SDO HMI 2014-03-29 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.58 | 30.57 | 0.85 | 16.69 | 3.68 | 138.93 | 22.55 | 294.11 | 0.4207 | 47.6 | 144.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.69 | 3.45 | 142.04 | 25.66 | 290.81 | 0.4643 | -933.0 | -776.4 | |
| 0.00 | 3.15 | 0.00 | 1.77 | 4.79 | 142.02 | 25.64 | 293.47 | 0.4720 | -948.0 | -825.1 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 5.15 | 141.91 | 25.52 | 294.27 | 0.4727 | -868.0 | -598.7 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 2.75 | 141.36 | 24.97 | 289.91 | 0.4504 | -800.0 | -670.7 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 5.09 | 141.37 | 24.99 | 294.64 | 0.4648 | -806.0 | -650.6 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 2.87 | 141.26 | 24.88 | 290.23 | 0.4497 | -836.0 | -705.0 | |
| 0.00 | 1.75 | 0.00 | 0.97 | 4.59 | 141.05 | 24.67 | 293.93 | 0.4571 | -697.0 | -624.5 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 2.38 | 138.54 | 22.15 | 291.53 | 0.4068 | 566.0 | 484.2 | |
| 0.00 | 1.66 | 0.00 | 0.89 | 2.42 | 137.35 | 20.96 | 292.80 | 0.3894 | 776.0 | 655.9 | |
| 0.00 | 2.37 | 0.00 | 1.28 | 4.48 | 137.33 | 20.95 | 297.52 | 0.4037 | 875.0 | 661.5 | |
| 0.00 | 3.42 | 0.00 | 1.85 | 4.14 | 137.26 | 20.87 | 296.86 | 0.4001 | 918.0 | 771.8 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 2.47 | 137.15 | 20.77 | 293.12 | 0.3869 | 980.0 | 943.2 | |
| 1.58 | 4.99 | 0.85 | 2.68 | 2.74 | 137.03 | 20.65 | 293.89 | 0.3869 | 1054.7 | 775.6 | |
| 0.00 | 2.80 | 0.00 | 1.51 | 3.71 | 137.02 | 20.64 | 296.15 | 0.3935 | 868.0 | 740.5 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 3.55 | 136.83 | 20.44 | 296.01 | 0.3895 | 715.0 | 561.9 | |
| 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. | |