SDO HMI 2014-04-05 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.73 | 149.11 | 17.79 | 81.15 | 17.63 | 30.17 | 5.04 | 348.38 | 0.4163 | -275.9 | -383.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.29 | 123.68 | 1.24 | 67.38 | 17.25 | 31.32 | 6.18 | 345.53 | 0.4136 | -978.0 | -504.9 | |
| 1.32 | -1.00 | 0.72 | -1.00 | 17.55 | 31.30 | 6.16 | 345.76 | 0.4180 | -903.2 | 999999 | |
| 16.89 | -1.00 | 9.20 | -1.00 | 17.71 | 30.89 | 5.76 | 346.76 | 0.4190 | -1243.6 | 999999 | |
| 1.58 | -1.00 | 0.86 | -1.00 | 17.57 | 30.66 | 5.53 | 347.19 | 0.4161 | -1360.1 | 999999 | |
| 1.85 | -1.00 | 1.01 | -1.00 | 17.71 | 30.54 | 5.41 | 347.53 | 0.4177 | -1173.4 | 999999 | |
| 0.00 | 4.31 | 0.00 | 2.35 | 18.00 | 30.17 | 5.04 | 348.51 | 0.4210 | -536.0 | -608.4 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.51 | 27.56 | 2.43 | 354.02 | 0.3911 | 683.0 | 576.7 | |
| 0.00 | 1.50 | 0.00 | 0.80 | 16.64 | 27.28 | 2.15 | 354.74 | 0.3927 | 880.0 | 713.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 17.12 | 26.25 | 1.12 | 357.32 | 0.3994 | 755.0 | 629.7 | |
| 6.51 | 12.75 | 3.52 | 6.90 | 17.42 | 25.65 | 0.52 | 358.77 | 0.4038 | 1046.7 | 841.2 | |
| 0.00 | 1.85 | 0.00 | 1.00 | 17.71 | 25.56 | 0.43 | 359.00 | 0.4085 | 766.0 | 577.3 | |
| 2.29 | -10.00 | 1.24 | -10.00 | 17.49 | 25.40 | 0.27 | 359.36 | 0.4048 | 923.7 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 18.44 | 25.34 | 0.21 | 359.53 | 0.4200 | 824.0 | 702.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 18.67 | 24.33 | -0.80 | 1.81 | 0.4239 | 617.0 | 479.2 | |
| 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. | |