SDO HMI 2011-11-15 02:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.52 | 289.97 | 26.99 | 219.46 | 16.16 | 63.59 | 48.13 | 288.97 | 0.7586 | -569.2 | -279.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.52 | 274.24 | 26.99 | 208.16 | 16.04 | 63.78 | 48.32 | 288.76 | 0.7604 | -1031.8 | -315.8 | |
| 0.00 | 0.52 | 0.00 | 0.38 | 15.57 | 62.35 | 46.89 | 288.47 | 0.7438 | -774.0 | -691.0 | |
| 0.00 | 2.58 | 0.00 | 1.96 | 18.46 | 63.27 | 47.81 | 292.01 | 0.7604 | 632.0 | 457.0 | |
| 0.00 | 1.20 | 0.00 | 0.91 | 17.64 | 62.92 | 47.47 | 291.04 | 0.7548 | -375.0 | -255.4 | |
| 0.00 | 1.12 | 0.00 | 0.82 | 16.32 | 62.03 | 46.58 | 289.54 | 0.7420 | -745.0 | -568.5 | |
| 0.00 | 0.69 | 0.00 | 0.50 | 16.17 | 61.13 | 45.68 | 289.57 | 0.7316 | 389.0 | 359.0 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 18.44 | 59.51 | 44.06 | 293.11 | 0.7196 | 527.0 | 445.0 | |
| 0.00 | 1.29 | 0.00 | 0.92 | 19.03 | 59.40 | 43.94 | 293.95 | 0.7202 | 466.0 | 391.9 | |
| 0.00 | 0.34 | 0.00 | 0.24 | 19.26 | 59.00 | 43.54 | 294.40 | 0.7164 | 454.0 | 491.2 | |
| 0.00 | 1.03 | 0.00 | 0.72 | 18.97 | 58.51 | 43.06 | 294.17 | 0.7100 | 731.0 | 670.1 | |
| 0.00 | 1.03 | 0.00 | 0.72 | 18.76 | 58.36 | 42.90 | 293.94 | 0.7076 | 641.0 | 507.5 | |
| 0.00 | 1.46 | 0.00 | 1.03 | 19.74 | 58.55 | 43.10 | 295.21 | 0.7131 | 647.0 | 495.2 | |
| 0.00 | 1.89 | 0.00 | 1.30 | 18.28 | 57.66 | 42.20 | 293.54 | 0.6981 | 619.0 | 487.8 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 18.20 | 57.29 | 41.84 | 293.56 | 0.6936 | 718.0 | 584.3 | |
| 0.00 | 0.52 | 0.00 | 0.36 | 20.23 | 57.00 | 41.54 | 296.48 | 0.6976 | 588.0 | 517.8 | |
| 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. | |