SDO HMI 2011-12-07 15:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.77 | 135.77 | 27.18 | 119.39 | 7.47 | 133.46 | 55.08 | 279.13 | 0.8224 | -157.9 | 21.1 | |
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back to the solar disc SDO HMI 2011-12-07 15:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.65 | 67.93 | 10.28 | 65.89 | 7.21 | 137.22 | 58.83 | 278.36 | 0.8601 | -698.2 | -61.7 | |
| 9.55 | 11.93 | 8.99 | 11.22 | 7.10 | 136.39 | 58.01 | 278.29 | 0.8526 | -685.6 | -533.9 | |
| 0.00 | 1.02 | 0.00 | 0.94 | 5.88 | 135.66 | 57.28 | 276.91 | 0.8452 | -568.0 | -419.6 | |
| 0.00 | 0.77 | 0.00 | 0.69 | 5.25 | 134.70 | 56.32 | 276.24 | 0.8357 | 324.0 | 293.8 | |
| 0.00 | 1.11 | 0.00 | 0.90 | 7.01 | 130.27 | 51.89 | 278.81 | 0.7925 | -588.0 | -498.2 | |
| 0.00 | 1.11 | 0.00 | 0.88 | 8.27 | 129.42 | 51.04 | 280.51 | 0.7850 | -623.0 | -489.5 | |
| 0.00 | 1.02 | 0.00 | 0.79 | 10.63 | 127.41 | 49.03 | 283.89 | 0.7668 | 618.0 | 500.7 | |
| 3.15 | 47.73 | 2.37 | 35.83 | 8.45 | 126.63 | 48.25 | 281.17 | 0.7545 | 561.4 | 225.5 | |
| 0.60 | -8.00 | 0.45 | -8.00 | 8.15 | 126.49 | 48.11 | 280.80 | 0.7525 | 762.6 | 999999 | |
| 6.82 | -8.00 | 5.09 | -8.00 | 7.85 | 126.40 | 48.02 | 280.42 | 0.7511 | 869.2 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.63 | 6.51 | 125.85 | 47.47 | 278.72 | 0.7431 | 513.0 | 448.2 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 7.91 | 122.77 | 44.39 | 281.14 | 0.7086 | 593.0 | 522.5 | |
| 0.00 | 1.36 | 0.00 | 0.96 | 8.84 | 122.91 | 44.53 | 282.41 | 0.7118 | 498.0 | 348.9 | |
| 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. | |