| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.49 | 266.36 | 17.14 | 136.64 | 16.93 | 168.79 | 8.26 | 326.95 | 0.2584 | -456.1 | -353.4 | |
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back to the solar disc SDO HMI 2011-07-18 01:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.87 | 244.85 | 11.71 | 125.43 | 16.51 | 169.29 | 8.76 | 324.89 | 0.2549 | -1353.1 | -445.5 | |
| 7.53 | -1.00 | 3.85 | -1.00 | 16.17 | 169.15 | 8.61 | 324.52 | 0.2489 | -1408.4 | 999999 | |
| 3.09 | -1.00 | 1.58 | -1.00 | 16.80 | 169.02 | 8.48 | 326.39 | 0.2561 | -932.8 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 16.18 | 168.41 | 7.87 | 326.89 | 0.2419 | -560.0 | -379.8 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.46 | 168.05 | 7.51 | 330.85 | 0.2571 | -673.0 | -517.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 20.98 | 166.14 | 5.60 | 342.11 | 0.2982 | 825.0 | 655.6 | |
| 0.00 | 3.90 | 0.00 | 2.05 | 23.78 | 163.92 | 3.38 | 350.68 | 0.3347 | 855.0 | 668.2 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 23.04 | 163.87 | 3.33 | 350.42 | 0.3225 | 918.0 | 741.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 23.10 | 163.64 | 3.10 | 351.10 | 0.3229 | 985.0 | 763.2 | |
| 0.00 | 2.99 | 0.00 | 1.57 | 23.62 | 163.55 | 3.01 | 351.61 | 0.3311 | 592.0 | 585.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 17.59 | 163.21 | 2.67 | 348.84 | 0.2305 | 887.0 | 704.6 | |
| 0.00 | 2.18 | 0.00 | 1.14 | 23.49 | 163.25 | 2.71 | 352.38 | 0.3284 | 777.0 | 600.7 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 23.84 | 162.79 | 2.25 | 353.79 | 0.3333 | 795.0 | 631.0 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 23.43 | 162.65 | 2.11 | 354.03 | 0.3262 | 698.0 | 578.7 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 22.94 | 162.41 | 1.87 | 354.55 | 0.3178 | 847.0 | 700.9 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 23.20 | 162.15 | 1.61 | 355.38 | 0.3217 | 860.0 | 691.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 23.17 | 158.60 | -1.94 | 5.57 | 0.3216 | 733.0 | 588.5 | |
| 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. | |