SDO HMI 2011-09-04 19:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.39 | 110.13 | 22.78 | 138.42 | 22.99 | 303.72 | 67.67 | 292.05 | 0.9186 | -128.3 | -60.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.96 | 90.64 | 2.64 | 120.09 | 22.55 | 305.56 | 69.51 | 291.44 | 0.9310 | 187.7 | -120.0 | |
| 12.32 | -1.00 | 16.27 | -1.00 | 22.57 | 305.11 | 69.06 | 291.47 | 0.9283 | -650.2 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.28 | 24.77 | 299.99 | 63.94 | 294.14 | 0.8956 | -480.0 | -382.7 | |
| 0.00 | 1.79 | 0.00 | 1.70 | 25.14 | 294.70 | 58.65 | 295.10 | 0.8558 | 567.0 | 461.5 | |
| 0.00 | 0.98 | 0.00 | 0.94 | 25.61 | 294.94 | 58.89 | 295.61 | 0.8582 | 533.0 | 418.8 | |
| 1.16 | 1.70 | 1.09 | 1.59 | 25.57 | 294.01 | 57.96 | 295.70 | 0.8506 | 481.4 | 414.7 | |
| 1.16 | 1.61 | 1.09 | 1.51 | 25.82 | 294.14 | 58.09 | 295.97 | 0.8520 | 377.5 | 349.4 | |
| 0.00 | 1.70 | 0.00 | 1.58 | 25.80 | 293.68 | 57.63 | 296.02 | 0.8482 | 475.0 | 402.5 | |
| 1.79 | 3.84 | 1.69 | 3.62 | 26.61 | 294.13 | 58.07 | 296.90 | 0.8529 | 353.2 | 391.6 | |
| 0.00 | 1.79 | 0.00 | 1.63 | 25.30 | 293.12 | 57.06 | 295.51 | 0.8428 | 194.0 | 202.4 | |
| 0.00 | 1.07 | 0.00 | 0.97 | 25.08 | 292.77 | 56.72 | 295.30 | 0.8396 | 519.0 | 439.7 | |
| 0.00 | 1.25 | 0.00 | 1.15 | 26.02 | 293.22 | 57.16 | 296.34 | 0.8446 | 628.0 | 527.4 | |
| 0.00 | 1.52 | 0.00 | 1.39 | 25.83 | 293.08 | 57.02 | 296.14 | 0.8432 | 780.0 | 633.8 | |
| 0.00 | 0.45 | 0.00 | 0.40 | 25.25 | 292.65 | 56.60 | 295.53 | 0.8388 | 516.0 | 493.4 | |
| 0.00 | 0.63 | 0.00 | 0.57 | 26.13 | 292.74 | 56.69 | 296.55 | 0.8408 | 613.0 | 532.3 | |
| 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. | |