| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.05 | 34.22 | 14.13 | 38.69 | 34.52 | 264.15 | 54.87 | 311.47 | 0.8996 | 66.2 | 115.6 | |
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back to the solar disc SDO HMI 2011-01-04 11:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.55 | 4.25 | 3.40 | 5.66 | 33.27 | 270.38 | 61.09 | 307.99 | 0.9302 | -397.2 | -204.7 | |
| 1.02 | 1.70 | 1.36 | 2.27 | 33.48 | 270.27 | 60.98 | 308.23 | 0.9301 | -277.0 | -99.9 | |
| 1.95 | 4.16 | 2.33 | 4.97 | 33.75 | 266.54 | 57.25 | 309.73 | 0.9110 | -312.8 | -378.5 | |
| 1.10 | 2.97 | 1.26 | 3.39 | 33.43 | 265.17 | 55.88 | 309.89 | 0.9024 | -271.0 | -223.3 | |
| 1.44 | 2.38 | 1.56 | 2.57 | 34.53 | 262.52 | 53.23 | 312.04 | 0.8905 | -278.6 | -436.4 | |
| 1.27 | 4.42 | 1.36 | 4.69 | 34.93 | 261.70 | 52.41 | 312.78 | 0.8870 | 404.4 | 362.9 | |
| 0.00 | 1.61 | 0.00 | 1.76 | 35.52 | 262.24 | 52.96 | 313.15 | 0.8923 | 337.0 | 214.5 | |
| 0.00 | 0.85 | 0.00 | 0.90 | 35.15 | 261.54 | 52.25 | 313.06 | 0.8869 | 200.0 | 59.7 | |
| 0.00 | 2.29 | 0.00 | 2.43 | 35.21 | 261.24 | 51.95 | 313.25 | 0.8853 | 507.0 | 376.7 | |
| 2.72 | 4.42 | 2.86 | 4.65 | 35.45 | 260.93 | 51.64 | 313.63 | 0.8844 | 530.2 | 504.7 | |
| 0.00 | 0.93 | 0.00 | 1.00 | 35.81 | 261.26 | 51.97 | 313.84 | 0.8876 | 179.0 | 123.9 | |
| 0.00 | 1.10 | 0.00 | 1.16 | 35.80 | 260.43 | 51.14 | 314.19 | 0.8828 | 359.0 | 308.5 | |
| 0.00 | 0.93 | 0.00 | 0.97 | 35.90 | 260.17 | 50.88 | 314.41 | 0.8817 | 375.0 | 340.3 | |
| 0.00 | 2.21 | 0.00 | 2.27 | 35.59 | 259.83 | 50.54 | 314.24 | 0.8784 | 607.0 | 458.4 | |
| 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. | |