SDO HMI 2011-05-31 03:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.71 | 172.07 | 26.87 | 151.63 | 16.67 | 21.11 | -53.63 | 69.07 | 0.8276 | -565.7 | -218.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.88 | 20.55 | 21.97 | -52.77 | 64.29 | 0.8296 | -648.0 | -504.6 | |
| 0.00 | 1.26 | 0.00 | 1.07 | 17.40 | 22.74 | -51.99 | 67.76 | 0.8145 | -667.0 | -540.1 | |
| 0.00 | 1.26 | 0.00 | 1.12 | 18.93 | 21.28 | -53.45 | 66.37 | 0.8316 | -172.0 | -178.7 | |
| 0.00 | 5.33 | 0.00 | 4.65 | 17.23 | 21.55 | -53.19 | 68.30 | 0.8251 | -466.0 | -328.6 | |
| 29.45 | 151.13 | 25.55 | 131.36 | 16.49 | 21.64 | -53.10 | 69.15 | 0.8227 | -848.8 | -258.3 | |
| 0.00 | 2.08 | 0.00 | 2.12 | 19.04 | 15.94 | -58.80 | 67.61 | 0.8764 | 638.0 | 506.7 | |
| 0.00 | 0.99 | 0.00 | 0.99 | 17.23 | 16.61 | -58.13 | 69.50 | 0.8680 | 406.0 | 370.7 | |
| 0.00 | 1.17 | 0.00 | 1.26 | 19.32 | 14.36 | -60.37 | 67.64 | 0.8889 | 387.0 | 291.5 | |
| 0.00 | 0.99 | 0.00 | 1.02 | 17.05 | 15.53 | -59.21 | 69.92 | 0.8764 | 469.0 | 430.9 | |
| 0.00 | 2.17 | 0.00 | 2.24 | 17.41 | 15.21 | -59.53 | 69.59 | 0.8794 | 520.0 | 396.6 | |
| 1.26 | 2.35 | 1.32 | 2.46 | 17.83 | 14.85 | -59.88 | 69.19 | 0.8828 | 350.8 | 363.3 | |
| 0.00 | 1.36 | 0.00 | 1.40 | 16.29 | 14.91 | -59.83 | 70.90 | 0.8801 | -379.0 | -322.8 | |
| 0.00 | 0.99 | 0.00 | 1.06 | 17.10 | 14.16 | -60.58 | 70.14 | 0.8871 | -285.0 | -215.3 | |
| 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. | |