| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.48 | 325.29 | 34.91 | 201.78 | 27.82 | 44.64 | -29.06 | 45.61 | 0.6031 | -860.2 | -324.7 | |
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back to the solar disc SDO HMI 2011-11-10 16:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.66 | 27.07 | 50.45 | -23.26 | 40.90 | 0.5391 | -616.0 | -528.8 | |
| 0.00 | 1.38 | 0.00 | 0.85 | 30.72 | 48.34 | -25.37 | 38.44 | 0.5946 | -208.0 | -262.6 | |
| 0.00 | 1.81 | 0.00 | 1.13 | 31.92 | 47.64 | -26.07 | 37.69 | 0.6122 | -737.0 | -502.3 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 26.94 | 47.54 | -26.17 | 44.16 | 0.5665 | 739.0 | 609.2 | |
| 0.00 | 0.69 | 0.00 | 0.44 | 32.08 | 45.70 | -28.00 | 39.32 | 0.6302 | -701.0 | -616.0 | |
| 0.00 | 1.72 | 0.00 | 1.10 | 32.31 | 45.34 | -28.36 | 39.36 | 0.6353 | -586.0 | -427.6 | |
| 56.48 | 307.04 | 34.91 | 189.88 | 27.75 | 44.87 | -28.84 | 45.54 | 0.6003 | -1197.2 | -356.9 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 27.57 | 41.89 | -31.81 | 48.23 | 0.6289 | -775.0 | -669.2 | |
| 0.00 | 1.89 | 0.00 | 1.24 | 26.49 | 38.45 | -35.25 | 52.12 | 0.6568 | 782.0 | 645.0 | |
| 0.00 | 0.86 | 0.00 | 0.56 | 24.88 | 38.60 | -35.11 | 54.22 | 0.6454 | 658.0 | 542.6 | |
| 0.00 | 3.62 | 0.00 | 2.39 | 26.30 | 37.70 | -36.00 | 52.85 | 0.6635 | 520.0 | 387.5 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 30.37 | 35.22 | -38.49 | 49.12 | 0.7125 | 534.0 | 398.5 | |
| 0.00 | 1.38 | 0.00 | 0.99 | 30.45 | 33.49 | -40.22 | 50.02 | 0.7288 | 474.0 | 383.6 | |
| 0.00 | 1.12 | 0.00 | 0.80 | 30.25 | 33.54 | -40.16 | 50.23 | 0.7272 | 498.0 | 412.8 | |
| 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. | |