SDO HMI 2014-03-24 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.39 | 39.65 | 7.40 | 28.54 | 3.15 | 137.40 | -45.48 | 78.97 | 0.7275 | -37.9 | 84.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.92 | 8.21 | 1.35 | 5.75 | 3.45 | 139.02 | -43.86 | 78.07 | 0.7092 | -733.2 | -476.8 | |
| 2.01 | -1.00 | 1.41 | -1.00 | 3.15 | 138.95 | -43.92 | 78.50 | 0.7092 | -622.1 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.67 | 2.71 | 138.76 | -44.11 | 79.17 | 0.7102 | -389.0 | -270.5 | |
| 0.00 | 1.83 | 0.00 | 1.29 | 3.48 | 138.68 | -44.19 | 78.14 | 0.7133 | 34.0 | -70.6 | |
| 3.84 | 7.08 | 2.73 | 5.03 | 3.91 | 138.23 | -44.64 | 77.70 | 0.7198 | -644.8 | -383.1 | |
| 0.00 | 1.75 | 0.00 | 1.24 | 3.54 | 138.05 | -44.83 | 78.27 | 0.7210 | 514.0 | 466.0 | |
| 0.00 | 0.96 | 0.00 | 0.69 | 3.96 | 137.68 | -45.20 | 77.81 | 0.7265 | -443.0 | -340.9 | |
| 0.00 | 0.52 | 0.00 | 0.38 | 3.51 | 137.66 | -45.21 | 78.43 | 0.7254 | 549.0 | 517.3 | |
| 0.70 | 3.41 | 0.51 | 2.48 | 3.85 | 136.87 | -46.01 | 78.21 | 0.7356 | -559.8 | -239.4 | |
| 0.00 | 3.67 | 0.00 | 2.67 | 2.71 | 136.76 | -46.11 | 79.77 | 0.7339 | 232.0 | 304.3 | |
| 1.92 | 4.54 | 1.40 | 3.32 | 2.31 | 136.43 | -46.44 | 80.39 | 0.7367 | 715.7 | 543.4 | |
| 0.00 | 0.61 | 0.00 | 0.45 | 2.27 | 135.55 | -47.32 | 80.68 | 0.7467 | 697.0 | 628.4 | |
| 0.00 | 1.92 | 0.00 | 1.43 | 2.46 | 135.46 | -47.42 | 80.45 | 0.7483 | 609.0 | 551.0 | |
| 0.00 | 4.19 | 0.00 | 3.14 | 2.37 | 135.10 | -47.77 | 80.66 | 0.7521 | 486.0 | 435.7 | |
| 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. | |