SDO HMI 2012-05-07 00:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.57 | 36.61 | 5.11 | 20.12 | 15.80 | 226.18 | -16.89 | 40.05 | 0.4326 | 70.8 | 327.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.23 | 13.00 | 235.26 | -7.80 | 24.99 | 0.3146 | -729.0 | -610.0 | |
| 9.57 | 15.12 | 5.11 | 8.07 | 13.64 | 229.38 | -13.69 | 38.09 | 0.3744 | -1044.4 | -661.7 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 16.88 | 226.93 | -16.13 | 37.52 | 0.4384 | -731.0 | -522.3 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 16.31 | 224.80 | -18.26 | 41.81 | 0.4530 | 637.0 | 540.3 | |
| 0.00 | 1.79 | 0.00 | 1.00 | 17.18 | 224.65 | -18.42 | 40.73 | 0.4644 | 777.0 | 613.8 | |
| 0.00 | 1.61 | 0.00 | 0.90 | 16.95 | 224.61 | -18.46 | 41.13 | 0.4623 | 825.0 | 676.9 | |
| 0.00 | 3.76 | 0.00 | 2.10 | 17.28 | 224.44 | -18.63 | 40.90 | 0.4677 | 850.0 | 673.4 | |
| 0.00 | 3.31 | 0.00 | 1.86 | 17.32 | 224.20 | -18.87 | 41.20 | 0.4705 | 778.0 | 615.1 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 17.70 | 223.08 | -19.99 | 42.25 | 0.4862 | 794.0 | 613.9 | |
| 0.00 | 1.52 | 0.00 | 0.86 | 17.87 | 222.72 | -20.34 | 42.50 | 0.4917 | 824.0 | 690.5 | |
| 0.00 | 2.15 | 0.00 | 1.22 | 17.45 | 222.74 | -20.33 | 43.10 | 0.4870 | 831.0 | 715.5 | |
| 0.00 | 2.51 | 0.00 | 1.42 | 17.68 | 222.58 | -20.49 | 42.98 | 0.4912 | 812.0 | 625.8 | |
| 0.00 | 1.88 | 0.00 | 1.07 | 17.49 | 222.43 | -20.64 | 43.46 | 0.4907 | 880.0 | 680.0 | |
| 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. | |