| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.07 | 34.66 | 4.99 | 18.84 | -20.06 | 69.80 | 20.64 | 233.72 | 0.4108 | 190.9 | 215.4 | |
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back to the solar disc SDO HMI 2011-02-12 23:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 6.25 | 0.00 | 3.45 | -20.22 | 72.36 | 23.20 | 236.77 | 0.4439 | 905.0 | 788.4 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -20.62 | 72.29 | 23.13 | 235.90 | 0.4459 | 737.0 | 441.8 | |
| 7.10 | 8.64 | 3.91 | 4.75 | -19.97 | 71.88 | 22.72 | 236.79 | 0.4357 | 950.4 | 728.6 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -19.40 | 71.55 | 22.40 | 237.63 | 0.4273 | 872.0 | 753.1 | |
| 1.97 | 2.91 | 1.08 | 1.59 | -20.18 | 71.19 | 22.04 | 235.65 | 0.4284 | 929.3 | 820.9 | |
| 0.00 | 3.00 | 0.00 | 1.64 | -20.14 | 70.74 | 21.59 | 235.25 | 0.4222 | 938.0 | 762.9 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -18.10 | 70.16 | 21.01 | 239.03 | 0.3992 | 798.0 | 563.1 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -18.71 | 69.18 | 20.02 | 236.53 | 0.3904 | -725.0 | -566.2 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -19.65 | 69.20 | 20.04 | 234.48 | 0.3982 | -763.0 | -616.3 | |
| 0.00 | 1.46 | 0.00 | 0.77 | -20.29 | 64.67 | 15.52 | 226.44 | 0.3478 | -905.0 | -734.2 | |
| 0.00 | 2.05 | 0.00 | 1.08 | -20.55 | 63.36 | 14.20 | 223.49 | 0.3353 | -752.0 | -750.0 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -20.59 | 63.04 | 13.88 | 222.78 | 0.3321 | -1093.0 | -846.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -21.08 | 62.92 | 13.76 | 221.49 | 0.3366 | -703.0 | -587.7 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -21.03 | 59.77 | 10.61 | 214.63 | 0.3038 | -786.0 | -602.4 | |
| 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. | |