SDO HMI 2011-08-30 17:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.79 | 36.58 | 7.17 | 19.09 | 24.73 | 299.14 | -4.07 | 11.75 | 0.3130 | -253.3 | 7.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.52 | 25.66 | 307.10 | 3.89 | 349.10 | 0.3249 | 839.0 | 669.7 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 21.38 | 303.52 | 0.32 | 358.79 | 0.2469 | -844.0 | -657.6 | |
| 7.70 | 10.47 | 4.00 | 5.45 | 24.68 | 300.67 | -2.54 | 7.60 | 0.3053 | -1053.8 | -734.7 | |
| 6.09 | 8.95 | 3.17 | 4.66 | 24.90 | 300.10 | -3.11 | 9.16 | 0.3102 | -929.3 | -665.0 | |
| 0.00 | 1.25 | 0.00 | 0.65 | 24.35 | 298.68 | -4.53 | 13.65 | 0.3059 | -707.0 | -594.8 | |
| 0.00 | 1.52 | 0.00 | 0.79 | 24.19 | 298.38 | -4.82 | 14.64 | 0.3045 | -761.0 | -582.4 | |
| 0.00 | 3.49 | 0.00 | 1.83 | 25.35 | 297.23 | -5.97 | 16.73 | 0.3281 | 710.0 | 783.6 | |
| 0.00 | 1.70 | 0.00 | 0.89 | 25.15 | 296.73 | -6.47 | 18.23 | 0.3275 | 865.0 | 549.4 | |
| 0.00 | 1.43 | 0.00 | 0.75 | 25.47 | 296.35 | -6.86 | 18.89 | 0.3344 | 817.0 | 690.1 | |
| 0.00 | 1.43 | 0.00 | 0.75 | 25.21 | 295.92 | -7.28 | 20.25 | 0.3327 | 917.0 | 588.1 | |
| 0.00 | 1.70 | 0.00 | 0.90 | 25.93 | 295.34 | -7.87 | 20.87 | 0.3471 | -890.0 | -590.9 | |
| 0.00 | 0.98 | 0.00 | 0.51 | 20.69 | 294.79 | -8.41 | 30.18 | 0.2733 | 739.0 | 568.0 | |
| 0.00 | 1.25 | 0.00 | 0.66 | 25.84 | 293.91 | -9.29 | 24.29 | 0.3547 | 873.0 | 735.0 | |
| 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. | |