SDO HMI 2011-10-14 10:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.46 | 73.70 | 11.54 | 41.54 | 19.87 | 98.64 | 25.58 | 301.73 | 0.4792 | -353.0 | -377.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.85 | 0.00 | 2.18 | 19.29 | 99.59 | 26.53 | 299.79 | 0.4877 | -22.0 | -50.6 | |
| 3.15 | 7.43 | 1.79 | 4.23 | 20.25 | 99.62 | 26.56 | 301.55 | 0.4942 | -686.2 | -495.8 | |
| 2.62 | 42.31 | 1.49 | 23.92 | 19.83 | 99.36 | 26.30 | 300.97 | 0.4881 | -686.0 | -561.2 | |
| 7.17 | -3.00 | 4.06 | -3.00 | 19.55 | 99.25 | 26.18 | 300.56 | 0.4848 | -1058.7 | 999999 | |
| 0.00 | 3.32 | 0.00 | 1.88 | 20.11 | 99.27 | 26.21 | 301.57 | 0.4888 | -737.0 | -664.8 | |
| 2.54 | -3.00 | 1.43 | -3.00 | 19.57 | 98.96 | 25.90 | 300.81 | 0.4812 | -1107.8 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 20.00 | 98.97 | 25.91 | 301.62 | 0.4841 | -853.0 | -742.9 | |
| 0.35 | 1.66 | 0.20 | 0.93 | 19.78 | 98.33 | 25.27 | 301.76 | 0.4743 | -906.5 | -722.1 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 19.40 | 97.81 | 24.75 | 301.48 | 0.4650 | -667.0 | -477.1 | |
| 0.00 | 1.66 | 0.00 | 0.92 | 19.64 | 97.12 | 24.06 | 302.59 | 0.4576 | -927.0 | -739.3 | |
| 4.11 | 6.21 | 2.28 | 3.45 | 21.02 | 96.09 | 23.03 | 306.27 | 0.4548 | 922.9 | 697.8 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 20.90 | 95.79 | 22.73 | 306.37 | 0.4501 | 980.0 | 816.5 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 20.43 | 95.06 | 22.00 | 306.26 | 0.4372 | 676.0 | 481.5 | |
| 0.52 | 2.80 | 0.29 | 1.54 | 20.54 | 94.60 | 21.53 | 307.00 | 0.4322 | 1097.0 | 852.5 | |
| 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. | |