SDO HMI 2012-05-07 14:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.58 | 25.39 | 1.86 | 13.47 | 15.19 | 226.88 | -8.50 | 23.12 | 0.3537 | -12.2 | -7.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.60 | 13.77 | 235.64 | 0.25 | 359.16 | 0.2973 | -634.0 | -534.0 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 13.39 | 235.20 | -0.18 | 0.61 | 0.2909 | -736.0 | -587.8 | |
| 0.00 | 2.77 | 0.00 | 1.45 | 13.85 | 229.49 | -5.89 | 18.55 | 0.3147 | -939.0 | -791.4 | |
| 3.58 | 5.73 | 1.86 | 2.98 | 13.63 | 229.46 | -5.92 | 18.86 | 0.3114 | -1104.7 | -910.0 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 13.86 | 228.01 | -7.37 | 22.73 | 0.3235 | -954.0 | -719.6 | |
| 0.00 | 2.59 | 0.00 | 1.37 | 14.45 | 226.32 | -9.06 | 26.44 | 0.3439 | -801.0 | -714.2 | |
| 0.00 | 2.33 | 0.00 | 1.23 | 13.99 | 225.23 | -10.15 | 29.78 | 0.3456 | 914.0 | 727.6 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 16.87 | 224.77 | -10.61 | 26.98 | 0.3901 | 780.0 | 600.7 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 17.80 | 222.96 | -12.42 | 29.56 | 0.4167 | 954.0 | 700.8 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 16.96 | 222.92 | -12.46 | 30.72 | 0.4056 | 849.0 | 673.9 | |
| 0.00 | 2.86 | 0.00 | 1.56 | 18.06 | 222.78 | -12.60 | 29.59 | 0.4217 | 806.0 | 705.5 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 17.80 | 222.77 | -12.61 | 29.94 | 0.4183 | 782.0 | 627.8 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 17.35 | 222.44 | -12.94 | 31.15 | 0.4149 | 865.0 | 653.8 | |
| 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. | |