SDO HMI 2011-11-12 03:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.77 | 278.40 | 20.84 | 139.01 | 9.71 | 56.58 | 2.12 | 331.94 | 0.1239 | -900.5 | -377.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.22 | 246.29 | 20.06 | 122.85 | 9.42 | 57.12 | 2.66 | 337.03 | 0.1178 | -1526.2 | -462.3 | |
| 0.00 | 1.46 | 0.00 | 0.73 | 11.34 | 56.25 | 1.80 | 347.71 | 0.1451 | -847.0 | -467.9 | |
| 0.00 | 3.27 | 0.00 | 1.63 | 9.90 | 56.22 | 1.76 | 345.42 | 0.1207 | -1034.0 | -795.6 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 11.31 | 56.07 | 1.62 | 348.88 | 0.1439 | -836.0 | -563.2 | |
| 0.00 | 0.95 | 0.00 | 0.47 | 10.11 | 56.07 | 1.61 | 347.01 | 0.1236 | -721.0 | -543.1 | |
| 1.55 | 12.92 | 0.78 | 6.48 | 12.15 | 55.20 | 0.74 | 355.35 | 0.1563 | -861.9 | 286.3 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 11.67 | 54.50 | 0.04 | 359.72 | 0.1475 | 886.0 | 746.8 | |
| 0.00 | 1.38 | 0.00 | 0.69 | 9.84 | 53.39 | -1.07 | 9.10 | 0.1172 | -855.0 | -623.1 | |
| 0.00 | 3.27 | 0.00 | 1.65 | 12.71 | 49.75 | -4.71 | 25.90 | 0.1841 | 987.0 | 815.6 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 11.18 | 45.57 | -8.88 | 47.46 | 0.2066 | 814.0 | 617.8 | |
| 0.00 | 1.89 | 0.00 | 0.96 | 12.02 | 45.45 | -9.00 | 44.92 | 0.2178 | 865.0 | 688.8 | |
| 0.00 | 0.69 | 0.00 | 0.35 | 11.93 | 45.27 | -9.18 | 45.78 | 0.2189 | 756.0 | 661.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 11.91 | 43.55 | -10.91 | 50.62 | 0.2406 | 916.0 | 679.2 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 16.59 | 42.53 | -11.93 | 40.47 | 0.3066 | 784.0 | 620.7 | |
| 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. | |