SDO HMI 2014-03-11 20:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.83 | 0.00 | 11.93 | -10.36 | 14.62 | 24.78 | 260.53 | 0.4191 | 155.3 | 323.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.47 | 0.00 | 0.84 | -9.53 | 19.62 | 29.78 | 263.40 | 0.4951 | 689.0 | 559.4 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -9.68 | 18.66 | 28.82 | 263.02 | 0.4808 | 590.0 | 472.6 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -10.18 | 18.19 | 28.35 | 261.90 | 0.4741 | 680.0 | 511.2 | |
| 0.00 | 1.04 | 0.00 | 0.58 | -9.59 | 18.07 | 28.23 | 263.14 | 0.4717 | 711.0 | 585.2 | |
| 0.00 | 5.81 | 0.00 | 3.22 | -10.26 | 16.76 | 26.93 | 261.51 | 0.4524 | 837.0 | 702.5 | |
| 0.00 | 2.77 | 0.00 | 1.53 | -10.17 | 16.32 | 26.48 | 261.65 | 0.4454 | 885.0 | 646.4 | |
| 0.00 | 2.17 | 0.00 | 1.16 | -10.06 | 12.58 | 22.74 | 261.17 | 0.3868 | 874.0 | 706.1 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -9.74 | 12.29 | 22.45 | 261.93 | 0.3818 | 836.0 | 738.6 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -11.01 | 11.99 | 22.15 | 258.52 | 0.3794 | -813.0 | -727.1 | |
| 0.00 | 0.87 | 0.00 | 0.46 | -11.54 | 11.54 | 21.70 | 256.94 | 0.3736 | -791.0 | -632.6 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -12.14 | 8.64 | 18.80 | 253.67 | 0.3297 | -912.0 | -682.6 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -11.57 | 7.80 | 17.96 | 254.84 | 0.3143 | -748.0 | -626.5 | |
| 0.00 | 1.30 | 0.00 | 0.68 | -10.60 | 7.48 | 17.64 | 257.74 | 0.3062 | -819.0 | -669.7 | |
| 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. | |