SDO HMI 2011-11-14 05:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.59 | 79.86 | 16.01 | 51.95 | 8.25 | 346.81 | -40.19 | 80.76 | 0.6491 | 346.5 | -43.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.86 | 7.69 | 349.19 | -37.81 | 81.30 | 0.6168 | 744.0 | 573.8 | |
| 1.46 | 29.43 | 0.92 | 18.66 | 7.95 | 348.90 | -38.10 | 80.92 | 0.6211 | 452.2 | -321.7 | |
| 6.71 | -2.00 | 4.25 | -2.00 | 8.03 | 348.54 | -38.45 | 80.85 | 0.6260 | -859.6 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.60 | 8.50 | 348.18 | -38.81 | 80.17 | 0.6315 | 624.0 | 563.5 | |
| 0.00 | 1.38 | 0.00 | 0.89 | 8.64 | 347.07 | -39.92 | 80.11 | 0.6464 | -497.0 | -367.6 | |
| 0.00 | 2.32 | 0.00 | 1.52 | 8.74 | 346.43 | -40.57 | 80.06 | 0.6549 | 675.0 | 513.2 | |
| 1.46 | 5.94 | 0.96 | 3.89 | 8.02 | 346.36 | -40.63 | 81.17 | 0.6549 | 865.8 | 796.5 | |
| 1.20 | -7.00 | 0.79 | -7.00 | 7.92 | 346.14 | -40.86 | 81.34 | 0.6578 | 848.6 | 999999 | |
| 10.32 | 30.80 | 6.82 | 20.39 | 8.44 | 345.67 | -41.32 | 80.61 | 0.6644 | 812.3 | -79.4 | |
| 3.44 | -9.00 | 2.27 | -9.00 | 8.14 | 345.63 | -41.37 | 81.07 | 0.6646 | 710.4 | 999999 | |
| 0.00 | 3.36 | 0.00 | 2.23 | 8.31 | 345.29 | -41.71 | 80.86 | 0.6692 | -48.0 | -46.3 | |
| 0.00 | 2.32 | 0.00 | 1.55 | 8.45 | 345.11 | -41.89 | 80.67 | 0.6716 | -75.0 | -75.7 | |
| 0.00 | 0.95 | 0.00 | 0.65 | 9.24 | 343.56 | -43.44 | 79.72 | 0.6920 | 813.0 | 747.1 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 9.65 | 343.37 | -43.63 | 79.16 | 0.6949 | 666.0 | 569.2 | |
| 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. | |