SDO HMI 2011-11-30 02:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.48 | 58.55 | 11.54 | 43.48 | 18.27 | 223.54 | 45.80 | 293.90 | 0.7470 | -290.5 | -209.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 1.26 | 15.44 | 226.67 | 48.93 | 289.31 | 0.7723 | 529.0 | 467.9 | |
| 2.14 | 8.98 | 1.61 | 6.78 | 17.93 | 224.54 | 46.80 | 293.11 | 0.7564 | -732.7 | -478.9 | |
| 0.00 | 0.77 | 0.00 | 0.57 | 16.73 | 224.14 | 46.40 | 291.68 | 0.7487 | -482.0 | -333.4 | |
| 0.00 | 0.34 | 0.00 | 0.25 | 14.99 | 223.58 | 45.84 | 289.57 | 0.7378 | 542.0 | 567.8 | |
| 0.00 | 1.20 | 0.00 | 0.89 | 17.57 | 223.87 | 46.13 | 292.85 | 0.7482 | -602.0 | -484.5 | |
| 0.00 | 1.37 | 0.00 | 1.02 | 17.94 | 224.00 | 46.26 | 293.29 | 0.7507 | -672.0 | -523.5 | |
| 0.00 | 2.39 | 0.00 | 1.74 | 16.13 | 223.16 | 45.42 | 291.20 | 0.7362 | 478.0 | 386.1 | |
| 13.34 | 34.28 | 9.93 | 25.52 | 18.32 | 223.72 | 45.98 | 293.87 | 0.7489 | -790.1 | -360.5 | |
| 0.00 | 1.88 | 0.00 | 1.41 | 20.98 | 223.12 | 45.38 | 297.50 | 0.7516 | -647.0 | -506.6 | |
| 0.00 | 1.62 | 0.00 | 1.18 | 20.21 | 221.59 | 43.85 | 297.13 | 0.7328 | 544.0 | 401.5 | |
| 0.00 | 1.62 | 0.00 | 1.15 | 19.20 | 220.29 | 42.55 | 296.32 | 0.7149 | 532.0 | 380.2 | |
| 0.00 | 0.94 | 0.00 | 0.65 | 18.83 | 219.42 | 41.68 | 296.21 | 0.7038 | 701.0 | 622.9 | |
| 0.00 | 0.51 | 0.00 | 0.35 | 20.48 | 217.27 | 39.53 | 299.45 | 0.6870 | 602.0 | 494.5 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 22.25 | 217.72 | 39.98 | 301.58 | 0.7004 | 663.0 | 541.3 | |
| 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. | |