| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.10 | 74.97 | 26.75 | 79.25 | 18.70 | 315.12 | 61.03 | 290.32 | 0.8847 | -195.8 | -142.7 | |
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back to the solar disc SDO HMI 2011-11-24 07:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.34 | 30.33 | 14.13 | 34.60 | 18.70 | 317.60 | 63.51 | 289.94 | 0.9036 | -625.1 | -391.0 | |
| 0.00 | 1.11 | 0.00 | 1.23 | 17.45 | 316.65 | 62.56 | 288.68 | 0.8956 | -501.0 | -443.7 | |
| 0.00 | 3.86 | 0.00 | 4.25 | 17.70 | 316.60 | 62.51 | 288.96 | 0.8955 | -351.0 | -415.1 | |
| 0.00 | 1.37 | 0.00 | 1.61 | 20.00 | 318.18 | 64.09 | 291.29 | 0.9089 | -357.0 | -280.6 | |
| 0.00 | 0.77 | 0.00 | 0.84 | 17.87 | 316.36 | 62.27 | 289.18 | 0.8939 | -527.0 | -478.6 | |
| 0.00 | 1.46 | 0.00 | 1.47 | 17.19 | 313.84 | 59.75 | 288.77 | 0.8737 | 227.0 | 269.2 | |
| 0.00 | 1.20 | 0.00 | 1.20 | 16.92 | 313.51 | 59.42 | 288.52 | 0.8707 | -467.0 | -436.3 | |
| 0.00 | 1.20 | 0.00 | 1.21 | 17.53 | 313.84 | 59.75 | 289.16 | 0.8740 | 356.0 | 280.9 | |
| 4.71 | 5.91 | 4.87 | 6.11 | 19.20 | 314.30 | 60.21 | 290.97 | 0.8798 | -423.8 | -329.6 | |
| 0.00 | 0.69 | 0.00 | 0.66 | 15.99 | 312.57 | 58.48 | 287.59 | 0.8618 | -457.0 | -402.2 | |
| 0.00 | 0.86 | 0.00 | 0.84 | 17.36 | 312.95 | 58.86 | 289.11 | 0.8666 | 312.0 | 299.0 | |
| 0.00 | 0.77 | 0.00 | 0.73 | 17.09 | 311.63 | 57.54 | 289.01 | 0.8551 | 234.0 | 222.0 | |
| 0.00 | 1.80 | 0.00 | 1.79 | 19.51 | 312.81 | 58.72 | 291.59 | 0.8684 | -331.0 | -319.9 | |
| 2.14 | 2.57 | 2.06 | 2.47 | 18.10 | 311.96 | 57.88 | 290.12 | 0.8594 | 286.8 | 238.2 | |
| 5.91 | 16.36 | 5.69 | 15.82 | 19.29 | 311.78 | 57.69 | 291.53 | 0.8596 | 584.7 | 223.5 | |
| 0.00 | 1.63 | 0.00 | 1.53 | 18.75 | 310.96 | 56.87 | 291.06 | 0.8519 | 454.0 | 353.8 | |
| 0.00 | 3.08 | 0.00 | 2.89 | 19.22 | 310.81 | 56.72 | 291.63 | 0.8513 | 602.0 | 480.4 | |
| 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. | |