| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.98 | 30.20 | 3.12 | 16.05 | -8.13 | 7.32 | -21.09 | 96.51 | 0.3604 | 153.3 | 46.5 | |
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back to the solar disc SDO HMI 2014-04-05 05:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.73 | -9.07 | 12.06 | -16.36 | 100.70 | 0.2843 | 897.0 | 749.8 | |
| 2.64 | 4.40 | 1.37 | 2.28 | -8.18 | 11.24 | -17.17 | 97.28 | 0.2959 | 1064.6 | 804.2 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -6.69 | 10.67 | -17.74 | 92.21 | 0.3043 | 898.0 | 686.4 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -6.85 | 10.32 | -18.10 | 92.75 | 0.3102 | 900.0 | 763.1 | |
| 2.64 | 4.84 | 1.38 | 2.54 | -9.62 | 9.51 | -18.91 | 101.24 | 0.3272 | 1119.9 | 802.6 | |
| 0.70 | 1.94 | 0.37 | 1.02 | -9.11 | 8.73 | -19.68 | 99.41 | 0.3386 | 1014.9 | 881.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -9.34 | 8.46 | -19.96 | 99.98 | 0.3435 | 568.0 | 493.9 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -6.68 | 5.22 | -23.20 | 92.23 | 0.3932 | -1049.0 | -853.2 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -11.89 | 4.54 | -23.87 | 105.03 | 0.4118 | 908.0 | 820.2 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -6.84 | 4.72 | -23.70 | 92.64 | 0.4012 | -632.0 | -467.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -12.08 | 4.22 | -24.20 | 105.35 | 0.4174 | 651.0 | 426.2 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -6.57 | 4.07 | -24.35 | 91.98 | 0.4115 | -879.0 | -754.5 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -6.44 | 3.78 | -24.64 | 91.67 | 0.4162 | -755.0 | -674.0 | |
| 0.00 | 2.38 | 0.00 | 1.29 | -6.64 | 3.70 | -24.72 | 92.17 | 0.4174 | -804.0 | -764.3 | |
| 0.00 | 2.38 | 0.00 | 1.29 | -6.79 | 3.59 | -24.82 | 92.52 | 0.4191 | -849.0 | -718.3 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -7.32 | 3.33 | -25.09 | 93.78 | 0.4233 | -801.0 | -635.5 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -6.56 | 3.27 | -25.14 | 91.99 | 0.4242 | -670.0 | -464.5 | |
| 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. | |