SDO HMI 2011-05-05 17:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.20 | 327.31 | 27.20 | 177.27 | 17.97 | 60.95 | 10.01 | 335.85 | 0.4061 | -894.6 | -357.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.34 | 307.84 | 0.73 | 166.70 | 18.35 | 61.38 | 10.44 | 335.37 | 0.4142 | -393.9 | -419.8 | |
| 43.33 | -1.00 | 23.47 | -1.00 | 17.83 | 61.22 | 10.28 | 335.14 | 0.4056 | -1398.0 | 999999 | |
| 3.39 | -1.00 | 1.84 | -1.00 | 18.25 | 60.85 | 9.91 | 336.35 | 0.4093 | -1030.9 | 999999 | |
| 1.16 | -1.00 | 0.63 | -1.00 | 17.53 | 60.68 | 9.74 | 335.96 | 0.3978 | -1060.0 | 999999 | |
| 0.98 | -1.00 | 0.53 | -1.00 | 18.41 | 60.60 | 9.66 | 337.04 | 0.4101 | -689.0 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.73 | 19.48 | 59.50 | 8.56 | 340.37 | 0.4194 | -751.0 | -566.6 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 21.70 | 59.63 | 8.68 | 341.88 | 0.4530 | -653.0 | -457.9 | |
| 0.00 | 6.70 | 0.00 | 3.59 | 17.66 | 57.77 | 6.83 | 342.72 | 0.3832 | 767.0 | 683.0 | |
| 0.00 | 3.39 | 0.00 | 1.82 | 17.47 | 57.51 | 6.57 | 343.19 | 0.3790 | 250.0 | 380.7 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 18.51 | 57.52 | 6.58 | 343.97 | 0.3951 | 778.0 | 636.4 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 17.92 | 57.37 | 6.43 | 343.88 | 0.3853 | 822.0 | 694.2 | |
| 0.00 | 1.79 | 0.00 | 0.96 | 18.82 | 55.61 | 4.66 | 348.65 | 0.3927 | 944.0 | 784.3 | |
| 0.00 | 2.32 | 0.00 | 1.30 | 23.90 | 55.51 | 4.57 | 351.08 | 0.4712 | 787.0 | 656.8 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 25.80 | 55.48 | 4.54 | 351.78 | 0.4998 | 698.0 | 591.6 | |
| 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. | |