SDO HMI 2014-03-10 17:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.36 | 80.83 | 16.11 | 41.52 | 6.66 | 10.79 | 6.11 | 336.36 | 0.2639 | 86.0 | 61.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.21 | 2.34 | 0.63 | 1.21 | 5.84 | 14.47 | 9.79 | 322.95 | 0.2821 | -1026.8 | -843.5 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 5.89 | 14.32 | 9.64 | 323.50 | 0.2814 | -852.0 | -635.2 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 6.13 | 13.77 | 9.10 | 325.56 | 0.2794 | -916.0 | -733.8 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 6.43 | 13.63 | 8.96 | 326.60 | 0.2823 | -1102.0 | -827.1 | |
| 11.26 | 18.37 | 5.81 | 9.47 | 6.96 | 12.31 | 7.63 | 331.61 | 0.2786 | -1054.7 | -562.8 | |
| 0.00 | 3.90 | 0.00 | 2.01 | 6.71 | 12.09 | 7.42 | 331.87 | 0.2732 | -642.0 | -348.9 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 7.32 | 11.65 | 6.97 | 334.30 | 0.2789 | -838.0 | -719.0 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 5.31 | 10.53 | 5.86 | 334.84 | 0.2402 | 1126.0 | 874.2 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 5.43 | 10.32 | 5.65 | 335.83 | 0.2406 | 1130.0 | 911.2 | |
| 2.51 | 34.39 | 1.29 | 17.64 | 7.33 | 10.05 | 5.38 | 339.67 | 0.2686 | -925.6 | 271.3 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 6.81 | 9.95 | 5.28 | 339.32 | 0.2598 | 1041.0 | 733.0 | |
| 2.69 | 4.59 | 1.37 | 2.34 | 5.83 | 9.82 | 5.15 | 338.39 | 0.2434 | 1109.9 | 784.9 | |
| 13.08 | -10.00 | 6.70 | -10.00 | 6.74 | 9.50 | 4.83 | 340.87 | 0.2561 | 1109.5 | 999999 | |
| 0.61 | 2.95 | 0.31 | 1.51 | 6.46 | 8.74 | 4.07 | 343.37 | 0.2477 | 971.0 | 796.1 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 6.21 | 8.74 | 4.07 | 343.09 | 0.2437 | 1041.0 | 791.8 | |
| 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. | |