SDO HMI 2014-03-16 02:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.17 | 109.35 | 37.71 | 265.14 | 5.75 | 11.08 | 77.26 | 277.45 | 0.9795 | 194.8 | 65.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.43 | 0.00 | 6.52 | 2.96 | 12.74 | 78.92 | 274.39 | 0.9838 | 274.0 | 184.9 | |
| 0.00 | 1.56 | 0.00 | 4.25 | 3.44 | 12.72 | 78.90 | 274.88 | 0.9839 | -126.0 | -58.2 | |
| 0.00 | 1.48 | 0.00 | 3.98 | 3.68 | 12.64 | 78.82 | 275.12 | 0.9838 | -286.0 | -248.5 | |
| 0.00 | 3.48 | 0.00 | 10.91 | 6.33 | 13.77 | 79.96 | 277.63 | 0.9881 | -326.0 | -163.9 | |
| 0.00 | 4.78 | 0.00 | 15.23 | 6.78 | 13.90 | 80.08 | 278.05 | 0.9886 | -107.0 | -82.3 | |
| 0.00 | 2.17 | 0.00 | 5.97 | 4.79 | 12.60 | 78.79 | 276.25 | 0.9842 | -334.0 | -352.2 | |
| 0.00 | 1.65 | 0.00 | 4.34 | 5.16 | 12.15 | 78.33 | 276.69 | 0.9829 | -263.0 | -296.8 | |
| 2.09 | 8.35 | 5.18 | 20.69 | 5.08 | 11.53 | 77.71 | 276.70 | 0.9808 | -213.5 | -201.9 | |
| 5.13 | 72.33 | 12.20 | 169.42 | 5.92 | 10.92 | 77.10 | 277.64 | 0.9792 | 182.4 | 154.0 | |
| 4.35 | -9.00 | 10.01 | -9.00 | 6.32 | 10.43 | 76.61 | 278.11 | 0.9777 | 417.5 | 999999 | |
| 1.91 | -9.00 | 4.36 | -9.00 | 6.03 | 10.30 | 76.48 | 277.84 | 0.9770 | 553.4 | 999999 | |
| 1.30 | 8.69 | 2.75 | 18.67 | 4.39 | 9.54 | 75.72 | 276.29 | 0.9732 | 339.5 | 57.5 | |
| 1.39 | -9.00 | 3.21 | -9.00 | 6.61 | 10.31 | 76.49 | 278.43 | 0.9774 | 298.6 | 999999 | |
| 0.00 | 2.43 | 0.00 | 5.16 | 4.95 | 9.48 | 75.67 | 276.88 | 0.9733 | 471.0 | 418.0 | |
| 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. | |