.71 | 42.64 | 297.60 | 0.7225 | 671.0 | 518.6 | |
| 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. | |