SDO HMI 2011-07-24 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.32 | 43.26 | 10.09 | 22.72 | 24.38 | 78.62 | 0.21 | 359.14 | 0.3335 | -484.4 | -214.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.53 | 7.98 | 3.93 | 4.17 | 23.53 | 81.08 | 2.67 | 352.29 | 0.3197 | -905.7 | -827.8 | |
| 8.07 | 9.62 | 4.22 | 5.03 | 23.63 | 80.62 | 2.21 | 353.65 | 0.3204 | -933.7 | -220.1 | |
| 3.72 | 5.17 | 1.94 | 2.70 | 23.66 | 80.25 | 1.84 | 354.71 | 0.3203 | -970.7 | -734.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 22.60 | 79.68 | 1.26 | 356.11 | 0.3021 | -878.0 | -648.5 | |
| 0.00 | 2.18 | 0.00 | 1.14 | 23.53 | 78.96 | 0.54 | 358.42 | 0.3170 | -997.0 | -824.7 | |
| 0.00 | 2.27 | 0.00 | 1.21 | 26.84 | 77.54 | -0.88 | 2.11 | 0.3715 | -742.0 | -594.5 | |
| 0.00 | 1.72 | 0.00 | 0.92 | 27.40 | 77.33 | -1.09 | 2.54 | 0.3807 | -922.0 | -628.1 | |
| 0.00 | 3.63 | 0.00 | 1.92 | 25.44 | 77.31 | -1.10 | 2.87 | 0.3488 | -488.0 | -536.9 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 25.80 | 77.27 | -1.14 | 2.90 | 0.3547 | -902.0 | -646.9 | |
| 0.00 | 1.72 | 0.00 | 0.92 | 27.23 | 75.03 | -3.38 | 7.94 | 0.3814 | 753.0 | 525.4 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 26.73 | 74.64 | -3.78 | 9.08 | 0.3744 | 801.0 | 603.0 | |
| 0.00 | 2.63 | 0.00 | 1.37 | 23.00 | 73.56 | -4.86 | 14.25 | 0.3181 | 902.0 | 644.5 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 24.45 | 73.37 | -5.05 | 13.60 | 0.3419 | 872.0 | 604.8 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 25.47 | 71.56 | -6.85 | 17.20 | 0.3658 | 768.0 | 606.5 | |
| 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. | |