SDO HMI 2014-05-21 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.55 | 173.19 | 21.38 | 138.87 | -24.89 | 189.94 | 48.25 | 239.43 | 0.7883 | 470.0 | 246.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.55 | 163.74 | 21.38 | 131.79 | -24.77 | 190.20 | 48.51 | 239.68 | 0.7902 | 936.6 | 289.1 | |
| 0.00 | 0.45 | 0.00 | 0.37 | -26.60 | 190.18 | 48.49 | 237.47 | 0.7963 | 346.0 | 272.8 | |
| 0.00 | 0.99 | 0.00 | 0.74 | -25.83 | 185.94 | 44.25 | 236.67 | 0.7540 | -501.0 | -395.8 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -25.73 | 185.66 | 43.97 | 236.66 | 0.7509 | -312.0 | -471.3 | |
| 0.00 | 0.90 | 0.00 | 0.67 | -25.64 | 185.29 | 43.60 | 236.61 | 0.7469 | -444.0 | -403.2 | |
| 0.00 | 0.72 | 0.00 | 0.53 | -25.41 | 185.14 | 43.45 | 236.82 | 0.7444 | -559.0 | -533.4 | |
| 0.00 | 1.08 | 0.00 | 0.80 | -25.68 | 185.12 | 43.43 | 236.48 | 0.7454 | -650.0 | -557.3 | |
| 0.00 | 0.81 | 0.00 | 0.61 | -26.34 | 185.38 | 43.69 | 235.78 | 0.7509 | -561.0 | -437.4 | |
| 0.00 | 1.26 | 0.00 | 0.95 | -27.51 | 185.67 | 43.98 | 234.48 | 0.7589 | -531.0 | -402.9 | |
| 0.00 | 0.63 | 0.00 | 0.47 | -28.53 | 183.91 | 42.22 | 232.39 | 0.7475 | -623.0 | -506.0 | |
| 0.00 | 1.17 | 0.00 | 0.87 | -28.81 | 183.72 | 42.03 | 231.95 | 0.7472 | -419.0 | -400.8 | |
| 0.00 | 1.17 | 0.00 | 0.87 | -29.33 | 183.75 | 42.05 | 231.35 | 0.7501 | -551.0 | -462.8 | |
| 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. | |