SDO HMI 2011-08-08 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.77 | 0.00 | 13.52 | 19.92 | 223.84 | -13.44 | 41.59 | 0.3266 | -512.5 | -493.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.70 | 19.17 | 226.26 | -11.02 | 38.68 | 0.2902 | -979.0 | -788.6 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 19.58 | 226.17 | -11.11 | 38.00 | 0.2963 | -962.0 | -731.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.76 | 225.99 | -11.29 | 40.29 | 0.2879 | -871.0 | -714.2 | |
| 0.00 | 1.99 | 0.00 | 1.03 | 19.63 | 225.93 | -11.35 | 38.44 | 0.2994 | -1029.0 | -771.0 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 18.54 | 226.01 | -11.27 | 40.77 | 0.2851 | -832.0 | -631.2 | |
| 0.00 | 2.62 | 0.00 | 1.36 | 19.01 | 225.85 | -11.44 | 40.07 | 0.2925 | -745.0 | -725.3 | |
| 0.00 | 5.24 | 0.00 | 2.74 | 20.72 | 225.52 | -11.76 | 37.10 | 0.3174 | -1075.0 | -802.5 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 19.47 | 225.55 | -11.73 | 39.71 | 0.3014 | -746.0 | -572.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 21.65 | 224.78 | -12.51 | 36.91 | 0.3366 | -661.0 | -421.9 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 18.17 | 224.40 | -12.88 | 45.38 | 0.2990 | -791.0 | -596.3 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 20.97 | 221.58 | -15.70 | 44.42 | 0.3627 | -838.0 | -695.1 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 18.04 | 218.89 | -18.39 | 55.05 | 0.3675 | 735.0 | 484.7 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 21.57 | 214.33 | -22.95 | 53.10 | 0.4553 | 860.0 | 712.3 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 22.27 | 214.18 | -23.10 | 51.98 | 0.4629 | 759.0 | 652.3 | |
| 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. | |