| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.05 | 59.72 | 28.63 | 61.06 | 19.48 | 87.23 | 60.23 | 290.67 | 0.8764 | -128.9 | -119.3 | |
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back to the solar disc SDO HMI 2011-11-14 05:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.69 | 23.32 | 0.74 | 24.88 | 19.38 | 89.11 | 62.11 | 290.30 | 0.8909 | 169.1 | -329.4 | |
| 0.00 | 0.86 | 0.00 | 0.94 | 19.78 | 89.31 | 62.32 | 290.72 | 0.8928 | -174.0 | -167.4 | |
| 6.02 | -1.00 | 6.47 | -1.00 | 19.33 | 88.87 | 61.88 | 290.27 | 0.8891 | -450.3 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.39 | 19.67 | 88.97 | 61.97 | 290.64 | 0.8901 | -368.0 | -330.1 | |
| 5.08 | -1.00 | 5.35 | -1.00 | 19.26 | 88.30 | 61.30 | 290.27 | 0.8847 | -712.7 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.70 | 18.69 | 86.98 | 59.98 | 289.81 | 0.8738 | -526.0 | -439.6 | |
| 9.29 | 13.42 | 9.13 | 13.17 | 18.33 | 86.02 | 59.03 | 289.52 | 0.8656 | 532.8 | 308.9 | |
| 0.00 | 3.96 | 0.00 | 3.93 | 19.35 | 86.18 | 59.18 | 290.67 | 0.8681 | 549.0 | 300.9 | |
| 0.00 | 0.95 | 0.00 | 0.92 | 18.71 | 85.75 | 58.75 | 290.01 | 0.8638 | -332.0 | -302.9 | |
| 0.00 | 0.95 | 0.00 | 0.95 | 20.02 | 86.53 | 59.53 | 291.39 | 0.8717 | 401.0 | 268.5 | |
| 0.00 | 0.77 | 0.00 | 0.74 | 18.61 | 85.15 | 58.16 | 289.98 | 0.8587 | 344.0 | 277.8 | |
| 1.98 | 10.24 | 2.00 | 10.30 | 21.31 | 86.61 | 59.61 | 292.84 | 0.8740 | -460.1 | -396.6 | |
| 0.00 | 0.95 | 0.00 | 0.90 | 19.00 | 84.89 | 57.89 | 290.47 | 0.8570 | 535.0 | 408.4 | |
| 3.96 | -12.00 | 3.96 | -12.00 | 21.36 | 86.26 | 59.26 | 292.95 | 0.8713 | -611.3 | 999999 | |
| 1.03 | 1.55 | 0.98 | 1.48 | 19.66 | 84.73 | 57.73 | 291.26 | 0.8565 | 336.8 | 344.2 | |
| 0.00 | 0.77 | 0.00 | 0.76 | 21.55 | 85.57 | 58.57 | 293.28 | 0.8661 | -534.0 | -416.2 | |
| 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. | |