| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.80 | 55.97 | 19.31 | 58.31 | 16.63 | 298.33 | 60.70 | 288.12 | 0.8804 | -160.0 | 31.4 | |
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back to the solar disc SDO HMI 2011-11-25 13:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.68 | 24.99 | 0.77 | 27.96 | 16.28 | 300.94 | 63.31 | 287.35 | 0.9004 | 123.6 | -103.1 | |
| 11.04 | -1.00 | 12.32 | -1.00 | 16.35 | 300.56 | 62.94 | 287.47 | 0.8977 | -559.5 | 999999 | |
| 3.17 | 3.94 | 3.44 | 4.27 | 15.60 | 299.81 | 62.18 | 286.73 | 0.8914 | -273.9 | -242.9 | |
| 0.00 | 1.03 | 0.00 | 1.07 | 16.00 | 298.40 | 60.77 | 287.36 | 0.8809 | 319.0 | 223.2 | |
| 0.00 | 1.11 | 0.00 | 1.13 | 16.36 | 297.45 | 59.82 | 287.90 | 0.8737 | -499.0 | -443.9 | |
| 0.00 | 3.51 | 0.00 | 3.51 | 16.77 | 297.05 | 59.42 | 288.43 | 0.8709 | -372.0 | -380.4 | |
| 0.00 | 2.91 | 0.00 | 2.86 | 16.66 | 296.38 | 58.76 | 288.40 | 0.8653 | 81.0 | 122.2 | |
| 0.00 | 1.28 | 0.00 | 1.24 | 16.73 | 295.88 | 58.26 | 288.57 | 0.8612 | 378.0 | 328.3 | |
| 0.00 | 0.68 | 0.00 | 0.67 | 17.41 | 296.16 | 58.54 | 289.30 | 0.8644 | 243.0 | 175.8 | |
| 0.00 | 0.86 | 0.00 | 0.83 | 17.60 | 295.79 | 58.16 | 289.58 | 0.8615 | 229.0 | 173.1 | |
| 0.00 | 0.68 | 0.00 | 0.65 | 16.75 | 295.36 | 57.73 | 288.67 | 0.8568 | 402.0 | 374.8 | |
| 0.00 | 1.37 | 0.00 | 1.31 | 17.52 | 295.27 | 57.65 | 289.58 | 0.8571 | 402.0 | 374.7 | |
| 2.91 | 3.77 | 2.78 | 3.59 | 17.74 | 295.21 | 57.58 | 289.84 | 0.8569 | 542.3 | 431.5 | |
| 0.00 | 6.50 | 0.00 | 6.16 | 17.28 | 294.98 | 57.35 | 289.35 | 0.8543 | 574.0 | 535.9 | |
| 0.00 | 2.23 | 0.00 | 2.05 | 17.15 | 293.95 | 56.32 | 289.38 | 0.8451 | -211.0 | -250.9 | |
| 0.00 | 1.11 | 0.00 | 1.01 | 17.72 | 293.32 | 55.70 | 290.17 | 0.8404 | -322.0 | -329.4 | |
| 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. | |