SDO HMI 2011-11-15 15:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.24 | 159.38 | 19.80 | 103.69 | 28.25 | 41.21 | 32.87 | 312.54 | 0.6494 | -619.8 | -300.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.32 | 143.47 | 17.89 | 93.98 | 28.28 | 41.90 | 33.56 | 311.92 | 0.6566 | -1063.0 | -337.0 | |
| 2.92 | -1.00 | 1.91 | -1.00 | 28.73 | 41.41 | 33.07 | 312.84 | 0.6550 | -754.9 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.12 | 28.90 | 41.03 | 32.69 | 313.35 | 0.6526 | -747.0 | -610.2 | |
| 0.00 | 0.86 | 0.00 | 0.56 | 29.43 | 41.14 | 32.80 | 313.94 | 0.6576 | -532.0 | -429.5 | |
| 0.00 | 1.12 | 0.00 | 0.73 | 29.01 | 40.59 | 32.25 | 313.83 | 0.6492 | -632.0 | -586.2 | |
| 0.00 | 2.23 | 0.00 | 1.44 | 29.23 | 39.70 | 31.36 | 314.80 | 0.6424 | -208.0 | -292.4 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 25.58 | 37.58 | 29.25 | 311.69 | 0.5923 | -627.0 | -564.3 | |
| 0.00 | 0.95 | 0.00 | 0.61 | 29.96 | 38.72 | 30.38 | 316.51 | 0.6390 | -710.0 | -642.2 | |
| 0.00 | 0.69 | 0.00 | 0.44 | 30.13 | 38.58 | 30.24 | 316.84 | 0.6391 | -587.0 | -493.1 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 27.00 | 36.35 | 28.01 | 314.75 | 0.5914 | 672.0 | 553.8 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 28.27 | 31.91 | 23.57 | 320.90 | 0.5605 | 606.0 | 461.2 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 24.23 | 29.79 | 21.45 | 317.82 | 0.4986 | 725.0 | 583.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 24.88 | 24.95 | 16.62 | 325.49 | 0.4598 | 678.0 | 573.2 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 25.07 | 24.78 | 16.44 | 326.03 | 0.4606 | 769.0 | 632.5 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 24.98 | 22.19 | 13.85 | 330.16 | 0.4380 | 724.0 | 638.5 | |
| 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. | |