SDO HMI 2011-11-29 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.58 | 98.01 | 18.72 | 61.88 | 18.06 | 223.80 | 35.06 | 298.33 | 0.6228 | -559.7 | -323.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.60 | 15.53 | 226.15 | 37.41 | 293.33 | 0.6398 | 524.0 | 451.7 | |
| 0.00 | 1.03 | 0.00 | 0.64 | 14.12 | 224.15 | 35.42 | 292.09 | 0.6089 | 624.0 | 503.5 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 19.65 | 225.27 | 36.53 | 299.80 | 0.6484 | 722.0 | 602.9 | |
| 9.06 | 22.92 | 5.77 | 14.59 | 17.89 | 224.52 | 35.78 | 297.66 | 0.6305 | -769.1 | -408.8 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 13.64 | 223.51 | 34.78 | 291.63 | 0.5986 | 574.0 | 541.6 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 17.86 | 224.16 | 35.43 | 297.82 | 0.6262 | -845.0 | -725.5 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 17.52 | 223.97 | 35.24 | 297.42 | 0.6221 | -727.0 | -537.1 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 17.77 | 223.84 | 35.10 | 297.87 | 0.6218 | -799.0 | -715.0 | |
| 0.00 | 1.20 | 0.00 | 0.74 | 15.11 | 223.10 | 34.37 | 294.17 | 0.5996 | 728.0 | 542.4 | |
| 0.00 | 1.80 | 0.00 | 1.13 | 17.71 | 223.60 | 34.86 | 297.92 | 0.6185 | -857.0 | -772.7 | |
| 20.52 | 62.77 | 12.95 | 39.56 | 18.24 | 223.60 | 34.87 | 298.70 | 0.6213 | -944.9 | -363.8 | |
| 0.00 | 1.11 | 0.00 | 0.71 | 21.25 | 222.74 | 34.01 | 303.64 | 0.6285 | -577.0 | -437.3 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 19.62 | 219.18 | 30.45 | 303.80 | 0.5766 | 673.0 | 518.0 | |
| 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. | |