SDO HMI 2011-10-21 18:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.63 | 230.65 | 71.37 | 516.08 | 9.28 | 53.88 | 77.55 | 278.34 | 0.9733 | 57.8 | -28.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.87 | 137.47 | 8.20 | 365.70 | 7.81 | 56.91 | 80.58 | 277.00 | 0.9855 | 508.5 | 0.1 | |
| 5.83 | -1.00 | 15.30 | -1.00 | 8.47 | 56.01 | 79.68 | 277.61 | 0.9826 | 348.2 | 999999 | |
| 12.27 | -1.00 | 30.71 | -1.00 | 8.51 | 55.54 | 79.21 | 277.62 | 0.9811 | -452.8 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.98 | 9.22 | 54.38 | 78.05 | 278.27 | 0.9768 | -440.0 | -460.2 | |
| 0.00 | 12.09 | 0.00 | 26.94 | 9.75 | 54.21 | 77.88 | 278.81 | 0.9761 | -637.0 | -504.4 | |
| 0.00 | 11.57 | 0.00 | 19.80 | 9.64 | 50.09 | 73.76 | 278.47 | 0.9583 | -341.0 | -215.8 | |
| 0.00 | 1.04 | 0.00 | 1.66 | 10.36 | 48.82 | 72.49 | 279.16 | 0.9516 | -25.0 | 36.3 | |
| 0.00 | 1.65 | 0.00 | 2.63 | 10.66 | 48.89 | 72.56 | 279.48 | 0.9519 | 16.0 | 63.1 | |
| 0.00 | 1.74 | 0.00 | 2.70 | 10.43 | 48.35 | 72.02 | 279.22 | 0.9491 | 388.0 | 338.5 | |
| 10.53 | 52.38 | 15.50 | 77.63 | 12.14 | 47.34 | 71.01 | 280.99 | 0.9432 | 551.3 | 46.4 | |
| 0.00 | 5.83 | 0.00 | 8.79 | 13.87 | 47.85 | 71.52 | 282.83 | 0.9458 | -219.0 | -134.8 | |
| 0.00 | 0.87 | 0.00 | 1.27 | 13.15 | 47.24 | 70.91 | 282.07 | 0.9425 | 555.0 | 516.2 | |
| 1.13 | 4.79 | 1.66 | 7.07 | 13.39 | 47.31 | 70.98 | 282.32 | 0.9429 | 462.5 | 333.7 | |
| 0.00 | 0.78 | 0.00 | 0.91 | 9.21 | 41.50 | 65.17 | 277.66 | 0.9057 | 439.0 | 383.9 | |
| 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. | |