SDO HMI 2014-03-10 16:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.93 | 81.62 | 16.90 | 41.85 | 6.63 | 10.62 | 5.40 | 338.81 | 0.2588 | -30.7 | 111.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.95 | 2.60 | 0.49 | 1.34 | 5.83 | 14.40 | 9.18 | 324.70 | 0.2759 | -981.8 | -737.4 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 5.98 | 14.22 | 9.00 | 325.54 | 0.2763 | -725.0 | -631.1 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 6.12 | 13.65 | 8.43 | 327.57 | 0.2730 | -911.0 | -779.8 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 6.48 | 13.60 | 8.37 | 328.44 | 0.2778 | -1037.0 | -788.3 | |
| 12.30 | 16.38 | 6.34 | 8.43 | 7.05 | 12.22 | 6.99 | 333.80 | 0.2749 | -1063.5 | -703.7 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 6.65 | 12.15 | 6.93 | 333.36 | 0.2684 | -1023.0 | -803.4 | |
| 0.00 | 1.47 | 0.00 | 0.76 | 7.37 | 11.50 | 6.27 | 336.67 | 0.2749 | -833.0 | -656.6 | |
| 0.78 | 1.73 | 0.40 | 0.88 | 5.28 | 10.57 | 5.34 | 336.76 | 0.2361 | 985.2 | 886.2 | |
| 0.00 | 2.43 | 0.00 | 1.24 | 5.43 | 10.36 | 5.14 | 337.82 | 0.2371 | 1112.0 | 804.4 | |
| 1.91 | 35.26 | 0.98 | 18.07 | 7.36 | 10.08 | 4.86 | 341.52 | 0.2661 | -881.5 | 203.3 | |
| 0.00 | 2.86 | 0.00 | 1.47 | 6.87 | 10.07 | 4.85 | 340.94 | 0.2582 | 855.0 | 595.0 | |
| 2.86 | 7.54 | 1.46 | 3.84 | 5.82 | 9.82 | 4.60 | 340.50 | 0.2401 | 1098.2 | 787.6 | |
| 13.00 | -10.00 | 6.65 | -10.00 | 6.77 | 9.53 | 4.31 | 342.83 | 0.2538 | 1104.9 | 999999 | |
| 1.13 | 5.20 | 0.58 | 2.65 | 6.40 | 8.78 | 3.55 | 345.32 | 0.2443 | 872.7 | 729.2 | |
| 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. | |