SDO HMI 2011-10-22 00:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.36 | 43.16 | 6.35 | 22.13 | 17.78 | 324.86 | -8.15 | 31.72 | 0.2562 | 591.6 | -3.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.53 | 0.00 | 6.38 | 16.98 | 326.76 | -6.25 | 27.29 | 0.2283 | -1299.0 | -977.6 | |
| 2.79 | 3.39 | 1.42 | 1.73 | 17.19 | 326.38 | -6.64 | 28.24 | 0.2344 | -933.3 | -852.3 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 17.07 | 326.13 | -6.89 | 29.38 | 0.2346 | -677.0 | -564.7 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 14.30 | 325.45 | -7.57 | 39.26 | 0.2026 | 933.0 | 757.3 | |
| 0.00 | 2.52 | 0.00 | 1.29 | 18.16 | 325.27 | -7.75 | 29.97 | 0.2577 | 906.0 | 677.3 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 17.54 | 324.85 | -8.17 | 32.59 | 0.2526 | 1066.0 | 792.4 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 14.32 | 324.95 | -8.07 | 40.95 | 0.2084 | 867.0 | 640.5 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 18.17 | 324.25 | -8.77 | 33.02 | 0.2669 | 899.0 | 697.8 | |
| 1.39 | 5.05 | 0.72 | 2.60 | 18.78 | 324.00 | -9.02 | 32.48 | 0.2777 | 1055.1 | 892.0 | |
| 8.18 | 8.53 | 4.21 | 4.39 | 18.45 | 323.95 | -9.07 | 33.31 | 0.2734 | 1124.7 | 869.0 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 18.29 | 323.51 | -9.50 | 34.88 | 0.2754 | 983.0 | 810.6 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 19.19 | 322.69 | -10.33 | 35.14 | 0.2954 | 713.0 | 687.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 20.16 | 319.80 | -13.21 | 39.78 | 0.3368 | 913.0 | 775.6 | |
| 0.00 | 1.39 | 0.00 | 0.75 | 23.02 | 318.43 | -14.59 | 37.13 | 0.3856 | 790.0 | 638.6 | |
| 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. | |