SDO HMI 2011-06-30 19:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.43 | 47.57 | 8.32 | 24.12 | 14.53 | 25.24 | -3.60 | 16.51 | 0.2139 | -174.3 | -225.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.55 | 16.16 | 29.90 | 1.06 | 355.61 | 0.2330 | -876.0 | -671.0 | |
| 9.35 | 17.25 | 4.72 | 8.70 | 13.17 | 26.10 | -2.74 | 14.49 | 0.1870 | 1126.0 | 774.0 | |
| 1.91 | 2.72 | 0.96 | 1.37 | 13.26 | 25.60 | -3.25 | 16.86 | 0.1909 | 875.6 | 700.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 14.10 | 25.46 | -3.38 | 16.26 | 0.2053 | -890.0 | -639.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.44 | 25.15 | -3.69 | 15.81 | 0.2287 | -976.0 | -763.1 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 15.56 | 25.03 | -3.82 | 16.17 | 0.2313 | -938.0 | -656.6 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 14.25 | 24.83 | -4.01 | 18.84 | 0.2111 | -996.0 | -823.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 15.81 | 24.67 | -4.17 | 17.25 | 0.2371 | -1116.0 | -882.5 | |
| 4.72 | 11.71 | 2.41 | 5.98 | 16.25 | 24.41 | -4.44 | 17.68 | 0.2455 | -920.6 | -786.9 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 13.57 | 24.24 | -4.60 | 22.61 | 0.2037 | 1119.0 | 698.2 | |
| 0.00 | 2.36 | 0.00 | 1.20 | 15.59 | 24.20 | -4.64 | 19.37 | 0.2361 | -932.0 | -793.5 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 14.44 | 24.10 | -4.74 | 21.62 | 0.2183 | -1015.0 | -762.4 | |
| 0.45 | 1.27 | 0.23 | 0.65 | 15.06 | 23.83 | -5.01 | 21.63 | 0.2298 | -1172.8 | -1019.4 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 14.06 | 23.79 | -5.05 | 23.58 | 0.2145 | 758.0 | 474.7 | |
| 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. | |