| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.98 | 99.58 | 19.99 | 64.78 | -10.96 | 11.62 | -40.81 | 98.38 | 0.6507 | 440.6 | -49.4 | |
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back to the solar disc SDO HMI 2014-03-07 02:00:28 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.19 | -10.37 | 14.57 | -37.85 | 97.59 | 0.6112 | 862.0 | 672.6 | |
| 0.00 | 1.47 | 0.00 | 0.93 | -10.82 | 13.73 | -38.69 | 98.27 | 0.6228 | 797.0 | 593.0 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -12.29 | 13.40 | -39.02 | 100.61 | 0.6281 | 723.0 | 627.7 | |
| 0.00 | 2.86 | 0.00 | 1.81 | -11.00 | 13.46 | -38.96 | 98.56 | 0.6264 | 820.0 | 618.7 | |
| 10.30 | 13.32 | 6.52 | 8.43 | -10.26 | 13.54 | -38.88 | 97.37 | 0.6251 | 897.6 | 573.7 | |
| 5.28 | 35.39 | 3.39 | 22.87 | -10.84 | 12.55 | -39.88 | 98.25 | 0.6386 | 868.3 | 298.5 | |
| 9.60 | -6.00 | 6.22 | -6.00 | -10.43 | 11.90 | -40.52 | 97.58 | 0.6470 | 825.2 | 999999 | |
| 0.00 | 2.42 | 0.00 | 1.58 | -10.21 | 11.41 | -41.01 | 97.23 | 0.6533 | 425.0 | 462.9 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -10.44 | 10.97 | -41.45 | 97.58 | 0.6591 | 341.0 | 203.5 | |
| 1.30 | 16.53 | 0.85 | 10.83 | -10.91 | 10.85 | -41.57 | 98.29 | 0.6608 | -782.9 | -422.0 | |
| 0.00 | 1.38 | 0.00 | 0.91 | -10.33 | 10.74 | -41.68 | 97.41 | 0.6620 | 438.0 | 291.9 | |
| 0.00 | 1.47 | 0.00 | 0.98 | -11.88 | 10.22 | -42.20 | 99.72 | 0.6692 | -810.0 | -644.3 | |
| 1.82 | 9.26 | 1.21 | 6.18 | -12.12 | 9.89 | -42.54 | 100.06 | 0.6736 | -923.4 | -708.8 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -11.84 | 9.78 | -42.65 | 99.64 | 0.6749 | -612.0 | -593.1 | |
| 0.69 | 3.89 | 0.46 | 2.62 | -11.92 | 9.59 | -42.83 | 99.74 | 0.6772 | -716.2 | -568.5 | |
| 1.99 | 6.84 | 1.34 | 4.60 | -12.32 | 9.43 | -42.99 | 100.33 | 0.6795 | -650.1 | -448.5 | |
| 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. | |