SDO HMI 2011-12-07 17:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.31 | 37.49 | 13.23 | 34.98 | 17.45 | 133.14 | 55.86 | 291.09 | 0.8423 | 152.3 | -180.9 | |
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back to the solar disc SDO HMI 2011-12-07 17:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.66 | 8.69 | 4.01 | 9.50 | 16.90 | 139.10 | 61.82 | 288.97 | 0.8938 | -285.0 | -282.2 | |
| 0.00 | 3.07 | 0.00 | 3.29 | 17.05 | 138.40 | 61.12 | 289.26 | 0.8887 | -350.0 | -320.2 | |
| 0.00 | 1.19 | 0.00 | 1.25 | 16.37 | 137.84 | 60.56 | 288.59 | 0.8836 | -215.0 | -168.2 | |
| 0.00 | 0.51 | 0.00 | 0.55 | 17.42 | 138.35 | 61.08 | 289.68 | 0.8889 | -210.0 | -260.7 | |
| 0.68 | 8.44 | 0.70 | 8.60 | 16.31 | 137.12 | 59.84 | 288.65 | 0.8778 | 318.0 | 267.6 | |
| 4.35 | -5.00 | 4.42 | -5.00 | 16.43 | 136.75 | 59.48 | 288.85 | 0.8751 | 549.7 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.68 | 18.17 | 126.40 | 49.12 | 293.40 | 0.7851 | -532.0 | -427.5 | |
| 0.00 | 2.39 | 0.00 | 1.90 | 18.39 | 126.39 | 49.11 | 293.67 | 0.7856 | -602.0 | -484.0 | |
| 0.00 | 3.83 | 0.00 | 2.99 | 19.58 | 124.91 | 47.64 | 295.63 | 0.7745 | -732.0 | -544.2 | |
| 5.62 | 5.97 | 4.10 | 4.35 | 18.26 | 121.69 | 44.41 | 295.17 | 0.7366 | 724.2 | 580.5 | |
| 0.00 | 0.85 | 0.00 | 0.62 | 18.73 | 121.58 | 44.30 | 295.82 | 0.7372 | 462.0 | 386.9 | |
| 0.00 | 1.02 | 0.00 | 0.75 | 20.30 | 121.20 | 43.93 | 297.99 | 0.7392 | 440.0 | 352.8 | |
| 0.00 | 0.68 | 0.00 | 0.50 | 20.74 | 120.79 | 43.52 | 298.73 | 0.7367 | 647.0 | 558.8 | |
| 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. | |