SDO HMI 2014-04-04 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.25 | 28.38 | 4.53 | 15.61 | -7.97 | 9.20 | -25.82 | 95.31 | 0.4355 | 548.0 | 410.6 | |
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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 | 0.90 | -8.05 | 12.40 | -22.63 | 95.74 | 0.3846 | 820.0 | 733.4 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -6.62 | 11.82 | -23.21 | 92.00 | 0.3934 | 874.0 | 675.4 | |
| 2.02 | 6.50 | 1.10 | 3.52 | -8.29 | 11.00 | -24.03 | 96.16 | 0.4071 | 926.9 | 755.3 | |
| 2.37 | -3.00 | 1.29 | -3.00 | -8.41 | 10.99 | -24.04 | 96.46 | 0.4073 | 1033.7 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.81 | -6.79 | 10.32 | -24.70 | 92.46 | 0.4171 | 738.0 | 548.5 | |
| 1.14 | 3.08 | 0.63 | 1.69 | -8.86 | 9.55 | -25.48 | 97.30 | 0.4303 | 983.2 | 827.6 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -7.05 | 9.54 | -25.49 | 93.09 | 0.4295 | 768.0 | 669.8 | |
| 2.02 | 4.04 | 1.11 | 2.22 | -9.32 | 9.28 | -25.75 | 98.34 | 0.4351 | 900.4 | 734.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -10.67 | 9.16 | -25.86 | 101.39 | 0.4392 | 600.0 | 477.1 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -8.84 | 8.71 | -26.32 | 97.15 | 0.4434 | 888.0 | 717.4 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -8.99 | 8.56 | -26.47 | 97.45 | 0.4458 | 767.0 | 557.8 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -2.40 | 7.86 | -27.17 | 82.94 | 0.4617 | 730.0 | 553.7 | |
| 0.70 | 2.02 | 0.40 | 1.15 | -6.52 | 5.10 | -29.93 | 92.05 | 0.4980 | -913.5 | -758.3 | |
| 0.00 | 2.11 | 0.00 | 1.22 | -7.66 | 4.00 | -31.03 | 94.33 | 0.5144 | -916.0 | -799.4 | |
| 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. | |