SDO HMI 2014-04-08 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 26.69 | 0.19 | 14.10 | -8.15 | 8.91 | 20.09 | 262.83 | 0.3460 | 147.2 | 257.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.15 | 0.00 | 0.62 | -10.50 | 11.96 | 23.14 | 257.63 | 0.3972 | -719.0 | -631.5 | |
| 0.35 | 7.31 | 0.19 | 3.92 | -8.51 | 11.20 | 22.37 | 262.49 | 0.3813 | 1032.0 | 773.5 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -8.82 | 10.92 | 22.09 | 261.60 | 0.3773 | 927.0 | 743.0 | |
| 0.00 | 1.94 | 0.00 | 1.03 | -9.08 | 10.48 | 21.65 | 260.79 | 0.3707 | 758.0 | 675.4 | |
| 0.00 | 2.82 | 0.00 | 1.49 | -4.05 | 9.19 | 20.37 | 274.86 | 0.3499 | -2.0 | 3.6 | |
| 0.00 | 1.67 | 0.00 | 0.88 | -3.00 | 9.04 | 20.22 | 277.89 | 0.3499 | 8.0 | 3.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -10.37 | 8.99 | 20.17 | 256.65 | 0.3501 | 692.0 | 595.3 | |
| 0.00 | 2.47 | 0.00 | 1.30 | -10.05 | 8.65 | 19.82 | 257.39 | 0.3437 | 840.0 | 717.0 | |
| 0.00 | 1.94 | 0.00 | 1.01 | -7.45 | 6.21 | 17.38 | 264.59 | 0.2989 | -897.0 | -776.8 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -7.58 | 5.80 | 16.98 | 264.05 | 0.2923 | -728.0 | -618.4 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -7.97 | 5.03 | 16.20 | 262.49 | 0.2800 | -757.0 | -699.3 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -8.30 | 4.91 | 16.09 | 261.26 | 0.2787 | -855.0 | -669.8 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -11.77 | 4.55 | 15.72 | 248.89 | 0.2856 | 777.0 | 609.1 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -11.78 | 4.39 | 15.56 | 248.70 | 0.2831 | 817.0 | 662.1 | |
| 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. | |