SDO HMI 2014-04-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.08 | 21.65 | 1.55 | 10.95 | -8.24 | 8.47 | -11.15 | 100.24 | 0.1985 | 257.1 | 177.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.67 | 0.00 | 0.83 | -6.86 | 12.65 | -6.97 | 95.13 | 0.1216 | 916.0 | 690.0 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -4.10 | 12.56 | -7.06 | 73.07 | 0.1287 | 875.0 | 680.4 | |
| 0.00 | 0.53 | 0.00 | 0.26 | -3.55 | 11.90 | -7.72 | 70.78 | 0.1427 | 609.0 | 593.8 | |
| 0.00 | 2.11 | 0.00 | 1.06 | -8.04 | 11.50 | -8.13 | 102.77 | 0.1442 | 1002.0 | 826.1 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -10.21 | 10.61 | -9.01 | 114.40 | 0.1700 | 895.0 | 648.5 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -9.03 | 10.22 | -9.41 | 107.04 | 0.1696 | -870.0 | -624.5 | |
| 3.08 | 4.66 | 1.55 | 2.35 | -9.84 | 9.79 | -9.83 | 110.71 | 0.1807 | 1090.1 | 781.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -6.18 | 9.73 | -9.89 | 89.92 | 0.1716 | 877.0 | 671.0 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -11.40 | 5.99 | -13.63 | 111.78 | 0.2500 | 758.0 | 600.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.25 | 5.63 | -13.99 | 94.79 | 0.2418 | -822.0 | -553.7 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -7.20 | 5.04 | -14.58 | 94.48 | 0.2517 | -913.0 | -762.4 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -6.87 | 5.02 | -14.60 | 93.16 | 0.2519 | -867.0 | -693.0 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -6.66 | 3.93 | -15.69 | 92.27 | 0.2701 | -949.0 | -801.9 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -11.84 | 359.10 | -20.52 | 106.82 | 0.3600 | 540.0 | 363.2 | |
| 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. | |