SDO HMI 2011-08-08 06:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.99 | 33.15 | 0.53 | 17.59 | 19.63 | 224.41 | -15.62 | 45.94 | 0.3475 | -376.8 | -415.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.07 | 0.00 | 1.56 | 15.81 | 231.52 | -8.51 | 40.41 | 0.2206 | -671.0 | -663.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 16.99 | 230.05 | -9.98 | 41.40 | 0.2517 | -745.0 | -677.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 16.83 | 229.89 | -10.13 | 42.26 | 0.2515 | -729.0 | -551.9 | |
| 0.00 | 2.62 | 0.00 | 1.37 | 19.55 | 226.24 | -13.79 | 43.94 | 0.3251 | -874.0 | -778.9 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 18.84 | 226.26 | -13.76 | 45.55 | 0.3168 | -816.0 | -609.6 | |
| 0.00 | 3.43 | 0.00 | 1.80 | 19.70 | 225.99 | -14.04 | 44.09 | 0.3296 | -706.0 | -755.9 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 18.64 | 225.95 | -14.08 | 46.64 | 0.3184 | -603.0 | -726.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 19.10 | 225.71 | -14.32 | 46.00 | 0.3262 | -629.0 | -609.2 | |
| 0.99 | 4.97 | 0.53 | 2.63 | 20.85 | 225.48 | -14.55 | 42.59 | 0.3483 | -962.2 | -806.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 21.32 | 225.33 | -14.69 | 41.91 | 0.3553 | -652.0 | -576.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 19.41 | 225.52 | -14.51 | 45.66 | 0.3318 | -708.0 | -527.0 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 20.81 | 225.15 | -14.88 | 43.29 | 0.3516 | -737.0 | -553.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 20.24 | 225.00 | -15.02 | 44.76 | 0.3469 | -964.0 | -757.3 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 18.71 | 220.88 | -19.14 | 54.52 | 0.3831 | 804.0 | 694.6 | |
| 0.00 | 3.16 | 0.00 | 1.80 | 22.13 | 214.45 | -25.57 | 54.66 | 0.4922 | 702.0 | 541.7 | |
| 0.00 | 1.63 | 0.00 | 0.92 | 21.60 | 214.45 | -25.58 | 55.63 | 0.4883 | 900.0 | 698.8 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 22.09 | 214.21 | -25.82 | 54.96 | 0.4949 | 709.0 | 546.5 | |
| 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. | |